Updated on 2024/11/27

Information

 

写真a

 
YOSHIKAWA AKIMASA
 
Organization
Faculty of Science Department of Earth and Planetary Sciences Professor
International Center for Space and Planetary Environmental Science (Concurrent)
International Center for Space and Planetary Environmental Science (Concurrent)
School of Sciences Department of Earth and Planetary Sciences(Concurrent)
Graduate School of Sciences Department of Earth and Planetary Sciences(Concurrent)
Title
Professor
Contact information
メールアドレス
Tel
0928026240
Profile
理学研究院地球惑星科学部門を主担、国際宇宙惑星環境研究センター長を複坦としての研究・教育活動を行っている。  主たる研究分野は宇宙空間物理学であり、特に磁気圏-電離圏-中性大気-固体地球結合系での巨視的電磁流体波動(MHD波動)の相互作用・運動論的結合にについて理論的解析を中心とした領域で国際的な研究を展開しており、2005年より米国・EU域の共同研究者とプロジェクトチームを立ち上げ、現在は「全球Cowlingチャンネルの解明」のPrinciple Investigator(PI)として活動を行っている。  また、多くの学生、共同研究者とは上記理論的研究と相補的な観測的・解析的研究を展開しており、2013年6月より、全世界に72点の観測点を有する世界最大の地磁気観測網MAGDAS/CPMNプロジェクトのPIとしての活動も開始している。  副担である国際宇宙天気科学・教育センターでは、実質的な運営にも深く関わっており、ネットワーク観測事業を軸として国際的な研究活動を展開している。特に国連と連携した国際宇宙天気イニシアティブ事業に於いては、中核的な役割を果たしており、宇宙環境科学を基軸とした国際的なキャパシティ・ビルディング活動の拠点化を目指した活動を行っており、宇宙理学・宇宙工学・実用天文学等の分野融合した研究・教育活動を推進している。  関連する学術活動としては、地球電磁気・地球惑星圏学会の運営委員を、地球惑星科学関連48学協会を団体会員とする学術団体である地球惑星科学連合では、代議員(宇宙惑星科学分野選出)、災害環境対策委員などを務めており、全国共同利用研での各種委員も担当している。また、国際学術誌Earth, Planet and Spaceの運営委員に引き続き、編集委員も務めている。 最後に、現在展開している研究教育テーマを列挙する。 1. 「移動性局所性電離層対流による電離圏起源のオーロラ爆発現象の研究」 2. 「極域から磁気赤道域を結合する全球Cowlingチャンネルの実証的研究」 3. 「強磁場・弱電離気体系における学理の構築」 4.「MAGDAS/FM-CWネットワークデータを用いた太陽風・磁気圏・電離圏・地圏結合系の実証的的研究」 5. 下層大気変動に対する地磁気応答メカニズムの解明 6. 「光球-彩層-コロナ結合系に於ける太陽フレア励起の研究」 7.「国際宇宙天気キャパシティ・ビルディング事業の展開」

Research Areas

  • Natural Science / Theoretical studies related to particle-, nuclear-, cosmic ray and astro-physics

  • Natural Science / Space and planetary sciences

Degree

  • Doctor of Sciences

Research History

  • なし   

    なし

  • なし   

Research Interests・Research Keywords

  • Research theme: Studies on Poleward Intensification of aurora expansion caused by moving localized ionospheric flow

    Keyword: Composite system, mathematical sciences

    Research period: 2016.4 - 2020.3

  • Research theme: Studies on formation of Cowling channel connecting from polar to equatorial ionosphere

    Keyword: Composite system, mathematical sciences

    Research period: 2012.4 - 2017.5

  • Research theme: Mathematical science for composite system

    Keyword: Composite system, mathematical sciences

    Research period: 2010.3 - 2014.5

  • Research theme: Studies on the generation mechanism of substorm process by using global MI-coupling simulation

    Keyword: magnetosphere-ionosphere coupling, substorm, simulation, mathematical science

    Research period: 2008.5 - 2013.4

  • Research theme: Studies on the 3D-Cowling effect

    Keyword: 3D-current system, Hall current divergence, Sq, auroral electrojet

    Research period: 2007.5 - 2010.4

  • Research theme: Development of Magnetospheric Storm simulator

    Keyword: magnetospheric storm, global simulation, multi-sphere coupling

    Research period: 2005.3 - 2007.3

  • Research theme: magnetospheric physics in the multi-species ion and electron plasma system

    Keyword: herman magnetosphere, Jupiter magnetosphere, magnetosphere coupling, space reserch

    Research period: 2002.4 - 2011.3

  • Research theme: Understanding of the 3D-current system in the geospace

    Keyword: geospace, space weather, 3D-current system, global, CPMN, MAGDAS

    Research period: 2002.4 - 2010.3

  • Research theme: Complex physics in the solar terrestrial system

    Keyword: complex system, inter hierarchical coupling, magnetosphere-ionosphere coupling

    Research period: 2000.4 - 2011.3

  • Research theme: Interaction between MHD waves and ionosphere

    Keyword: Hall effect, magnetosphere-ionosphere coupling, energy balance, field-aligned current, inductive coupling

    Research period: 2000.4 - 2011.3

  • Research theme: Comparative study of geo-electromagnetic fields using FM-CW radar and MAGDS/CPMN data

    Keyword: HF-doppler, ionospheric electric field, ionospheric current system, ionospheric physics

    Research period: 2000.4 - 2010.3

Awards

  • 田中館賞

    2015.5   地球電磁気・地球惑星圏学会   磁気圏電離圏結合系の理論的研究

  • 第一回年九州大学総長賞

    2001.12   九州大学  

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    「The nature of reflection and mode conversion of MHD waves in the inductive ionosphere: Multistep mode conversion between divergent and rotational electric fields」
    九州大学の40歳以下の研究者のうち、国際的に高い評価を受けた研究をおこなったもの。全学より4名選出

Papers

  • Mid-latitude Ground Magnetic and Electric Field Responses Associated with SCW Development during Substorms Reviewed International journal

    #Hayashi, M., @A. Yoshikawa, A. Fujimoto

    Proceedings of the 8th International Conference on Space Science and Communication (IconSpace) 2023、Springer Proceedings in Physics (SPPHY)   303   63 - 74   2023.10

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    Language:Others   Publishing type:Research paper (international conference proceedings)  

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  • The Experience of Magnetovariational Sounding in the Arctic: the Laptev Sea Region Reviewed International journal

    S. S. Starzhinskii, V. M. Nikiforov, @A. Yoshikawa

    Izvestiya, Physics of the Solid Earth   56 ( 2 )   225 - 237   2020.3

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    Language:English   Publishing type:Research paper (scientific journal)  

    Abstract—We present the results of magnetovariational soundings at two sites (Tiksi Observatory and Kotelny Island in the Laptev Sea region of the Arctic) and their three-dimensional (3D) inversion using the ModEM program. In the models obtained by the inversion, the conductive heterogeneities are present in the regions of the both sites down to a depth of 200 km in the region of the observatory and 100 km beneath the Kotelny Island. The geoelectric heterogeneities in the model in the region of the observatory are most contrasting and voluminous, whereas beneath the island they are more localized. The correlation between the locations of these heterogeneities at both sites and the features of the geological and geophysical structure of the region is noted. It is shown that the applied algorithm of data processing eliminates the effect of the polar electrojet which provides the possibility to study the geoelectric structure of the region by magnetovariational method.

    DOI: 10.1134/S106935132002010X

  • Formation of a 3-D Oscillatory Current System Associated With Global High-Correlation Pi 2 Event: A Case Study Reviewed International journal

    @T. Uozumi, @A. Yoshikawa, S. Ohtani

    Journal of Geophysical Research: Space Physics   125 ( 1 )   2020.1

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    We present a typical example of the formation of a three-dimensional (3-D) oscillatory current system associated with a global high-correlation Pi 2 event. The time variation of the field-aligned current (FAC) density in the magnetosphere is estimated using multisatellite magnetic field data in the near-Earth plasma sheet (~10 RE, ~23 MLT). Pi 2 pulsations, which were accompanied with the development of the upward and downward FACs in the substorm current wedge, were observed at mid-latitude stations in the pre-midnight sector (20.6 and 22.6 MLT), and the periodicity of the FAC fluctuations was correlated with the estimated current-density fluctuations in the near-Earth plasma sheet. Compressional signals of the Pi 2 pulsation were observed by an equatorial ground station and a geosynchronous satellite located in the midnight sector (0.1 and 0.4 MLT). A detailed comparison of the Pi 2 waveforms, which were simultaneously observed on the ground and in the near-Earth magnetosphere, revealed high correlations between the fluctuations of the FACs and compressional pulses. These observations strongly suggest the formation of a 3-D oscillatory current system associated with the global high-correlation Pi 2 event. The sources of the oscillatory current system and compressional pulses were confirmed to be closely coupled with one another.

    DOI: 10.1029/2019JA026988

  • Seasonal dependence of semidiurnal equatorial magnetic variation during quiet and disturbed periods Reviewed

    Akiko Fujimoto, Akimasa Yoshikawa, Teiji Uozumi, Shuji Abe

    10th Anniversary International Conference on Solar-Terrestrial Relations and Physics of Earthquake Precursors, STRPEP 2019 E3S Web of Conferences   127   2019.11

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    The analysis of 20-year long-term semidiurnal lunar tidal variations gave the evidence that the semidiurnal variations are completely different between the magnetic quiet and disturbed periods. This is the first time that the seasonal dependence of disturbance-time semidiurnal variation has been provided from the analysis of the EE-index. We found the Kp dependence of semidiurnal variation: For full and new moon phase, counter troughs are amplified during disturbance time, possibly related to disturbance dynamo. For all moon phase, there are positive enhancements in dawn and strong depressions after sunset, resulting from the penetration of polar electric filed. For Seasonal dependence, semidiurnal variations are divided to three seasonal groups, and characterized as deep trough, enhanced crest and weak structure for D-solstice, Equinoxes and J-solstice, respectively. There is no significant longitudinal difference between Ancon and Davao, except for the amplitude of semidiurnal variations. The deep troughs occur during D-solstice and the enhanced crests during Equinoxes, at both Ancon and Davao.

    DOI: 10.1051/e3sconf/201912702025

  • Features of horizontal magnetic field intensity over northern island of Malaysia Reviewed International journal

    R Umar, SF Natasha, SSN Aminah, KN Juhari, MH Jusoh, NSA Hamid, MH Hashim, ZM Radzi, AN Ishak, SN Hazmin, WZAW Mokhtar, MKA Kamarudin, H Juahir, A Yoshikawa

    Indian Journal of Physics   93 ( 5 )   553 - 564   2019.5

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    Language:English  

    Magnetic Data Acquisition System (MAGDAS) is a magnetometer initiated by the International Center for Space Weather Science and Education in Kyushu University, Japan, to study space weather. The latest of real-time Magnetic Data Acquisition System/Circum-pan Pacific Magnetometer Network was successfully installed at the East Coast Environmental Research Institute in Universiti Sultan Zainal Abidin, Terengganu, Malaysia, by Kyushu University. This is the fifth magnetometer under the MAGDAS network (geographic latitude and longitude: 5.23°, 103.04° and geomagnetic latitude and longitude: − 4.21°, 175.91°). In this study, the results of data plot obtained at Terengganu (TRE) station were shown to have reliable patterns of geomagnetic elements. The amplitude variations for each component were also proximate with other stations and a standard model. This study compared MAGDAS-II data for the H component with solar wind data (input energy, IMF, dynamic pressure and speed).

    DOI: 10.1007/s12648-018-1318-x

  • Modeling Geomagnetically Induced Currents in Australian Power Networks Using Different Conductivity Models Reviewed International journal

    R. A. Marshall, L. Wang, G. A. Paskos, G. Olivares-Pulido, T. Van Der Walt, C. Ong, D. Mikkelsen, G. Hesse, B. McMahon, E. Van Wyk, G. Ivanovich, D. Spoor, C. Taylor, A. Yoshikawa

    Space Weather   7 ( 5 )   727 - 756   2019.4

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    Space weather manifests in power networks as quasi-DC currents flowing in and out of the power system through the grounded neutrals of high-voltage transformers, referred to as geomagnetically induced currents. This paper presents a comparison of modeled geomagnetically induced currents, determined using geoelectric fields derived from four different impedance models employing different conductivity structures, with geomagnetically induced current measurements from within the power system of the eastern states of Australia. The four different impedance models are a uniform conductivity model (UC), one-dimensional n-layered conductivity models (NU and NW), and a three-dimensional conductivity model of the Australian region (3DM) from which magnetotelluric impedance tensors are calculated. The modeled 3DM tensors show good agreement with measured magnetotelluric tensors obtained from recently released data from the Australian Lithospheric Architecture Magnetotelluric Project. The four different impedance models are applied to a network model for four geomagnetic storms of solar cycle 24 and compared with observations from up to eight different locations within the network. The models are assessed using several statistical performance parameters. For correlation values greater than 0.8 and amplitude scale factors less than 2, the 3DM model performs better than the simpler conductivity models. When considering the model performance parameter, P, the highest individual P value was for the 3DM model. The implications of the results are discussed in terms of the underlying geological structures and the power network electrical parameters.

    DOI: 10.1029/2018SW002047

  • Global response of Magnetic field and Ionosonde observations to intense solar flares on 6 and 10 September 2017 Reviewed International journal

    A Fujimoto, @A Yoshikawa, A Ikeda

    E3S Web of Conferences   ( 62 )   2018.11

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    Intense X-ray fluxes during solar flares are known to cause enhanced ionization in the Earth’s ionospheric D, E and F region. This sudden change of ionospheric electron density profile is serious problem to radio wave communication and navigation system. The ground magnetograms often record the sudden change in the sunlit hemisphere during the enhanced X-ray flux, due to the sudden increase in the global ionospheric current system caused by the flare-induced enhanced ionospheric conductivity. These geomagnetic field disturbances are known as ‘‘solar flare effects’’ (SFEs) or geomagnetic crochets [Campbell, 2003]. The typical SFE is increase variation on the equatorial magnetic data. On Ionosonde observation during solar flare event, the High-Frequency (HF) radio wave blackout is often detected in ionogram due to the sudden disturbance in ionosphere. Two intense X-class solar flares occurred on 6 and 10 September 2017. We investigated the magnetic field and Ionosonde responses to the intense solar flare events. Dayside magnetic field variations sudden increased due to the ionospheric disturbance resulting from solar flare. There is no response in night side magnetometer data. The magnitude of SFE (magnetic field) is independent of solar flare x-ray magnitude. We found HF radio wave blackout in ionogram at dayside Ionosonde stations. The duration of blackout is dependent of latitude and local time of Ionosonde stations. There is the different feature of ionogram at night side.

    DOI: 10.1051/e3sconf/20186201007

  • Schumann resonance parameters at Kuju station during solar flares Reviewed International journal

    A Ikeda, @T Uozumi, @A Yoshikawa, A Fujimoto, @S Abe

    E3S Web of Conferences   ( 62 )   2018.11

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    We examined the Schumann resonance (SR) at low-latitude station KUJ by comparing with solar X-ray flux and solar proton flux at a geostationary orbit. For intense solar activity in October-November 2003, the reaction of the SR frequency to X-ray enhancement and SPEs was different. The SR frequency in H component increased at the time of the Xray enhancement. The response of SR seems to be caused by the increase of the electron density in the ionospheric D region which ionized by the enhanced solar X-ray flux. In the case of the SPEs, the SR frequency in D component decreased with enhancement of solar proton flux. We suggest that the SPEs caused the decrease of altitude on the ionopheric D region at high-latitude region, and the SR frequency decreased.

    DOI: 10.1051/e3sconf/20186201012

  • Monitoring of Space and Earth electromagnetic environment by MAGDAS project Collaboration with IKIR-Introduction to ICSWSE/MAGDAS project Invited Reviewed International journal

    @Akimasa Yoshikawa, @Akiko Fujimoto, @Akihiro Ikeda, @Teiji Uozumi, @Shuji Abe

    E3S Web of Conferences   20   2017.10

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    For study of coupling processes in the Solar-Terrestrial System, International Center for Space Weather Science and Education (ICSWSE), Kyushu University has developed a real time magnetic data acquisition system (the MAGDAS project) around the world. The number of observational sites is increasing every year with the collaboration of host countries. Now at this time, the MAGDAS Project has installed 78 real time magnetometers-so it is the largest magnetometer array in the world. The history of global observation at Kyushu University is over 30 years and number of developed observational sites is over 140. Especially, Collaboration between IKIR is extended back to 1990's. Now a time, we are operating Flux-gate magnetometer and FM-CW Radar. It is one of most important collaboration for space weather monitoring. By using MAGDAS data, ICSWSE produces many types of space weather index, such as EE-index (for monitoring long tern and shot term variation of equatorial electrojet), Pc5 index (for monitoring solar-wind velocity and high energy electron flux), Sq-index (for monitoring global change of ionospheric low and middle latitudinal current system), and Pc3 index (for monitoring of plasma density variation at low latitudes). In this report, we will introduce recent development of MAGDAS/ICSWSE Indexes project and topics for new open policy for MAGDAS data will be also discussed.

    DOI: 10.1051/e3sconf/20172001013

  • Application of a global magnetospheric-ionospheric current model for dayside and terminator Pi2 pulsations Reviewed International journal

    S. Imajo, @Akimasa Yoshikawa, @T. Uozumi, Shin Ohtani, A. Nakamizo, P. J. Chi

    Journal of Geophysical Research   122 ( 8 )   8589 - 8603   2017.8

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    Pi2 magnetic oscillations on the dayside are considered to be produced by the ionospheric current that is driven by Pi2-associated electric fields from the high-latitude region, but this idea has not been quantitatively tested. The present study numerically tested the magnetospheric-ionospheric current system for Pi2 consisting of field-aligned currents (FACs) localized in the nightside auroral region, the perpendicular magnetospheric current flowing in the azimuthal direction, and horizontal ionospheric currents driven by the FACs. We calculated the spatial distribution of the ground magnetic field produced by these currents using the Biot-Savart law in a stationary state. The calculated magnetic field reproduced the observational features reported by previous studies: (1) the sense of the H component does not change a wide range of local time sectors at low latitudes, (2) the amplitude of the H component on the dayside is enhanced at the equator, (3) the D component reverses its phase near the dawn and dusk terminators, (4) the meridian of the D component phase reversal near the dusk terminator is shifted more sunward than that near the dawn terminator, and (5) the amplitude of the D component in the morning is larger than that in the early evening. We also derived the global distributions of observed equivalent currents for two Pi2 events. The spatial patterns of dayside equivalent currents were similar to the spatial pattern of numerically derived equivalent currents. The results indicate that the oscillation of the magnetospheric-ionospheric current system is a plausible explanation of Pi2s on the dayside and near the terminator.

    DOI: 10.1002/2017JA024246

  • A proposal on the study of solar-terrestrial coupling processes with atmospheric radars and ground-based observation network Reviewed

    Toshitaka Tsuda, Mamoru Yamamoto, Hiroyuki Hashiguchi, Kazuo Shiokawa, Yasunobu Ogawa, Satonori Nozawa, Hiroshi Miyaoka, @Akimasa Yoshikawa

    Radio Science   51 ( 9 )   1587 - 1599   2016.9

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    The solar energy can mainly be divided into two categories: the solar radiation and the solar wind. The former maximizes at the equator, generating various disturbances over a wide height range and causing vertical coupling processes of the atmosphere between the troposphere and middle and upper atmospheres by upward propagating atmospheric waves. The energy and material flows that occur in all height regions of the equatorial atmosphere are named as “Equatorial Fountain.” These processes from the bottom also cause various space weather effects, such as satellite communication and Global Navigation Satellite System positioning. While, the electromagnetic energy and high-energy plasma particles in the solar wind converge into the polar region through geomagnetic fields. These energy/particle inflow results in auroral Joule heating and ion drag of the atmosphere particularly during geomagnetic storms and substorms. The ion outflow from the polar ionosphere controls ambient plasma constituents in the magnetosphere and may cause long-term variation of the atmosphere. We propose to clarify these overall coupling processes in the solar-terrestrial system from the bottom and from above through high-resolution observations at key latitudes in the equator and in the polar region. We will establish a large radar with active phased array antenna, called the Equatorial Middle and Upper atmosphere radar, in west Sumatra, Indonesia. We will participate in construction of the EISCAT_3D radar in northern Scandinavia. These radars will enhance the existing international radar network. We will also develop a global observation network of compact radio and optical remote sensing equipment from the equator to polar region.

    DOI: 10.1002/2016RS006035

  • An application of the finite length Cowling channel model to auroral arcs with longitudinal variations Reviewed International journal

    R. Fujii, O. Amm, Heikki Antero Vanhamaki, @Akimasa Yoshikawa, A. Ieda

    Journal of Geophysical Research   117 ( 11 )   2012.12

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    A physical process for the latitudinal motion of an auroral arc based on the four-side bound Cowling channel model is proposed. Assuming that an upward field-aligned current (FAC) is associated with the auroral arc that forms a Cowling channel with finite lengths not only latitudinally but also longitudinally and that the upward FAC region is primarily embedded in a purely northward electric field, the primary Hall current driven by the northward electric field accumulates positive excess charges at the eastern edge of the channel and negative charges at the western edge for a perfect or partial Cowling channel with a nonzero Cowling efficiency. The charges produce a westward secondary electric field, indicating that a westward electric field can thus be produced by a purely northward primary electric field. This secondary electric field moves the arc with its magnetospheric source drifting together with the magnetospheric plasmas equatorward and simultaneously produces the electric field outside the channel that moves the downward FAC equatorward of the upward FAC region equatorward together with the upward FAC. Thus, the whole 3-D current system is expected to move equatorward as often observed in the afternoon auroral zone.

    DOI: 10.1029/2012JA017953

  • Ionospheric Joule heating and Poynting flux in quasi-static approximation Reviewed International journal

    Heikki Antero Vanhamaki, @Akimasa Yoshikawa, O. Amm, R. Fujii

    Journal of Geophysical Research   117 ( 8 )   2012.1

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    Energy flow is an important aspect of magnetosphere-ionosphere coupling. Electromagnetic energy is transported as Poynting flux from the magnetosphere to the ionosphere, where it is dissipated as Joule heating. Recently Richmond derived an "Equipotential Boundary Poynting Flux (EBPF) theorem", that the Poynting flux within a flux tube whose boundary is an equipotential curve is dissipated inside the ionospheric foot point of the flux tube. In this article we study Richmond's EBPF theorem more closely by considering the curl-free and divergence-free parts as well as the Hall and Pedersen parts of the ionospheric current system separately. Our main findings are that i) divergence-free currents are on average dissipationless, ii) the curl-free Pedersen current is responsible for the whole ionospheric Joule heating and iii) pointwise match between vertical Poynting flux and ionospheric Joule heating is broken by gradients of Hall and Pedersen conductances. Results i) and ii) hold when integrated over the whole ionosphere or any area bounded by an equipotential curve. The present study is limited to quasi-static phenomena. The more general topic of electrodynamic Joule heating and Poynting flux, including inductive effects, will be addressed in a future study.

    DOI: 10.1029/2012JA017841

  • A self-consistent synthesis description of magnetosphere-ionosphere coupling and scale-dependent auroral process using shear Alfvén wave Reviewed International journal

    @Akimasa Yoshikawa, O. Amm, Heikki Antero Vanhamaki, R. Fujii

    Journal of Geophysical Research   116 ( 8 )   2011.1

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    In order to correctly describe the dynamical behavior of the magnetosphere-ionosphere (MI) coupling system and the scale-dependent auroral process, we develop a synthesis formulation that combines the process of (1) the inverse Walen separation of MHD disturbance into parallel- and antiparallel-propagating shear Alfvén wave to the ambient magnetic field, (2) the shear Alfvén wave reflection process including (3) the scale-dependent electrostatic coupling process through the linearized Knight relation, (4) two-layer ionosphere model, and (5) dynamic conductance variations. A novel procedure that applies the inverse Walen relation to the incompressional MHD disturbances at the inner boundary of the MHD region enables to extract the component of the shear Alfvén wave incident to the ionosphere. The extracted incident electric field supplies an electromotive force for the generation of the MI coupling system, and the reflected electric field is generated such that it totally satisfies the synthesis MI-coupling equation. A three-dimensional ionospheric current system is represented by a two-layer model in which the Pedersen and the Hall current are confined in the separated layers, which are connected by field-aligned currents driven by the linear current-voltage relation between two layers. Hence, our scheme possibly reproduces two types of the scale-dependent MI-decoupling process of the perpendicular potential structure: due to the parallel potential drop at the auroral acceleration region and the other due to the parallel potential differences inside the ionosphere. Our newly formulation may be well suited for description of scale-dependent auroral process and mesoscale ionospheric electrodynamics interlocked with the dynamical development of magnetospheric processes.

    DOI: 10.1029/2011JA016460

  • Self-consistent formulation for the evolution of ionospheric conductances at the ionospheric e region within the M-I coupling scheme Reviewed International journal

    @Akimasa Yoshikawa, A. Nakamizo, O. Amm, Heikki Antero Vanhamaki, R. Fujii, Y. M. Tanaka, @T. Uozumi, @K. Yumoto, S. Ohtani

    Journal of Geophysical Research   116 ( 9 )   2011.1

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    We formulate the evolution of ionospheric conductivity in the framework of 3-D M-I coupling. Two important physical processes are taken into account. One is the ionization process by precipitating mono-energetic particles, which are accelerated by parallel-potential drops in the auroral acceleration region. The other process reflects the fact that part of field-aligned current (FAC) carried by electrons is closed with a perpendicular ionic current. Here, whereas the electric current is divergence-free, the divergence of electron current is finite. Therefore, the ionospheric electron density changes, and so does the conductivity. If the energy of electron precipitation is below ∼10 eV, this second process plays an important role in plasma transportation, production, and evacuation processes. In this case the density variation does not extend in space at the perpendicular electron velocity, but it rather moves at the ion perpendicular velocity. If the energy of electron precipitation is above ∼1 keV, in contrast, the precipitation has a nonlinear effect on plasma evolution. That is, the propagation speed of the density variation increases with increasing upward-FAC density, and the propagation takes place in the direction of the converging current into the upward FAC region. The Cowling effect on the plasma evolution process is crucially important. Our formulation is more general than the previous studies and is not limited to certain geometries, current component or interaction modes between the ionosphere and magnetosphere. It is therefore better-suited for describing the self-organized M-I coupling system, which evolves with current systems, conductivity, and magnetospheric processes interacting with each other.

    DOI: 10.1029/2011JA016449

  • Reformulation and energy flow of the Cowling channel Reviewed

    R. Fujii, O. Amm, @Akimasa Yoshikawa, A. Ieda, Heikki Antero Vanhamaki

    Journal of Geophysical Research   116 ( 2 )   2011.1

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    The question to which extent the divergence of the Hall current can be connected to the Pedersen current or to the closure current in the magnetosphere through field-aligned currents (FACs), that is, the Cowling channel process in the polar region, has long been debated but not fully understood. The present study reformulates the Cowling channel by introducing a two-layer model consisting of Hall and Pedersen conductivity layers with channel boundaries not only in the direction perpendicular to the channel but also in the direction along it. This new model enables us to better and more physically understand the connection between the Hall current, Pedersen current, and FAC. In particular, the finiteness of the channel along its direction enables us to understand that the primary nonzero electric field along the channel and FACs at the channel boundaries that faced each other in the channel direction carries the necessary energy for the Hall current to set up the secondary electric field from the magnetosphere. A case for a possible connection between the Pedersen and Hall currents is shown based on a polar current system derived from the Kamide-Richmond-Matsushita method. A more comprehensive analysis based on data is presented in the companion paper.

    DOI: 10.1029/2010JA015989

  • An empirical model of the quiet daily geomagnetic field variation Reviewed International journal

    Y. Yamazaki, @K. Yumoto, @M. G. Cardinal, B. J. Fraser, P. Hattori, Y. Kakinami, J. Y. Liu, K. J.W. Lynn, R. Marshall, D. McNamara, T. Nagatsuma, V. M. Nikiforov, R. E. Otadoy, M. Ruhimat, B. M. Shevtsov, K. Shiokawa, @S. Abe, @T. Uozumi, @Akimasa Yoshikawa

    Journal of Geophysical Research   116 ( 10 )   2011.1

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    An empirical model of the quiet daily geomagnetic field variation has been constructed based on geomagnetic data obtained from 21 stations along the 210 Magnetic Meridian of the Circum-pan Pacific Magnetometer Network (CPMN) from 1996 to 2007. Using the least squares fitting method for geomagnetically quiet days (Kp ≤ 2+), the quiet daily geomagnetic field variation at each station was described as a function of solar activity SA, day of year DOY, lunar age LA, and local time LT. After interpolation in latitude, the model can describe solar-activity dependence and seasonal dependence of solar quiet daily variations (S) and lunar quiet daily variations (L). We performed a spherical harmonic analysis (SHA) on these S and L variations to examine average characteristics of the equivalent external current systems. We found three particularly noteworthy results. First, the total current intensity of the S current system is largely controlled by solar activity while its focus position is not significantly affected by solar activity. Second, we found that seasonal variations of the S current intensity exhibit north-south asymmetry; the current intensity of the northern vortex shows a prominent annual variation while the southern vortex shows a clear semi-annual variation as well as annual variation. Thirdly, we found that the total intensity of the L current system changes depending on solar activity and season; seasonal variations of the L current intensity show an enhancement during the December solstice, independent of the level of solar activity.

    DOI: 10.1029/2011JA016487

  • A statistical investigation of the Cowling channel efficiency in the auroral zone Reviewed International journal

    O. Amm, R. Fujii, K. Kauristie, A. Aikio, @Akimasa Yoshikawa, A. Ieda, Heikki Antero Vanhamaki

    Journal of Geophysical Research   116 ( 2 )   2011.1

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    The Cowling channel mechanism describes the creation of a secondary polarization electric field at sharp conductance boundaries in the ionosphere due to excess charges for the case in which the release of these charges to the magnetosphere is fully or partially impeded. The secondary currents generated by the polarization electric field effectively modify the effective ionospheric conductivity inside the Cowling channel. While the Cowling mechanism is generally accepted for the equatorial electrojet, there is a long-standing discussion about the importance of this mechanism and its efficiency in the auroral electrojet. We present a statistical investigation that enables us to identify the most probable geospace conditions and MLT locations for a high Cowling efficiency. This investigation is based on more than 1600 meridional profiles of data from the Magnetometers-Ionospheric Radars-All-sky Cameras Large Experiment (MIRACLE) network in Scandinavia, in particular, ground magnetic field data from the International Monitor for Auroral Geomagnetic Effects (IMAGE) magnetometer network and electric field data from the Scandinavian Twin Auroral Radar Experiment (STARE) radar, supported with pointwise ionospheric conductance measurements from the European Incoherent Scatter (EISCAT) radar. We analyze the data in the framework of a 3-D ionospheric model, but our data set is filtered so that only electrojet-type situations are included so that the gradients of all measured quantities in longitudinal direction can be neglected. The analysis results in a steep peak of high Cowling channel efficiency probability in the early morning sector (0245-0645 MLT), with the largest probability around 0500 MLT and for medium and high geomagnetic activity. In agreement with an earlier single-event study by Amm and Fujii (2008), this indicates that the Cowling mechanism may be most effective in the early morning part of the central substorm bulge. Further, our analysis results in an almost monotonic increase of the probability of high Cowling channel efficiency with increasing geomagnetic activity.

    DOI: 10.1029/2010JA015988

  • Substorm convection and current system deduced from the global simulation Reviewed International journal

    @Tanaka T., @A. Nakamizo, @A. Yoshikawa , S. Fujita, H. Shinagawa, H. Shimazu, T. Kikuchi, K. Hashimoto

    J. Geophys. Res.   115 ( A05220 )   2010.12

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    DOI: 10.1029/2009JA014676

  • Alfvenic-coupling algorithm for global and dynamical magnetosphere-ionosphere coupled system Reviewed International journal

    @Yoshikawa A., H. Nakata, @A. Nakamizo, @T. Uozumi, M. Itonaga, S. Fujita, @K. Yumoto, and @T. Tanaka

    J. Geophys. Res.   115 ( A04211 )   2010.3

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    DOI: 10.1029/2009JA014924

  • A new magnetospherere- ionosphere coupling scheme for temporal and global magnetospheric MHD simulations Reviewed

    @Yoshikwa A., H. Nakata, @A. Nakamizo, @T. Uozumi, M. Itonaga, and @K. Yumoto

    Mem. Fac. Sci., Kyushu Univ., Ser. D, Earth & Planet.Sci.,Vol, XXXII, No2, 87-94   XXXII ( 2 )   2009.3

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  • A new index to monitor temporal and long-term variations of the equatorial electrojet by MAGDAS/CPMN real-time data EE-index Reviewed International journal

    @T. Uozumi, @K. Yumoto,@ K. Kitamura, @S. Abe, @Y. Kakinami, @M. Shinohara, @Akimasa Yoshikawa, @Hideaki Kawano, #T. Ueno, T. #Tokunaga, D. McNamara, J. K. Ishituka, S. L.G. Dutra, B. Damtie, V. Doumbia, O. Obrou, A. B. Rabiu, I. A. Adimula, M. Othman, M. Fairos, R. E.S. Otadoy

    Earth, Planets and Space   60 ( 7 )   785 - 790   2008.1

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    A new index, EE-index (EDst, EU, and EL), is proposed to monitor temporal and long-term variations of the equatorial electrojet by using the MAGDAS/CPMN real-time data. The mean value of the H component magnetic variations observed at the nightside (LT = 18-06) MAGDAS/CPMN stations along the magnetic equatorial region is found to show variations similar to those of Dst; we defined this quantity as EDst. The EDst can be used as a proxy of Dst for the real-time and long-term geospace monitoring. By subtracting EDst from the H component data of each equatorial station, ir is possible to extract the Equatorial Electrojet and Counter Electrojetcomponents, which are defined as EU and EL, respectively.

    DOI: 10.1186/BF03352828

  • Global features of Pi 2 pulsations obtained by independent component analysis Reviewed International journal

    #Terumasa Tokunaga, #Hiroko Kohta, @Akimasa Yoshikawa, @Teiji Uozumi, @Kiyohumi Yumoto

    Geophysical Research Letters   34 ( 14 )   2007.7

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    Ground Pi 2 pulsations are mixtures of several components reflecting (1) propagations of fast and shear Alfvén wave, (2) resonances of plasmaspheric/magnetospheric cavity and magnetic field lines, and (3) tansformations to ionospheric current systems. However, it has been unclear how they coupled with each other and how their signals are distributed at different latitudes. The present work is intended to pilot the future possibilities whether we can identify the global system of Pi 2 pulsations by Independent Component Analysis (ICA). We have successfully decomposed an isolated Pi 2 event on a quiet day observed at the CPMN stations into two components. One was the global oscillation that occurs from nightside high to equatorial latitudes with the common waveform and has an amplitude maximum at nightside high latitude. Another component was localized at nightside high latitudes. Its amplitudes were quite weak at low latitudes, but were enhanced near dayside dip equator.

    DOI: 10.1029/2007GL030174

  • Techniques to investigate the ionospheric effect on ULF waves Reviewed International journal

    Obana, A. Yoshikawa, J.V. Olson, R.J. Morris, B.J. Fraser, S.I. Solovyev, and K. Yumoto

    Proceeding of The fifth Workshop on Applications of Radio Science (WARS) obart Australia, on Feb. 18-20, 2004   2004.2

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  • The Diagnosis of the Plasmapause by Ground Magnetometer Network Observation at Multiple Local Times Reviewed

    Abe S., K. Yumoto, H. Kawano, A. Yoshikawa, Y. Obana, S. I. Solovyev, D.G. Baishev, J.V. Olson, E.W. Worthington, and the Circum-pan Pacific Magnetometer Network Group

    International Symposium on Information Science and Electrical Engineering 2003, Nov.13-14, 2003, ACROS Fukuoka, Fukuoka, Japan   2003.11

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  • Plasma Distribution in the Low-L part of the Plasma sphere during Magnetic Storms Reviewed

    #Takasaki S., @H. Kawano,# Y. Tanaka, @A. Yoshikawa, M. Seto, M. Iizima, and@ K. Yumoto

    International Symposium on Information Science and Electrical Engineering 2003, Nov.13-14, 2003, ACROS Fukuoka, Fukuoka, Japan   2003.11

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  • Inegrated Analysis of Coordinated Ground Magnetic Field Data for Space Weather Study Reviewed

    Yoshikawa A., H. Kohta, M.I tonaga, T. Uozumi, K. Yumoto

    International Symposium on Information Science and Electrical Engineering 2003, Nov.13-14, 2003, ACROS Fukuoka, Fukuoka, Japan   2003.11

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  • Environment Factors of PC 4 Amplitudes Observed at the CPMN Stations Reviewed

    Obana Y., A. Yoshikawa, J.V. Olson, R.J. Morris, B.J. Fraser, S.I. Solovyev and K. Yumoto

    International Symposium on Information Science and Electrical Engineering 2003, Nov.13-14, 2003, ACROS Fukuoka, Fukuoka, Japan   2003.11

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  • Quasi-periodic Substorms during Recovery Phase of Magnetic Storm for Space Weather Study Reviewed

    Kitamura. K., H. Kawano, S. Ohtani, A. Yoshikawa, K. Yumoto, and the Circum-pan Pacific Magnetometer Network Group

    2003.11

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  • On the energy of the poloidal magnetic field near the ionosphere Reviewed International journal

    @Yoshikawa, A., M. Itonaga and @K. Yumoto

    Advances in Polar Upper Atmospheric Research   2002.1

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  • A study on the generation of field-aligned current in the magnetosphere Reviewed

    @M. Itonaga, @A. Yoshikawa, @K. Yumoto, S. Fujita and H. Nakata

    Mem. Fac. Sci., Kyushu Univ., Ser. D, Earth and Planet. Sci.   2000.1

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  • One-dimensional transient response of the inner magnetosphere at the magnetic equator, 2. analysis of waveforms Reviewed International journal

    @M. Itonaga, @Akimasa Yoshikawa, @K. Yumoto

    Earth, Planets and Space   49 ( 1 )   49 - 68   1997.2

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    Under a model of altitude distribution of the Alfvén speed VA, one-dimensional transient response of the inner magnetosphere at the magnetic equator to earthward propagating impulse- and step-like MHD disturbances is considered. The waveforms of transient compressional oscillations due to these disturbances at some L shells are directly simulated by a numerical inversion of the Laplace transform with orthonormal Laguerre functions. The present paper concentrates on the analysis of waveforms. Then, it is verified that the compressional oscillations are due to the poles of the system under consideration. The oscillation arising from the cavity resonance all over the inner magnetosphere is most dominant. However, its amplitude becomes smaller as the characteristic time scale T of an incident disturbance grows large, and it is negligibly small for T greater than several times of eigenperiod of the resonance. On the other hand, when T is relatively small (e.g., T £10 s), the oscillations due to the cavity resonances trapped around the trough in VA are outstanding. It is also found that the relative phase between the cavity-mode oscillations all over the inner magnetosphere at the earth's surface and another L shell increases monotonically with L when the inner magnetosphere has no strong gradient or a strong positive gradient of VA at its outer boundary. However, the relative phase is nearly zero and nearly 180 inside and outside a specific L shell, respectively, when the inner magnetosphere has a strong negative gradient at its outer boundary. The one-dimensional cavity-mode type resonance of the inner magnetosphere is certainly a cause of equatorial Pi2 pulsations. However, some constituents of the Pi2's may be not cavity-mode oscillations but quasi-steady-state oscillations forced by some damped sinusoidal waves incident on the outer boundary of the inner magnetosphere.

  • One-dimensional transient response of the inner magnetosphere at the magnetic equator, 1. transfer function and poles Reviewed International journal

    @M. Itonaga, @Akimasa Yoshikawa, @K. Yumoto

    Earth, Planets and Space   49 ( 1 )   21 - 48   1997.1

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    One-dimensional transient response of the inner magnetosphere at the magnetic equator is investigated using two models of altitude distribution of the Alfvén speed VA- The present paper concentrates on the transfer function of the system under consideration and its poles, which govern the transient response of the system. The poles, which are mathematical counterparts of the cavity resonances, appear owing to the inhomogeneity of VA and their locations depend on the altitude distribution of VA as well as the position of external source (or outer boundary of the inner magnetosphere). Even if there exists no strong Alfvén velocity gradient at the outer boundary, an observable cavity-mode oscillation in the Pi2 range can be excited because of the existence of a strong gradient of the plasmapause within the inner magnetosphere. However, the existence of a strong gradient at the outer boundary brings about a long-lived nature of the cavity-mode oscillation as well as calls some new poles into existence. While the surface of the solid earth forms the inner boundary at which the almost perfect reflection of wave takes place, the ionosphere is of secondary importance as a reflector of wave. The existence of the solid earth plays an essential role in the observability of the compressional oscillation arising from the cavity resonance all over the inner magnetosphere. The real part of each pole has a negative value, meaning that the cavity-mode oscillation decays with a damping factor of absolute value of the real part of the pole. Such a damping is primarily due to the leakage of energy through the outer boundary of the inner magnetosphere.

    DOI: 10.5636/jgg.49.21

  • The excitation of shear alfvén wave and the associated modulation of compressional wave in the inner magnetosphere Reviewed

    @M. Itonaga, @Akimasa Yoshikawa

    Earth, Planets and Space   48 ( 11 )   1451 - 1459   1996.6

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    Two basic but novel equations directly describing the generation of shear Alfvén and compressional waves in the inner magnetosphere filled with a cold magnetized plasma are derived. The shear Alfvén wave is characterized by the field-aligned current and the compressional wave by the compressional component of the magnetic field. Such a generation arises from the effects of inhomogeneous Alfvén speed and curvilinear field line. Around the magnetic equator, if the Alfvén speed is inversely proportional to a power of the geocentric distance, these effects have magnitudes of the same order and their signs are identical. Considered in the present study is a situation that the earthward propagating compressional wave is launched from a large scale oscillating current wedge centered at midnight and symmetric about the magnetic equator. Then, it is found that the field-aligned current excited around the equator by the compressional wave has opposite senses in direction in the northern and southern hemispheres, in the pro- and post-midnight sectors as well as just inside the plasmapause and in its surrounding regions. As a result of the excitation of shear Alfvén wave, two types of oscillations appear on a field line: One is a forced oscillation and the other is an eigenoscillation. Although a modulation of the compressional wave may be caused locally (or microscopically) around the equator by the eigenoscillation of field line, the modulation can be globally (or macroscopically) neglected. So far as the propagation along the source longitude (source-earth line) around the equator is concerned, the coupling between compressional and shear Alfvén waves can be almost neglected and so one-dimensional response of the inner magnetosphere around the equator plays a significant role in the compressional oscillation.

    DOI: 10.5636/jgg.48.1451

  • Effect of the ionospheric induction current on magnetohydrodynamic waves in the magnetosphere Reviewed International journal

    #Yoshikawa, @A., M. Itonaga and @T.-I.Kitamura

    Proceedings of the NIPR Symposium on Upper Atmosphere Physics   1995.1

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  • Interaction between hydromagnetic waves and the anisotropically conducting ionosphere Reviewed International journal

    @Itonaga, M., @T.-I.Kitamura and #A. Yoshikawa

    Journal of Geomagnetism and Geoelectricity   47 ( 5 )   459 - 474   1995.1

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  • On the coupled effect between the field aligned and ionospheric current Reviewed International journal

    #Yoshikawa, A., @M. Itonaga and @T.-I.Kitamura

    Proceeding of Eight International Symposium on Solar Terrestrial Physics, June 5-10, 1994, Sendai, Japan   1994.6

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  • Discrete spectral structure of low latitude and equatorial Pi2 pulsations, Reviewed International journal

    @Itonaga, M., and @A. Yoshikawa

    Journal of Geomagnetism and Geoelectricity, Vol.44, No.3, 253-259   44 ( 3 )   253 - 259   1992.1

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  • Mid-Latitude Study of Ionospheric Variation Over Iran Associated With Equatorial Ionization Anomaly (EIA), and Artificial Neural Networks Model Development

    Vazifehkhah Hafteh M., Mahmoudian A., Yoshikawa A., Girgis K.

    Space Weather   22 ( 11 )   2024.11

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    The ionosphere over Iran is located on the upper edge of equatorial ionization anomaly (EIA). The Equatorial Electrojet (EEJ) as the proxy of temporal evolution of the EIA is explored using the MAGDAS stations near the magnetic equator during quiet and active geomagnetic conditions. The possible impact of EIA on Total Electron Content (TEC) over Iran is investigated. Analyzing data from 140 stations over 7 months, it is found that EEJ influences TEC and its latitudinal penetration. During geomagnetically active days, EEJ's behavior and TEC's latitudinal variations are investigated. Diurnal EEJ patterns and counter electrojets (CEJ) are analyzed, alongside solar wind timing effects on EEJ and TEC using data from stations in Brazil, Peru, the Philippines, and Sri Lanka. Statistical correlations between maximum TEC and parameters extracted from the daily EEJ profile, including EEJ (Formula presented.), integrated EEJ (IEEJ), and IEEJ (Formula presented.) —highlight Iran's position at the EIA's upper edge, indicating high susceptibility to equatorial dynamics. In addition, the Rate of Total Electron Content Index (ROTI) has been analyzed under geomagnetic active conditions. The results demonstrate that ROTI exhibits good agreement with TEC in terms of latitude penetration and the detected gradient in TEC. Employing Artificial Neural Networks (ANN) for local TEC prediction, Iran is segmented into eight regions based on GNSS receiver distribution. Each region's ANN model, trained during the quiet geomagnetic condition, assesses predictability and accuracy. The ANN model demonstrates reliable local TEC forecasting and confirms the direct impact of equatorial dynamics on Iran's ionosphere.

    DOI: 10.1029/2024SW004032

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  • Critical analysis of the ULF power depression as a possible Tohoku earthquake precursor

    Pilipenko, VA; Martines-Bedenko, VA; Yoshikawa, A; Girgis, KM

    EARTHQUAKE SCIENCE   37 ( 5 )   407 - 414   2024.10   ISSN:1674-4519 eISSN:1867-8777

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    Among electromagnetic methods of short-term earthquake prediction, an approach is being actively developed based on the phenomenon of magnetic ultra-low-frequency (ULF) power depression occurring a few days before an earthquake. In particular, a nighttime geomagnetic power depression in the band 0.03–0.05 Hz was observed approximately 5 days before the catastrophic Tohoku 2011 earthquake. To verify the reliability of this method, we performed an extended analysis using data from magnetometer arrays JMA, MAGDAS, PWING, and INTERMAGNET. The selected stations included sites close to the epicenter (<300 km) and remote points (∼10000 km). The band-integrated spectral power of nighttime magnetic noise decreased significantly from March 6–9, several days before the earthquake. However, such variations occur simultaneously not only at nearby stations but also at distant stations. During this event, the ULF power depression was caused by low global geomagnetic activity, as evidenced by the planetary index SME. Thus, the depression of geomagnetic ULF noise cannot be considered a reliable short-term precursor.

    DOI: 10.1016/j.eqs.2024.06.003

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  • Prediction of Ionospheric Scintillations Using Machine Learning Techniques during Solar Cycle 24 across the Equatorial Anomaly

    Nasurudiin, S; Yoshikawa, A; Elsaid, A; Mahrous, A

    ATMOSPHERE   15 ( 10 )   2024.10   eISSN:2073-4433

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    Ionospheric scintillation is a pressing issue in space weather studies due to its diverse effects on positioning, navigation, and timing (PNT) systems. Developing an accurate and timely prediction model for this event is crucial. In this work, we developed two machine learning models for the prediction of ionospheric scintillation events at the equatorial anomaly during the maximum and minimum phases of solar cycle 24. The models developed in this study are the Random Forest (RF) algorithm and the eXtreme Gradient Boosting (XGBoost) algorithm. The models take inputs based on the solar wind parameters obtained from the OMNI Web database from the years 2010–2017 and Pc5 wave power obtained from the Bear Island (BJN) magnetometer station. We retrieved data from the Scintillation Network and Decision Aid (SCINDA) receiver in Egypt from which the S4 index was computed to quantify amplitude scintillations that were utilized as the target in the model development. Out-of-sample model testing was performed to evaluate the prediction accuracy of the models on unseen data after training. The similarity between the observed and predicted scintillation events, quantified by the R2 score, was 0.66 and 0.74 for the RF and XGBoost models, respectively. The corresponding Root Mean Square Errors (RMSEs) associated with the models were 0.01 and 0.01 for the RF and XGBoost models, respectively. The similarity in error shows that the XGBoost model is a good and preferred choice for the prediction of ionospheric scintillation events at the equatorial anomaly. With these results, we recommend the use of ensemble learning techniques for the study of the ionospheric scintillation phenomenon.

    DOI: 10.3390/atmos15101213

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  • A Comprehensive Classification and Analysis of Geomagnetic Storms Over Solar Cycle 24

    Shah, RARH; Hamid, NSA; Abdullah, M; Annuar, A; Sarudin, I; Radzi, ZM; Yoshikawa, A

    RESEARCH IN ASTRONOMY AND ASTROPHYSICS   24 ( 8 )   2024.8   ISSN:1674-4527 eISSN:2397-6209

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    A geomagnetic storm is a global disturbance of Earth's magnetosphere, occurring as a result of the interaction with magnetic plasma ejected from the Sun. Despite considerable research, a comprehensive classification of storms for a complete solar cycle has not yet been fully developed, as most previous studies have been limited to specific storm types. This study, therefore, attempted to present complete statistics for solar cycle 24, detailing the occurrence of geomagnetic storm events and classifying them by type of intensity (moderate, intense, and severe), type of complete interval (normal or complex), duration of the recovery phase (rapid or long), and the number of steps in the storm's development. The analysis was applied to data from ground-based magnetometers, which measured the Dst index as provided by the World Data Center for Geomagnetism, Kyoto, Japan. This study identified 211 storm events, comprising moderate (177 events), intense (33 events), and severe (1 event) types. About 36% of ICMEs and 23% of CIRs are found to be geoeffective, which caused geomagnetic storms. Up to four-step development of geomagnetic storms was exhibited during the main phase for this solar cycle. Analysis showed the geomagnetic storms developed one or more steps in the main phase, which were probably related to the driver that triggered the geomagnetic storms. A case study was additionally conducted to observe the variations of the ionospheric disturbance dynamo (Ddyn) phenomenon that resulted from the geomagnetic storm event of 2015 July 13. The attenuation of the Ddyn in the equatorial region was analyzed using the H component of geomagnetic field data from stations in the Asian sector (Malaysia and India). The variations in the Ddyn signatures were observed at both stations, with the TIR station (India) showing higher intensity than the LKW station (Malaysia).

    DOI: 10.1088/1674-4527/ad5b34

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  • Syntheses of Al<i>L</i>B<sub>14</sub>(<i>L</i>=Li or Na) crystals using alkali fluorides and its properties

    Hagiwara, T; Kouzu, K; Okada, S; Nomura, A; Yubuta, K; Shishido, T; Yoshikawa, A; Mori, T

    JAPANESE JOURNAL OF APPLIED PHYSICS   63 ( 8 )   2024.8   ISSN:0021-4922 eISSN:1347-4065

  • A RORE-dependent Intronic Enhancer in the IL-7 Receptor-a Locus Controls Glucose Metabolism via Vy4++y8T17 Cells

    Tani-ichi, S; Obwegs, D; Yoshikawa, A; Watanabe, H; Kitano, S; Ejima, A; Hatano, S; Miyachi, H; Cui, GW; Shimba, A; Abe, S; Hori, S; Kondoh, G; Sagar; Yoshikai, Y; Ikuta, K

    JOURNAL OF IMMUNOLOGY   213 ( 3 )   283 - 295   2024.8   ISSN:0022-1767 eISSN:1550-6606

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  • Machine learning techniques for estimation of Pc5 geomagnetic pulsations observed at geostationary orbits during solar cycle 23

    Pappoe J.A., Akimasa Y., Kandil A., Mahrous A.

    Journal of Atmospheric and Solar-Terrestrial Physics   260   2024.7   ISSN:13646826

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    Publisher:Journal of Atmospheric and Solar-Terrestrial Physics  

    Pc5 geomagnetic pulsations can accelerate electrons in the radiation belts, which can pose adverse threats to both astronauts and satellites in space. The estimation of Pc5 waves in space is crucial to radiation belt dynamics studies and will help mitigate these challenges. Here, we explore the advantages of the Feed-forward Neural Network (FFNN) and Random Forest (RF) algorithm for effective estimation of Pc5 geomagnetic pulsations observed in space at geostationary orbit during solar cycle 23. The dataset used in this study is the vector magnetic field measurements retrieved from the Geostationary Operational Environmental Satellite-10 (GOES-10) and the solar wind parameters: Bz and Vx component of the solar wind in the Geocentric Solar Ecliptic (GSE) coordinate system, proton density, flow pressure, and plasma beta obtained from the OMNI Web database during part of solar cycle 23. Pc5 geomagnetic pulsations were extracted from the toroidal component of the magnetic field time series using a bandpass Butterworth filter. The continuous wavelet transform (CWT) was utilized to study the characteristics of the extracted wave in the time-frequency domain for its validation. The validated Pc5 events were used as the target in the model's development, with the solar wind parameters as the inputs. In addition to the solar wind parameters, we included an attribute of the magnetic field time series as an input variable in the model. The dataset is carefully divided to ensure effective training and testing of the models. Finally, we trained both models using the same inputs and targets and explored their estimation abilities. The model was tested during the maximum, descending, and minimum phases of solar cycle 23. Both the FFNN and RF models have a similar estimation, with average cross-correlation score (R) values of 0.74 and 0.73 and corresponding average root mean squared error (RMSEs) of 0.16 nT and 0.67 nT, respectively. The model was deployed to investigate the response of Pc5 waves during three storm days in each testing year. The machine learning (ML) model outputs showed good coherence with the observed Pc5 waves. To validate the models, we studied the correlation between the estimated Pc5 events with the Kp index, and a good correlation was seen to exist between both events. This validates the good performance of the developed models. This work will aid in the study of radiation belt dynamics and the construction of electron depletion regions in the radiation belt.

    DOI: 10.1016/j.jastp.2024.106258

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  • Inner Radiation Belt Simulations During the Successive Geomagnetic Storm Event of February 2022

    Kirolosse M. Girgis, Tohru Hada, Akimasa Yoshikawa, Shuichi Matsukiyo, Abraham C.‐L. Chian, Ezequiel Echer

    Space Weather   22 ( 7 )   2024.7   ISSN:1542-7390 eISSN:1542-7390

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    Publishing type:Research paper (scientific journal)   Publisher:American Geophysical Union (AGU)  

    Abstract

    Starting from 29 January 2022, a series of solar eruptions triggered a moderate geomagnetic storm on 3 February 2022, followed subsequently by another. Despite the typically minimal impact of unintense storms on space technology, 38 out of the 49 Starlink satellites underwent orbital decay, re‐entering Earth's atmosphere. These satellite losses were attributed to enhanced atmospheric drag conditions. This study employs numerical simulations, utilizing our test particle simulation code, to investigate the dynamics of the inner radiation belt during the two magnetic storms. Our analysis reveals an increase in proton density and fluxes during the transition from the recovery phase of the first storm to the initial phase of the second, primarily driven by intense solar wind dynamic pressure. Additionally, we assess Single Event Upset (SEU) rates, which exhibit a 50% increase in comparison to initial quiet conditions.

    DOI: 10.1029/2023SW003789

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  • Growth of bulk β-Ga<sub>2</sub>O<sub>3</sub> crystals from melt without precious-metal crucible by pulling from a cold container

    Yoshikawa, A; Kochurikhin, V; Tomida, T; Takahashi, I; Kamada, K; Shoji, Y; Kakimoto, K

    SCIENTIFIC REPORTS   14 ( 1 )   14881   2024.6   ISSN:2045-2322

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    Kakimoto, K; Takahashi, I; Tomida, T; Kochurikhin, VV; Kamada, K; Nakano, S; Yoshikawa, A

    JOURNAL OF CRYSTAL GROWTH   629   2024.3   ISSN:0022-0248 eISSN:1873-5002

  • Longitudinal variations of ionospheric responses to the February and April 2023 geomagnetic storms over American and Asian sectors

    M. Arslan Tariq, Libo Liu, Munawar Shah, Yuyan Yang, Wenjie Sun, M. Ali Shah, Ruilong Zhang, Akimasa Yoshikawa

    Advances in Space Research   73 ( 6 )   3033 - 3049   2024.3   ISSN:0273-1177 eISSN:1879-1948

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    This paper investigates the ionospheric responses to the February and April 2023 geomagnetic storms using Total Electron Content (TEC) derived from the 10 Global Navigation Satellite System (GNSS) stations at the transition of low to mid-latitudes (Approx. 20 ∼ 30°N) across different longitudes in the American and Asian sectors. Significant variations in both sectors were recorded during the recovery phase and were mainly attributed to the Prompt Penetration Electric Field (PPEF), Disturbance Dynamo Electric Field (DDEF) and the thermospheric neutral composition changes as O/N2 depletion. Similarly, the American and Asian sectors showed TEC enhancements, primarily attributed to the PPEF, during the main phase of the April storm. The negative TEC variations during the recovery phase were observed due to the DDEF and changes in O/N2. In the Asian sector, positive and negative variations were recorded over Pakistan and China, respectively, during the main phase of the April storm. These variations resulted in high and low concentrations of the O/N2 ratio due to Magnetosphere-Ionosphere-Thermosphere coupling.

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  • A penalized motion detection model for extracting ionospheric echoes from low signal-to-noise ratio Ionogram video images

    Hiroshige Yuu, Fujimoto Akiko, Ikeda Akihiro, Abe Shuji, Yoshikawa Akimasa

    Proceedings of International Conference on Artificial Life and Robotics   29   1025 - 1031   2024.2   eISSN:21887829

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    Measuring the altitude distribution of electron density in the upper atmosphere, known as the ionosphere, using HighFrequency radio wave reflections often causes the low signal-to-noise ratio of ionospheric echoes due to radio frequency interference. We propose a model for converting low-signal-to-noise-ratio ionospheric echo video images (Ionogram) into noise-reduced images using image processing techniques, for tracing the ionospheric echoes from Ionogram. The proposed method consists of three processing parts: noise removal optimized for individual Ionogram images, extraction of ionospheric echoes by penalized background subtraction technique, and fine-tuning of ionospheric echo signals using a minimum spanning tree algorithm. The proposed model successfully reproduces fine Ionograms with 98% recall and 99% precision.

    DOI: 10.5954/icarob.2024.gs5-3

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  • Study of twisting of β-Ga2O3 crystals based on optical absorption and thermal conductivity anisotropy in the crystals grown by the Czochralski method

    Kakimoto, K; Takahashi, I; Tomida, T; Kochurikhin, VV; Kamada, K; Nakano, S; Yoshikawa, A

    JOURNAL OF CRYSTAL GROWTH   628   2024.2   ISSN:0022-0248 eISSN:1873-5002

  • Modelling of ULF Pc4 - Pc5 Pulsations with solar winds and geomagnetic storm for ULF earthquake precursor

    S. N.A. Syed Zafar, R. Umar, S. N. Hazmin, M. H. Jusoh, A. Yoshikawa, S. Abe, T. Uozumi, N. Z.M. Afandi, N. A. Mahiddin

    Advances in Space Research   73 ( 3 )   1814 - 1830   2024.2   ISSN:0273-1177 eISSN:1879-1948

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    The physical destruction and fatalities caused by earthquake events has compelled scientists to develop a method for predicting Earthquakes. It is almost impossible to detect earthquake events due to limited seismometer sensitivity; therefore, a non-seismological predictor was established by using the Ultra-Low Frequency (ULF) magnetic field as a potential earthquake precursor. ULF waves respond to magnetic activity that are transferred to Earth by solar winds, and become ultimately linked to earthquake events. The statistical correlation analysis is used between ULF Pc4 and Pc5 pulsation, solar wind parameters; IMF- component (Bz), solar wind speed (Vsw), solar wind pressure (Psw), solar wind input energy (IEsw), and near-equator geomagnetic storm (SYM/H ). Through a multiple regression modelled approach, the relationship between solar wind (SW) parameters (IMF-Bz, Vsw, Psw, IEsw) and near-equator geomagnetic index (SYM/H ) with ULF wave pulsations (Pc4 - Pc5) prior to an earthquake (EQ) event (magnitude, M = 3.0–6.0, depth, d < 100 km, epicentre distance from magnetometer station, r < 100 km) was determined. The solar wind and geomagnetic index parameters were obtained from OMNIWeb, where ULF pulsations (Pc4 - Pc5) were computed from the magnetometer Davao station (Philippines) (7.00oN, 125.40oE) located in a low latitude region. The ULF Pc5 band demonstrated the best fit for the ULF earthquake precursor model in relation to solar wind parameters (Vsw, Psw) and geomagnetic index (SYM/H ) with R2 and R2-adjusted values of (R2 =0.5011, R2-adj = 0.4940). The Vsw, Psw and SYM/H are major factors that contribute to the emission of ULF Pc5 prior to an earthquake, as determined by the stepwise regression method. This ULF earthquake precursor model is intended to address the problem seismologists face when predicting seismic events by assisting non-seismologists in locating the most effective EM-ULF wave bands in solar-terrestrial activities for detecting seismic events.

    DOI: 10.1016/j.asr.2023.10.036

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  • Mid-Latitude Ground Magnetic and Electric Field Responses Associated with SCW Development During Substorms

    Moe Hayashi, Akimasa Yoshikawa, Akiko Fujimoto

    Springer Proceedings in Physics   303   63 - 74   2024   ISSN:0930-8989 ISBN:9789819701414 eISSN:1867-4941

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    This study elucidates the development of the global three-dimensional current system from polar to equatorial regions during substorms. We extracted 50 cases from 1934 isolated substorms between 2006 and 2013. These 50 cases met two criteria: the electric field was calm for 1 h before the substorm, and clear electric field fluctuations were observed during substorm onset. We compared the 210 MM and mid-latitude magnetic field data to capture each event's distribution and temporal evolution of the substorm current wedge. Additionally, we captured the electric field response using the mid-latitude Paratunka station. The results revealed that the electric field amplitude was proportional to the SuperMAG aurora electrojet index magnitude (correlation coefficient = 0.67). In the central region of the substorm current wedge (SCW), predominantly westward electric fields were observed between the upward and downward field-aligned currents (FACs) (i.e., among 12 cases, wherein the observation points were at the center of the SCW, 10 showed westward electric fields). Moreover, a tendency for larger amplitudes of these westward electric fields was observed at the SCW center. This may reflect the projection of the primary potential formed by the charges injected into the upward and downward FAC regions on the ionosphere. Contrarily, a tendency for eastward electric fields was observed near the upward FAC of the SCW (i.e., among 24 cases, wherein the observation points were near or slightly inside the upward FAC, 14 showed eastward electric fields), which might be due to the twisting of the potential distribution associated with Hall polarization.

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  • Mean Solar Quiet Profiling of Geomagnetic Field H-Component for Langkawi Observatory in Solar Cycle-24

    Mohd Helmy Hashim, Mohamad Huzaimy Jusoh, Nurul Shazana Abdul Hamid, Nur Dalila Khirul Ashar, Zahira Mohd Radzi, Akimasa Yoshikawa

    Springer Proceedings in Physics   303   115 - 124   2024   ISSN:0930-8989 ISBN:9789819701414 eISSN:1867-4941

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    It is well known that the geomagnetic field exhibits consistent diurnal, seasonal, and solar cycle fluctuations. In this paper, the seasonal variations of the quiet day (Sq) of the geomagnetic field in the recent solar cycle were obtained to characterise the profiling behaviour of the geomagnetic field using the horizontal component (H-component) at Langkawi. Long-term data analysis was limited to Magnetic Data Acquisition System (MAGDAS) data from 2011, 2012, 2013, 2016, and 2018. It was discovered that the seasonal variations of the geomagnetic field component during Sq demonstrated Langkawi as an equatorial station where the horizontal component of the geomagnetic field, MSq(H), peaked during the equinox for most of the year. The value is comparable to the predicted value by the model of the International Geomagnetic Reference Field (IGRF) at 41,794 nT. This information can be used to improve the accuracy of geomagnetic models and predictions, as well as gain a better understanding of the regular variations of Sq in Langkawi, one of equatorial observatories in Southeast Asia.

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  • Geomagnetic Field Effects Over the Philippines During Strong Solar Flares in April 2022

    Zane Nikia C. Domingo, Ernest P. Macalalad, Akimasa Yoshikawa

    Springer Proceedings in Physics   303   83 - 92   2024   ISSN:0930-8989 ISBN:9789819701414 eISSN:1867-4941

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    During solar storms, conductivities in Earth’s ionospheric regions become more enhanced. This phenomenon produces effects on Earth’s current systems to which emissions of solar radiation largely contribute. Such radiations are analyzed as short timescale variations of the X-ray and EUV fluxes. This was observed for the two X- and three M-class solar flares on 17, 20, and 21 April 2022. All of which are geomagnetically quiet days with nominal Kp, Hp, and Dst indices. Magnetic responses were observed from magnetometers in the Philippines, located in the low-latitude (MUT) and near-equatorial (DAV) stations. These coexisting variations observed with Earth’s magnetic field are referred to as magnetic crochets. Measurements also showed that solar flare effects (Sfe) are more pronounced near the equator, where high conductivity generates more variations in Earth’s magnetic fields. Yet, the largest variations were not consistently observed for the strongest flares. At MUT, manifest variations in Hsfe (horizontal) and Zsfe (downward) were aligned with the X1.1 and M1.89 flares on day 17. Variations are generally homogeneous on days 20 and 21. Meanwhile, the largest variations at DAV were found during the M9.7 flare on day 21. It is inferred that increases in Hsfe remain greater than in Zsfe at both stations. Fluctuations in Hsfe are nonetheless more prolonged and heightened at DAV station.

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  • Daily geomagnetic variations under variable IMF/solar conditions and their connection with underground conductivity changes in Japan

    Emad M. Takla, Akimasa Yoshikawa, Teiji Uozumi, Kirolosse M. Girgis, A. Abdelkader

    Annals of Geophysics   67 ( 1 )   GM102 - GM102   2024   ISSN:1593-5213 eISSN:2037-416X

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    Fluctuations in Solar Wind (SW) and Interplanetary Magnetic Field (IMF) significantly affect the Geomagnetic Field (GF) measurements particularly during extreme space weather events. The current study investigates the variations of horizontal (H), vertical (Z) geomagnetic components under quiet and disturbed IMF and solar conditions as well as the effect of underground conductivity on the stationary geomagnetic measurements in Japan. Results of data analysis show that the response of the GF to IMF and solar parameters fluctuations is variable. The H- and Z-components were in good harmony with high visual correlation along a latitudinal profile across Japan during quiet times. On the other hand, during the disturbed times related to a Coronal Mass Ejection (CME) launched on 13 May 2005, the GF components varied with the disturbance of IMF and solar parameters. The H-components showed highly correlated variations with a significant reduction along the examined profile due to intensified ionospheric currents, while the Z-components recorded in the northern part of Japan showed abnormal daily variations pattern (positive daily variations) with an enhanced amplitude which is opposite to the normal behavior of daily variations recorded in the central and southern parts of Japan (negative daily variations). The observed enhanced and abnormal daily variation of Z-components in north Japan, which we consider a remarkable observation here, is possibly linked with underground conductivity anomaly in this region.

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  • Comparative Analysis of dB/dt Response Towards dH/dt as Proxies for Geomagnetically Induced Currents (GICs) in Low-Latitude Region

    Zainuddin A., Hairuddin M.A., Yoshikawa A., Hashim M.H., Abd Latiff Z.I., Mohd Yassin A.I., Jusoh M.H.

    IEEE Symposium on Wireless Technology and Applications, ISWTA   235 - 240   2024   ISSN:23247843 ISBN:9798350351354

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    Geomagnetic storms impact communication technology by disturbing the ionosphere, affecting GPS signal propagation, and causing navigation errors. These storms also induce voltages in long conductors such as communication cables, power lines, and pipelines through geomagnetically induced currents (GICs), leading to potential disruptions. This study addresses the gap in understanding geomagnetic field variations in low-latitudes, where infrastructure is less equipped for GIC disruptions. Furthermore, limitations in the availability of magnetic field components often necessitate the use of dB/dt as a GIC proxy for this region. This study aims to assess the relationship between the rate of change of the total magnetic field (dB/dt) and the horizontal magnetic field component (dH/dt) across different latitudes during the geomagnetic storm of 22-23 June 2015. Utilizing data from high (Narsarsuaq, Greenland), mid (Boulder, USA), and low (Alibag, India) latitude stations through correlation, cross-correlation, and linear regression analyses. The results reveal significant latitude dependent differences with strong correlations at mid and low latitudes. A strong linear correlation between dB/dt and dH/dt was observed, particularly at mid and low-latitudes. Cross-correlation analysis reveals synchronous responses at zero lag, indicating highly predictable relationships at lower latitude regions. Regression analysis demonstrates greater predictability of dB/dt and dH/dt at lower latitudes than at higher latitudes. These findings indicate that dB/dt is an effective proxy for GIC studies in low-latitude regions and enhance our understanding of geomagnetic impacts on infrastructure and highlight the importance of developing strategies tailored to different latitudes. This research contributes to the field by providing new insights into the use of dB/dt as a reliable measure for assessing GIC risks in low-latitude regions.

    DOI: 10.1109/ISWTA62130.2024.10651826

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  • A penalized motion detection model for extracting ionospheric echoes from low signal-to-noise ratio Ionogram video images

    Yuu Hiroshige, Akiko Fujimoto, Akihiro Ikeda, Shuji Abe, Akimasa Yoshikawa

    Proceedings of International Conference on Artificial Life and Robotics   1025 - 1031   2024   ISBN:9784991333705 eISSN:2435-9157

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    Measuring the altitude distribution of electron density in the upper atmosphere, known as the ionosphere, using High- Frequency radio wave reflections often causes the low signal-to-noise ratio of ionospheric echoes due to radio frequency interference. We propose a model for converting low-signal-to-noise-ratio ionospheric echo video images (Ionogram) into noise-reduced images using image processing techniques, for tracing the ionospheric echoes from Ionogram. The proposed method consists of three processing parts: noise removal optimized for individual Ionogram images, extraction of ionospheric echoes by penalized background subtraction technique, and fine-tuning of ionospheric echo signals using a minimum spanning tree algorithm. The proposed model successfully reproduces fine Ionograms with 98% recall and 99% precision.

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  • A penalized motion detection model for extracting ionospheric echoes from low signal-to-noise ratio Ionogram video images

    Hiroshige Y., Fujimoto A., Ikeda A., Abe S., Yoshikawa A.

    Proceedings of International Conference on Artificial Life and Robotics   1025 - 1031   2024   ISBN:9784991333705

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    Measuring the altitude distribution of electron density in the upper atmosphere, known as the ionosphere, using High- Frequency radio wave reflections often causes the low signal-to-noise ratio of ionospheric echoes due to radio frequency interference. We propose a model for converting low-signal-to-noise-ratio ionospheric echo video images (Ionogram) into noise-reduced images using image processing techniques, for tracing the ionospheric echoes from Ionogram. The proposed method consists of three processing parts: noise removal optimized for individual Ionogram images, extraction of ionospheric echoes by penalized background subtraction technique, and fine-tuning of ionospheric echo signals using a minimum spanning tree algorithm. The proposed model successfully reproduces fine Ionograms with 98% recall and 99% precision.

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  • A Case Study on Magnetic Signature of Ionospheric Disturbance Dynamo During an Intense Geomagnetic Storm on 6 August 2011

    Raja Adibah Raja Halim Shah, Nurul Shazana Abdul Hamid, Mardina Abdullah, Adlyka Annuar, Idahwati Sarudin, Zahira Mohd Radzi, Akimasa Yoshikawa

    Springer Proceedings in Physics   303   227 - 233   2024   ISSN:0930-8989 ISBN:9789819701414 eISSN:1867-4941

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    Coronal mass ejection (CME) occurs in the Sun’s corona that travels and reaches Earth’s magnetosphere, and it can trigger a geomagnetic storm. In this work, we presented a case study of a geomagnetic storm triggered by CME and observed the presence of ionospheric disturbance dynamo (Ddyn) at the equatorial station. Our analysis utilized CME data from the SOHO/LASCO CME Catalog, which contains information such as CME speed, solar source location, digital data, and the CME LASCO/C2 movies. The Disturbance storm time (Dst) index calculated from ground-based magnetometer data describes the geomagnetic storm phases. On the other hand, the variation of the Ddyn at the equatorial region was derived from the H component of Earth’s magnetic field. Four stations at the dip equator cover the longitude sectors of Asia (DAV and TIR) and Africa (AAB and ILR). This study shows that halo CME on 4 August 2011 triggered intense geomagnetic storms (Dst = − 115 nT) on 6 August 2011. During this geomagnetic storm, after a few hours of Dst peak, the signature of Ddyn can be clearly observed in two stations of the African sector (ILR and AAB), while no presence of Ddyn in two other stations (TIR and DAV) in the Asian sector.

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  • Bibliographic dataset of literature for analysing global trends and progress of the machine learning paradigm in space weather research

    Nur Dalila K.A., Mohamad Huzaimy Jusoh, Syamsiah Mashohor, Aduwati Sali, Akimasa Yoshikawa, Nurhani Kasuan, Mohd Helmy Hashim, Muhammad Asraf Hairuddin

    Data in Brief   51   109667   2023.12   ISSN:2352-3409 eISSN:2352-3409

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    The field of space weather research has witnessed growing interest in the use of machine learning techniques. This could be attributed to the increasing accessibility of data, which has created a high demand for investigating scientific phenomena using data-driven methods. The dataset, which is based on bibliographic records from the Web of Science (WoS) and Scopus, was compiled over the last several decades and discusses multidisciplinary trends in this topic while revealing significant advances in current knowledge. It provides a comprehensive examination of trends in publication characteristics, with a focus on publications, document sources, authors, affiliations, and frequent word analysis as bibliometric indicators, all of which were analysed using the Biblioshiny application on the web. This dataset serves as the document profile metrics for emphasising the breadth and progress of current and previous studies, providing useful insights into hotspots for projection research subjects and influential entities that can be identified for future research.

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  • Geomagnetic Storm Effects on the LEO Proton Flux During Solar Energetic Particle Events

    Kirolosse M. Girgis, Tohru Hada, Akimasa Yoshikawa, Shuichi Matsukiyo, Viviane Pierrard, Susan W. Samwel

    Space Weather   21 ( 12 )   2023.12   ISSN:1542-7390 eISSN:1542-7390

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    During a few solar energetic particle (SEP) events, solar protons were trapped within the geomagnetic field and reached the outer edge of the inner radiation belt. We reproduced this phenomenon by modeling the proton flux distribution at the Low‐Earth Orbit (LEO) for different geomagnetic conditions during solar particle events. We developed a three‐dimensional relativistic test particle simulation code to compute the 70–180 MeV solar proton Lorentz trajectories in low L‐shell range from 1 to 3. The Tsyganenko model (T01) generated the background static magnetic field with the IGRF (v12) model. We have selected three Dst index values: −7, −150, and −210 nT, to define quiet time, strong, and severe geomagnetic storms and to generate the corresponding inner magnetic field configurations. Our results showed that the simulated solar proton flux was more enhanced in the high‐latitude regions and more expanded toward the lower latitude range as long as the geomagnetic storm was intensified. Satellite observations and geomagnetic cutoff rigidities confirmed the numerical results. Furthermore, the LEO proton flux distribution was deformed, so the structure of the proton flux inside the South Atlantic Anomaly (SAA) became longitudinally extended as the Dst index decreased. Moreover, we have assessed the corresponding radiation environment of the LEO mission. We realized that, for a higher inclined LEO mission during an intense geomagnetic storm (Dst = −210 nT), the probability of the occurrence of the Single Event Upset (SEU) rates increased by 19% and the estimated accumulated absorbed radiation doses increased by 17% in comparison with quiet conditions.

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  • Wavelet Analysis for Automatic Detection of Pi-2 Pulsations during Substorm Onset Along the 210$^{\circ}$ Magnetic Meridian

    stephen Owino Omondi, Akimasa Yoshikawa, Teiji Uozumi, Yuki Obana, Moe Hayashi, Ayman Mohamed Mahrous

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  • Response of the geomagnetic horizontal component during solar events at RANAU station

    R. Umar, A. N. Dagang, N. S.I. Roslan, S. N.A.Syed Zafar, M. H. Jusoh, A. Yoshikawa, S. Abe, T. Uozumi

    Indian Journal of Physics   97 ( 13 )   3735 - 3744   2023.11   ISSN:0973-1458 eISSN:0974-9845

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    The solar surface activity produces space weather. Solar flares, coronal mass ejections (CMEs), and coronal holes are examples of solar activity phenomena that can compress the magnetosphere and cause a geomagnetic storm. Previous studies have indicated that these solar events disturb the near-Earth region. This study examines the behavior of the terrestrial geomagnetic field (H-component) and focuses on how the geomagnetic index (SYM/H) responds to solar wind parameters related to solar activity. Results showed that on September 9, 2017, a powerful geomagnetic storm (SYM/H = 200 nT) was observed that was brought on by powerful solar flares, CMEs, and coronal holes that happened on September 7 and 8, 2017, which generated significant alterations in the magnetosphere’s solar wind. On October 3 and 18, 2017, a moderate geomagnetic storm occurred, which resulted in a strong southbound situation with a high solar wind pressure that blasted high-density plasma due to CME associated with a coronal hole event into the magnetosphere. A moderate geomagnetic storm (SYM/H = 80 nT) on November 14, 2017, was triggered, according to findings, by a wider direction and high speed of CME with CIR event occurrence implies the accelerated large-scale solar wind that exacerbated the reconnection of the flowing interplanetary magnetic field into the inner magnetosphere. There were fewer injections of ions and energetic solar particles into the magnetosphere on December 12, 2017, which were thought to be a source of a weak geomagnetic storm(SYM/H = 49 nT). Additionally, the response of solar wind parameters and geomagnetic storm due to solar flare, CMEs and coronal holes to the modest drop in the ground geomagnetic field resulted in H-component reading at the RAN and DLT station. This study has contributed to the study of earthquake precursors in ultra-low frequency (ULF) emission with the effect of solar wind.

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  • Latitudinal dependence of Pc3-4 amplitudes across the dip equator along the 210° Magnetic Meridian

    Emad M. Takla, Sukir Maryanto, Akimasa Yoshikawa, Teiji Uozumi

    Annals of Geophysics   66 ( 3-4 )   2023.10   ISSN:1593-5213 eISSN:2037-416X

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    Studying Pc3-4 geomagnetic pulsations at equatorial and very low latitude regions is an important issue to understand their generation and propagation mechanisms. Pc3-4 amplitudes and their latitudinal dependency across the dip equator up to low latitudes (± 25°) are investigated using geomagnetic data simultaneously obtained by the MAGDAS/CPMN stations along the 210° Magnetic Meridian (MM) chain. Forty-five Pc3 events and thirty-two Pc4 events were selected for this study. Our results show a clear dependence of Pc3-4 amplitudes on geomagnetic latitudes. At the dip equator, most of the selected Pc3 events (~75%) showed an enhancement in amplitudes, while the rest (~25%) showed an attenuation. After that, the amplitudes decreased gradually by increasing latitudes. These results suggest mixed generation and propagation mechanisms for the equatorial and very low latitudes Pc3s. For better understanding, the Interplanetary Magnetic Field (IMF) and solar conditions are examined during the selected events. Results indicate that Pc3 events with enhanced amplitudes at dip equator are mainly occurred in daytime with no preference to IMF (magnitude and direction) and solar parameters, which suggests the ionospheric currents model as a generation and propagation mechanism for these events. While the attenuation observed in the other Pc3 events was associated with intense and abrupt fluctuations in the IMF and solar parameters, which in turn suggests the compressional wave model for generating these Pc3 events. On the other hand, these two models can explain the observed enhancement in the Pc4 amplitudes at the dip equator. Therefore, our obtained results clarified the origin of equatorial Pc3-4 pulsations.

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  • Robust least square modelling for selected daytime ionospheric parameters using geomagnetic observations at low latitudes

    S. A. Bello, M. Abdullah, N. S.A. Hamid, K. A. Yusuf, A. Yoshikawa, A. Fujimoto

    Advances in Space Research   72 ( 5 )   1615 - 1633   2023.9   ISSN:0273-1177 eISSN:1879-1948

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    The east–west electric field and the characterized horizontal configuration of the geomagnetic fields around the equatorial region cause electron redistribution in the ionospheric bottomside F- region. This electric field E in turn causes the flow of current in a narrow band around this region called Equatorial Electrojet (EEJ) current. The paper discusses the robust least square modelling approach for modelling some selected ionospheric profile parameters below the maximum height of the F2 layer from the computed EEJ values at Jicamarca station (12°S, 76.9 °W) in the Southern American sector and Ilorin (8.50°N, 4.68°E) in the West African sector. The modelled parameters are the maximum electron density, NmF2, the maximum height, hmF2 and the thickness parameter, B0 of the F2- layer which were then compared with the recent ionospheric international standard model (IRI-2016). The proposed new model for ionospheric parameters based on ground-based magnetic field data at specific locations improved the model fit for hmF2 with RMSE value ∼ 30 km, an improvement to the IRI hmF2 model options. In addition, the derived NmF2 model performs poorly as compared to the IRI URSI and CCIR model options for NmF2. The model was however able to reproduce the temporal changes in the NmF2, for example, the semi-annual variation in the observational NmF2 value. The specific local features that were not fully reproduced in the IRI B0 model options can be seen in the derived model.

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  • Examining Solar Flare Effects on Earth’s Ionosphere using Ground-Based Measurements

    Nurul Shazana Abdul Hamid, Raja Adibah Raja Halim, Idahwati Sarudin, Akimasa Yoshikawa, Akiko Fujimoto

    Sains Malaysiana   52 ( 8 )   2309 - 2322   2023.8   ISSN:0126-6039

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    This study investigated the simultaneous effects of solar flares (SFs) on both the D and E layers of Earth’s ionosphere. The analysis focused on the M and X-class SFs that occurred during the 24th solar cycle as these two classes of SFs are known to produce significant effects on Earth’s environment, particularly during the daytime period. The data utilized to detect the SF events in this study were ground-based magnetometer data from the equatorial regions. Effects of the selected SF events on the E layer were investigated based on the EUEL index constructed using the geomagnetic data. Meanwhile, the changes in the strength of radio VLF signals in the D ionospheric layer during the selected SF events were monitored using Sudden Ionospheric Disturbance (SID) data. Two case studies were performed which consisted of four SF events from a total of 23 events that were detected by geomagnetic data during the period of study. Further analysis on the selected SF events showed the common effects of SFs on the D layer, which is the increment on the VLF signal measured from the SID stations although a different response was detected in the EUEL index variations. This indicates that the VLF signal always shows an increment even though a decrement in the ionization of the E layer occurs as a result of the SF events. The difference in responses could be attributed to the distinct changes in electron density of both layers during the SF occurrence. Further studies are needed to elucidate the underlying mechanism responsible for this unique response, utilizing appropriate parameters such as total electron content, as well as the electron density data to thoroughly analyze the ionospheric response during SF events.

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  • Automatic detection of auroral Pc5 geomagnetic pulsation using machine learning approach guided with discrete wavelet transform

    Stephen Omondi, Akimasa Yoshikawa, Waheed K. Zahra, Ibrahim Fathy, Ayman Mahrous

    Advances in Space Research   72 ( 3 )   866 - 883   2023.8   ISSN:0273-1177 eISSN:1879-1948

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    Geomagnetic micropulsations are ultra-low frequency (ULF) signals observed in the magnetosphere as well as on the ground. These signals offer us an effective means to study the coupling of the magnetosphere-ionosphere processes in the space field. The most prominent observed type of such ULF waves is the Pc5 pulsations (with a frequency range of 1–7 mHz), known to have their maximum amplitude in the auroral oval. The low magnitude of Pc5 signals withstands against distinguishing them from the background noise. This study presents a machine learning approach for the automatic detection of geomagnetic Pc5 pulsations in the auroral zone using artificial neural networks (ANN) guided by discrete wavelet transform. Our ANN algorithm is validated and tested using a huge amount of datasets of auroral ground-based geomagnetic records from the Svalbard network during the two solar cycles 23 and 24. The wavelet-based coherence was used to determine the signal's consistency detected by the magnetometer stations of the Svalbard network; since they are sensitive to all sorts of space wave-related phenomena that left their footprint on the magnetic field time series. The Daubechies wavelet transform was utilized to classify and extract Pc5 signals from the artificial noise and the results are correlated with the geomagnetic pulsation records as detected by our ANN-based model. The ANN-based model showed a good correlation of an average of 98% for the different phases of the two studied solar cycles. The statistical regression analysis of the post-processed results yielded a high coefficient of determination of R2 = 0.9 and norms of residuals of 8–21 nT. The Pc5 events detected by the ANN-based algorithm during the two solar cycles showed a good correlation with the Kp index, which enables our model for space weather forecasting.

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  • Alex magnetometer and telluric station in Egypt: First results on pulsation analysis

    Stephen Omondi, Akimasa Yoshikawa, Waheed K. Zahra, Ibrahim Fathy, Ayman Mahrous

    Advances in Space Research   72 ( 3 )   711 - 725   2023.8   ISSN:0273-1177 eISSN:1879-1948

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    This study presents the first results of a newly installed ground-based station Alex Magnetometer and Telluric Station (AMTS) located in Alexandria governorate in Egypt (geographic coordinate: 30° 51.68′ N, 29° 33.67′ E). The station consists of a fluxgate digital magnetometer and a two-channel digital Long Period Telluric Recorder (LPTR). The station commenced operation on October 12th, 2021, by providing real-time data of the geoelectric and geomagnetic field components. Despite the low solar activity, the AMTS detected several signatures of geomagnetic storms. An illustrative case study was conducted on the strong geomagnetic storm of November 4th, 2021. The magnetic field components recorded by the station demonstrated a prompt increase synchronized with the Sudden Storm Commencement (SSC) captured by the ACE satellite arriving at 19:42 UT on November 3rd, 2021. The three geomagnetic field components recorded by the AMTS during the storm were consistent with the nearby INTERMAGNET stations. The digital fluxgate magnetometer's high sampling frequency (400 Hz) and the LPTR with a sampling frequency (1 Hz), allowed us to capture all ULF pulsations. The structural pearl-shaped Pc1 pulsation was obtained in all phases of the geomagnetic storm with repetitive oscillations in the main storm phase. The wavelet analysis of micropulsations recorded at AMTS showed a high coherence with the nearby-four INTERMAGNET stations demonstrating high data integrity and reliability. The magnetometer and telluric measurements at the AMTS will fill the data gap in the northern section of Africa and allow us to study geoelectric and geomagnetic micropulsations in the region.

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  • Quantum Calculation of Classical Kinetic Equations: A Novel Approach for Numerical Analysis of 6D Boltzmann-Maxwell Equations in Collisionless Plasmas Using Quantum Computing

    Hayato Higuchi, Juan William Pedersen, Akimasa Yoshikawa

    2023.6

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    A novel quantum algorithm for solving the Boltzmann-Maxwell equations of the
    6D collisionless plasma is proposed. The equation describes the kinetic
    behavior of plasma particles in electromagnetic fields and is known for the
    classical first-principles equations in various domains, from space to
    laboratory plasmas. We have constructed a quantum algorithm for a future
    large-scale quantum computer to accelerate its costly computation. This
    algorithm consists mainly of two routines: the Boltzmann solver and the Maxwell
    solver. Quantum algorithms undertake these dual procedures, while classical
    algorithms facilitate their interplay. Each solver has a similar structure
    consisting of three steps: Encoding, Propagation, and Integration. We conducted
    a preliminary implementation of the quantum algorithm and performed a parallel
    validation against a comparable classical approach. IBM Qiskit was used to
    implement all quantum circuits.

    DOI: 10.22541/essoar.168748458.80915597/v1

  • Simulation of Dawn‐To‐Dusk Electric Field in the Jovian Inner Magnetosphere via Region 2‐Like Field‐Aligned Current Reviewed

    Yuki Nakamura, Koichiro Terada, Chihiro Tao, Naoki Terada, Yasumasa Kasaba, François Leblanc, Hajime Kita, Aoi Nakamizo, Akimasa Yoshikawa, Shinichi Ohtani, Fuminori Tsuchiya, Masato Kagitani, Takeshi Sakanoi, Go Murakami, Kazuo Yoshioka, Tomoki Kimura, Atsushi Yamazaki, Ichiro Yoshikawa

    Journal of Geophysical Research: Space Physics   128 ( 6 )   2023.6   ISSN:2169-9380 eISSN:2169-9402

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    The presence of the dawn-to-dusk electric field of about 4 mV/m in the Jovian inner magnetosphere and its response to the enhancement of the solar wind dynamic pressure are still a mystery of the rotation-dominated Jovian magnetosphere. Previous studies have suggested that magnetosphere-ionosphere (M-I) coupling via Region 2-like (R2-like) field-aligned current (FAC) could be the origin of the Jovian dawn-to-dusk electric field. This study investigates whether the dawn-to-dusk electric field is formed from this scenario by using a Jovian ionosphere model and a two-dimensional ionospheric potential solver. Our results show that the dawn-dusk asymmetry in the ionospheric potential form even at middle latitudes and that the dawn-to-dusk electric field is induced in the inner magnetosphere if the electric potential is mapped to the magnetospheric equatorial plane. Around the Io orbit, the calculated electric field strength for the ionosphere without meteoroid influx is too large, 200 mV/m at dawn and 88 mV/m at dusk. One of the solutions is to consider long-lived meteoric ions in the Jovian ionosphere, which reduce the electric field strength to 15 mV/m at dawn and 12 mV/m at dusk. The model also shows that the electric field strength increases with the intensity of R2-like FAC, consistent with its response to the solar wind dynamic pressure observed by the Hisaki satellite.

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  • Interim analysis results of gut microbiota in patients with unresectable cholangiopancreatic cancer: SCRUM-Japan MONSTAR-SCREEN.

    Tezuka, S; Sakai, S; Yamashita, R; Horasawa, S; Fujisawa, T; Sawada, K; Yoshikawa, A; Nakamura, Y; Umemoto, K; Shibata, N; Ohtsubo, K; Itoh, S; Todaka, A; Sudo, K; Furukawa, M; Ikeda, M; Morizane, C; Ueno, M; Yoshino, T

    JOURNAL OF CLINICAL ONCOLOGY   41   733 - 733   2023.2   ISSN:0732-183X eISSN:1527-7755

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  • Predictors of Activities of Daily Living in Intensive Care Unit Survivors: A Propensity Score Matching Analysis

    Matsumoto Tsuyoshi, Yoshikawa Ryo, Harada Risa, Fujii Yasumitsu, Adachi Akimasa, Onishi Hirokazu, Imamura Ai, Takamiya Daiki, Makiura Daisuke, Komaki Kodai, Ogawa Masato, Sakai Yoshitada

    Progress in Rehabilitation Medicine   8   n/a   2023   eISSN:2432-1354

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    <b>Objectives: </b>Increased long-term impairment is common among intensive care unit (ICU) survivors. However, predictors of activities of daily living (ADL) in ICU survivors are poorly understood. We aimed to focus on the trajectory of physical function and explore the clinical variables that affect ADL at hospital discharge.

    <b>Methods: </b>We enrolled 411 patients admitted to the ICU from April 2018 to October 2020. Physical function was evaluated at ICU admission, ICU discharge, and hospital discharge. We assessed physical function (grip strength, arm and calf circumference, quadriceps thickness, and Barthel index). Patients were assigned to the high or low ADL group based on their Barthel index at discharge. Propensity score matching analysis was performed to minimize selection biases and differences in clinical characteristics.

    <b>Results: </b>After matching propensity scores, 114 of the 411 patients (aged 65±15 years) were evaluated. The high ADL group showed better physical function at ICU discharge and hospital discharge than the low ADL group. An overall decreasing trend in muscle mass was observed over time; the rates of decline were lower in the high ADL group than in the low ADL group. The cutoff values for relative changes in calf circumference and quadriceps thickness to predict high ADL were −7.89% (sensitivity: 77.8%, specificity: 55.6%) and −28.1% (sensitivity: 81.0%, specificity: 58.8%), respectively.

    <b>Conclusions: </b>The relative decreases in calf circumference and quadriceps thickness during hospitalization were lower in patients who maintained their ADL. Assessment of the trajectory of physical function can predict ADL status at hospital discharge among ICU survivors.

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  • Multiple Linear Regression on Ultra-Low Frequency (ULF) and Solar Wind for Earthquake Precursor Purposes

    Umar, R; Zafar, SNAS; Sabri, NH; Jusoh, MH; Dagang, AN; Yoshikawa, A; Abe, S; Uozumi, T

    JURNAL FIZIK MALAYSIA   44 ( 1 )   10013 - 10019   2023   ISSN:0128-0333

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  • Analysis of ULF Emissions in Solar Winds as A Short-Term Earthquake Precursor

    S. N.A.Syed Zafar, R. Umar, N. H. Sabri, M. H. Jusoh, A. Yoshikawa, S. Abe, T. Uozumi

    ASM Science Journal   18   2023   ISSN:1823-6782

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    The physical destruction and fatalities caused by earthquake events compelled scientists to develop Earthquake predictions. Due to limited seismometer sensitivity, it was impossible to detect earthquake events; therefore, non-seismological is established, which in Ultra Low Frequency (ULF). The study of electromagnetic waves (EM) in the Ultra-Low Frequency (ULF) range is a promising tool for investigating seismomagnetic effects that act as an earthquake precursor. This study analysed the ULF frequency range as a short-term earthquake precursor at a depth < 100 km and an epicentral distance < 100 km (distance from Cebu magnetometer station) measured using a ground magnetometer installed in Cebu (10.36°N, 123.91°E), in the Philippines. This study also intended to determine the emission of magnetic pulsation (Pc4 and Pc5), solar wind parameters and near equatorial geomagnetic storms (SYM/H) in low latitude regions prior to an earthquake event. Findings show that the most evident ULF that acts as a potential earthquake precursor was at a frequency range of Pc5 (1.7-6.7 mHz) compared to Pc4 (6.7-22 mHz). It also shows that high solar wind changes and geomagnetic storms respond to the emission of ULF magnetic pulsations (Pc4 and Pc5) prior to earthquake events at low latitudes. Thus, it can be concluded that magnetic pulsations are signatures that indicate the probability of short-term earthquakes precursor.

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  • A machine learning approach combined with wavelet analysis for automatic detection of Pc5 geomagnetic pulsations observed at geostationary orbits

    Justice Allotey Pappoe, Akimasa Yoshikawa, Ali Kandil, Ayman Mahrous

    Advances in Space Research   2023   ISSN:0273-1177 eISSN:1879-1948

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    Pc5 geomagnetic pulsations are ultra-low frequency (ULF) waves whose period lies within 150–600 s. Their detection is crucial for accurate space weather modelling, monitoring, and analysis. Identification of these pulsations using manual approaches is difficult and time-consuming because of the smaller magnitudes and the limited durations within which they occur. To overcome this challenge, we propose a robust Cascade Forward Neural Network (CFNN) model combined with the wavelet technique for automatically detecting Pc5 events from satellite datasets observed at geostationary orbits. The dataset used in this study is the magnetic field vector measurements retrieved from the Geostationary Operational Environmental Satellite-10 (GOES-10) from 2000 to 2009. Pc5 geomagnetic pulsations were extracted from the toroidal component of the field perturbation using a bandpass Butterworth filter. Continuous wavelet transform (CWT) analysis using the mother Morlet wavelet was utilized to validate the integrity of the extracted signal in the time–frequency domain. The extracted Pc5 signal was decomposed into details and approximations using Daubechies wavelet transform to separate the intelligible signal from the incoherent noise that left their trace on the magnetic field time series. The detail signal was subjected to denoising using the heuristic Stein Unbiased Risk Estimate (SURE) approach with soft thresholding to obtain the denoised Pc5 events. The denoised Pc5 events were utilized as the target in the machine learning whereas the inputs were obtained from 5-dimensional space transformation of the toroidal component of the time series. The developed algorithm performed well and demonstrated a detection accuracy of 80 % and a Root Mean Square Error (RMSE) of 0.13 nT indicating a high performance in detecting Pc5 events. For effective validation of the model, Pc5 events detected by our model were correlated with the Kp index and the amplitude of the Pc5 events observed at geostationary orbit. A good correlation was obtained in both cases, making our model a practical and preferred choice for Pc5 pulsation detection in contrast to conventional frequency analysis tools which take much time for signal processing on large data sets.

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  • 太陽フレア発生時のシューマン共鳴の特性

    Ikeda Akihiro

    大気電気学会誌   Vol. 17, No. 1   40 - 41   2023

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  • Geoelectric Section of the Coastal Region of the Chukchi Sea near the Cape Schmidt Observatory

    Starzhinskii, SS; Yoshikawa, A; Khomutov, SY

    RUSSIAN GEOLOGY AND GEOPHYSICS   63 ( 12 )   1459 - 1473   2022.12   ISSN:1068-7971 eISSN:1878-030X

  • Fecal microbiota in patients with a stoma decreases anaerobic bacteria and alters taxonomic and functional diversities

    Sakai, SA; Aoshima, M; Sawada, K; Horasawa, S; Yoshikawa, A; Fujisawa, T; Kadowaki, S; Denda, T; Matsuhashi, N; Yasui, H; Goto, M; Yamazaki, K; Komatsu, Y; Nakanishi, R; Nakamura, Y; Bando, H; Hamaya, Y; Kageyama, SI; Yoshino, T; Tsuchihara, K; Yamashita, R

    FRONTIERS IN CELLULAR AND INFECTION MICROBIOLOGY   12   925444   2022.9   ISSN:2235-2988

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  • Using Principal Component Analysis of Satellite and Ground Magnetic Data to Model the Equatorial Electrojet and Derive Its Tidal Composition

    Gabriel Soares, Yosuke Yamazaki, Achim Morschhauser, Jurgen Matzka, Katia J. Pinheiro, Claudia Stolle, Patrick Alken, Akimasa Yoshikawa, Kornyanat Hozumi, Atul Kulkarni, Pornchai Supnithi

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   127 ( 9 )   2022.9   ISSN:2169-9380 eISSN:2169-9402

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    The intensity of the equatorial electrojet (EEJ) shows temporal and spatial variability that is not yet fully understood nor accurately modeled. Atmospheric solar tides are among the main drivers of this variability but determining different tidal components and their respective time series is challenging. It requires good temporal and spatial coverage with observations, which, previously could only be achieved by accumulating data over many years. Here, we propose a new technique for modeling the EEJ based on principal component analysis (PCA) of a hybrid ground-satellite geomagnetic data set. The proposed PCA-based model (PCEEJ) represents the observed EEJ better than the climatological EEJM-2 model, especially when there is good local time separation among the satellites involved. The amplitudes of various solar tidal modes are determined from PCEEJ based tidal equation fitting. This allows to evaluate interannual and intraannual changes of solar tidal signatures in the EEJ. On average, the obtained time series of migrating and nonmigrating tides agree with the average climatology available from earlier work. A comparison of tidal signatures in the EEJ with tides derived from neutral atmosphere temperature observations show a remarkable correlation for nonmigrating tides such as DE3, DE2, DE4, and SW4. The results indicate that it is possible to obtain a meaningful EEJ spectrum related to solar tides for a relatively short time interval of 70 days.

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  • The Variation of Counter-Electrojet Current at the Southeast Asian Sector during Different Solar Activity Levels

    Nur Izzati Mohd Rosli, Nurul Shazana Abdul Hamid, Mardina Abdullah, Khairul Adib Yusof, Akimasa Yoshikawa, Teiji Uozumi, Babatunde Rabiu

    APPLIED SCIENCES-BASEL   12 ( 14 )   2022.7   eISSN:2076-3417

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    Studies on counter-electrojet currents (CEJ) using ground data revealed that this current could occur simultaneously among locations that are less than 30 degrees longitude apart. In our work, the symmetricity of CEJ variation between the west and east of Southeast Asia, separated by similar to 25 degrees, was preliminarily examined according to its types: morning (MCEJ) and afternoon (ACED. Since most of the past studies had overlooked the occurrence after dusk, the monitoring period was also extended from 18:00 to 21:00 LT, namely, the post-sunset depletion (PSD). The magnetometer station in Davao, Philippines (DAV) and Langkawi, Malaysia (LKW) were chosen to represent the east and west parts. The EEJ index (i.e., EUEL) over the periods of the solar cycle 24 (2008-2018) was utilized specifically during magnetically quiet days (Kp < 3). As the result, both parts symmetrically showed that MCEJ and ACEJ were positively and negatively correlated with the F10.7 index. Contrarily, MCEJ and ACEJ were asymmetrically prominent in the east and west. CEJ types also varied symmetrically with the season, especially for MCEJ and ACEJ (at high level), prominent during Equinox and J-solstice. Post-sunset depletion (PSD) in both parts was symmetrically solar activity independent, as no correlation with the F10.7 index was observed in the extended observation. PSD that varied symmetrically with season was also solar activity independent, except in the east during Equinox, where it was negatively correlated with the F10.7 index. Our finding also revealed that PSD was prominent during Equinox, except for the high level in the west part.

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  • Signatures of Auroral Potential Structure Extending Through the Near‐Equatorial Inner Magnetosphere

    S. Imajo, Y. Miyoshi, K. Asamura, I. Shinohara, M. Nosé, K. Shiokawa, Y. Kasahara, Y. Kasaba, A. Matsuoka, S. Kasahara, S. Yokota, K. Keika, T. Hori, M. Shoji, S. Nakamura, M. Teramoto

    Geophysical Research Letters   49 ( 10 )   2022.5   ISSN:0094-8276 eISSN:1944-8007

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  • Generation Mechanisms of Plasma Density Irregularity in the Equatorial Ionosphere During a Geomagnetic Storm on 21–22 December 2014

    T. Sori, A. Shinbori, Y. Otsuka, T. Tsugawa, M. Nishioka, A. Yoshikawa

    Journal of Geophysical Research: Space Physics   127 ( 5 )   2022.5   ISSN:2169-9380 eISSN:2169-9402

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    The equatorial ionosphere endured plasma density irregularities during a geomagnetic storm on 21–22 December 2014. To understand the underlying mechanism, we analyzed the rate of the total electron content change (ROTI) data obtained from a global navigation satellite system, along with solar wind, interplanetary magnetic field (IMF), geomagnetic indices, Jicamarca incoherent scatter radar, and magnetometer data. The results indicate that the ROTI enhancement related to plasma density irregularities (plasma bubbles) occurred three times in the equatorial and low latitude regions of the American sector during the geomagnetic storm. The first, second, and third enhancements which have a longitudinal extent of ∼20° appeared in the post-sunset, pre-midnight, and post-midnight sectors, respectively. The second enhancement occurred during the recovery phase of the storm-time substorm even though the IMF remained southward. During this period, the direction of the dayside equatorial electrojet (EEJ) changed from eastward to westward, while the nightside upward plasma velocity at Jicamarca increased to 28.8 m/s. The response of the EEJ and upward ion drift implies that the westward and eastward electric fields were intensified on the dayside and nightside, respectively. Therefore, these results suggest that an over-shielding electric field penetrates the dayside/nightside equator simultaneously in association with a substorm recovery phase, and that the electric field generates plasma bubbles by the Rayleigh-Taylor instability mechanism. Plasma bubbles induced by the penetration of an over-shielding electric field due to substorm activity have not previously been reported.

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  • Effect of Meteoric Ions on Ionospheric Conductance at Jupiter

    Yuki Nakamura, Koichiro Terada, Chihiro Tao, Naoki Terada, Yasumasa Kasaba, François Leblanc, Hajime Kita, Aoi Nakamizo, Akimasa Yoshikawa, Shinichi Ohtani, Fuminori Tsuchiya, Masato Kagitani, Takeshi Sakanoi, Go Murakami, Kazuo Yoshioka, Tomoki Kimura, Atsushi Yamazaki, Ichiro Yoshikawa

    Journal of Geophysical Research: Space Physics   127 ( 3 )   2022.3   ISSN:2169-9380 eISSN:2169-9402

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    Effect of Meteoric Ions on Ionospheric Conductance at Jupiter
    Ionospheric Pedersen and Hall conductances play significant roles in electromagnetic coupling between the planetary ionosphere and magnetosphere. Several observations and models have suggested the existence of meteoric ions with interplanetary origins in the lower part of Jupiter’s ionosphere; however, no models have considered the contributions of meteoric ions to ionospheric conductance. This study is designed to evaluate the contribution of meteoric ions to ionospheric conductance by developing an ionospheric model combining a meteoroid ablation model and a photochemical model. We find that the largest contribution to Pedersen and Hall conductivities occurs in the meteoric ion layer at altitudes of 350–600 km due to the large concentration of meteoric ions resulting from their long lifetimes of more than 100 Jovian days. Pedersen and Hall conductances are enhanced by factors of 3 and 10, respectively, in the middle- and low-latitude and auroral regions when meteoric ions are included. The distribution of Pedersen and Hall conductances becomes axisymmetric in the middle- and low-latitude regions. Enhanced axisymmetric ionospheric conductance should impact magnetospheric plasma convection. The contribution of meteoric ions to the ionospheric conductance is expected to be important only on Jupiter in our solar system because of Jupiter’s intense magnetic and gravitational fields.

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  • Extreme Enhancements of Electron Temperature in Low Latitude Topside Ionosphere During the October 2016 Storm

    Ruilong Zhang, Libo Liu, Han Ma, Yiding Chen, Huijun Le, Akimasa Yoshikawa

    Journal of Geophysical Research: Space Physics   127 ( 3 )   2022.3   ISSN:2169-9380 eISSN:2169-9402

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    We use the in-situ observations of DMSP and SWARM satellites to report the changes of the topside ionospheric electron temperature during the October 2016 storm. Electron temperature in the afternoon sector dramatically increases in low latitudes in the recovery phase of the storm. Furthermore, the temperature enhancements have an obvious dependence on longitude and are mainly centralized around 100°–150°E in different satellite observations. The temperature enhancements attain more than 2,000 K at 840 km and 1,500 K at 450 km around the magnetic equator. The decrease in the electron-ion collision cooling rate, resulting from the lessened topside electron density, could not fully explain the temperature enhancement. At the same time, the electron densities in crests of the equatorial ionization anomaly are suppressed drastically at 100°–150°E, which cause a less heat conduction effect from the equatorial topside ionosphere to low altitudes via magnetic field lines and heat the topside ionospheric electron temperature. Further analysis indicates that dayside westward disturbance dynamo electric field presents a significant longitude structure and is a primary driver for the topside ionospheric temperature enhancement during the storm.

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  • Ionospheric Current Variations by Empirical Orthogonal Function Analysis: Solar Activity Dependence and Longitudinal Differences

    Charles Owolabi, Haibing Ruan, Y. Yamazaki, R. O. Kaka, O. O. Akinola, Akimasa Yoshikawa

    Journal of Geophysical Research: Space Physics   127 ( 1 )   2022.1   ISSN:2169-9380 eISSN:2169-9402

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    The solar quiet (Sq) ionospheric current variations exhibit spatial and temporal patterns that can be identified by the prevailing eigenmodes based on the empirical orthogonal function (EOF) analysis. In this study, the Sq current function over the American and European/African sectors are derived using ground magnetometer data from 2006 to 2019 based on the spherical harmonic analysis technique. Subsequently, we decomposed the Sq current function into eigenmodes by applying the EOF analysis, where the first three eigenmodes capture 96% of the overall Sq current variance. Additionally, these eigenmodes are utilized to model the Sq current function and compare its properties between the two longitudinal sectors. We observed that the EOF model could reconstruct the observed Sq current function with the first three eigenmodes in both longitudinal sectors. Moreover, the EOF model unveils a clear association of the Sq current function with several driven features, such as magnetic latitude, local time, season, and solar activity. Both longitudinal sectors had comparable Sq current patterns under varying solar activity, while their amplitudes varied. Besides, the newly developed model could reproduce a refined Sq current variability over the two longitudinal sectors as long as the observed Sq variations have sufficient duration. Our EOF model shows that the variations of the Sq current function with solar activity can be explained by the first three eigenmodes, which could be used as a basis for further numerical modeling of the Sq current variations.

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  • Missing data imputation of MAGDAS-9’s ground electromagnetism with supervised machine learning and conventional statistical analysis models

    Muhammad Asraf H., Nur Dalila Nur, Nooritawati Md Tahir, Zatul Iffah Abd Latiff, Mohamad Huzaimy Jusoh, Yoshikawa Akimasa

    Alexandria Engineering Journal   61 ( 1 )   937 - 947   2022.1   ISSN:1110-0168 eISSN:2090-2670

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    Data imputation studies include reconstruction or estimation of imperfect data gaps caused by system sensing failure, and non-responsive data transmission remains an open issue. In space weather applications, imputation of ground electromagnetism is significant in capturing the complex interaction of sun–earth prior to the subsequent analysis of the space weather effects. Key contributions to the demonstration of supervised machine learning (ML) imputation approach with artificial neural network, K-nearest neighbour, support vector regression (SVR), and General Regression Neural Network (GRNN) for MAGDAS-9 ground electromagnetism dataset have not yet been established. A total of 1,585,950 data points were analysed with supervised ML models which included performance benchmark with statistical analysis namely zero value substitution, listwise deletion, mean substitution, and hot deck imputation. To achieve low reconstruction errors, different imputation models with hyperparameter tuned settings are varied, and computational time execution has been shown to contribute to imputation performance. Performance metrics measured by mean square error (MSE), mean absolute error (MAE),mean absolute percentage error (MAPE), and execution time respectively demonstrate the capability of SVR to perfectly impute missing data for all ground electromagnetism components at an average of 0.314 MSE, 0.738 MAPE, closeness to 0.510 MAE and 0.91-second at various percentage level of data missingness. A comparison with traditional imputation shows that the supervised ML with SVR model has improved imputation performance by up to 80% of data gap. The outcome of the proposed imputation will benefit space weather applications for event characterisation, which will cover a large number of missing data in the MAGDAS-9 dataset.

    DOI: 10.1016/j.aej.2021.04.096

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  • Thermospheric wind response to a sudden ionospheric variation in the trough: Event at a pseudo breakup during geomagnetically quiet conditions Reviewed

    S.-i. Oyama, H. Vanhamäki, L. Cai, A. Aikio, M. Rietveld, Y. Ogawa, T. Raita, M. Kellinsalmi, K. Kauristie, B. Kozelov, A. Shinbori, K. Shiokawa, T. T. Tsuda, T. Sakanoi

    Earth Planets Space   74 ( 1 )   154   2022   ISSN:1343-8832 eISSN:1880-5981

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    The thermospheric wind response to a sudden westward turning of the ion velocity at a high latitude was studied by analyzing data obtained with a Fabry-Perot interferometer (FPI; 630 nm), Dynasonde, and Swarm A & C satellites during a conjunction event. The event occurred during a geomagnetically quiet period (Kp= 0+) through the night, but some auroral activity occurred in the north. The collocated FPI and Dynasonde measured the thermospheric wind (U) and ionospheric plasma velocity (V), respectively, in the F region at the equatorward trough edge. A notable scientific message from this study is the possible role of thermospheric wind in the energy dissipation process at F-region altitude. The FPI thermospheric wind did not instantly follow a sudden V change due to thermospheric inertia in the F region. At a pseudo-breakup during the event, V suddenly changed direction from eastward to westward within 10 min. U was concurrently accelerated westward, but its development was more gradual than that of V, with U remaining eastward for a while after the pseudo-breakup. The delay of U is attributed to the thermospheric inertia. During this transition interval, U.V was negative, which would result in more efficient generation of frictional heating than the positive U.V case. The sign of U.V, which is related to the relative directions of the neutral wind and plasma drift, is important because of its direct impact on ion-neutral energy exchange during collisions. This becomes especially important during substorm events, where rapid plasma velocity changes are common. The sign of U.V may be used as an indicator to find the times and locations where thermospheric inertia plays a role in the energy dissipation process.

    DOI: 10.1186/s40623-022-01710-6

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  • Radiation Analysis of LEO Mission in the South Atlantic Anomaly during Geomagnetic Storm

    Kirolosse M. Girgis, Tohru Hada, Shuichi Matsukiyo, Akimasa Yoshikawa

    IEEE Journal of Radio Frequency Identification   6   292 - 298   2022   eISSN:2469-7281

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    We have studied the radiation environment of LEO spacecraft when passing through the South Atlantic Anomaly (SAA) during the geomagnetic storm event of 15 May 2005. The 70-180 MeV proton flux information were numerically obtained from a simulation model of the inner radiation belt. The radiation analysis was consisted of two parts: the estimation of the Single Event Upset (SEU) rates and the absorbed radiation doses. One of the characteristics of the SAA at 800 km altitude during the recovery phase of the geomagnetic storm was the enhancement of its southern proton flux cell. It was found that the excess SEU rates and absorbed radiation doses could reach at least 200 % and 70 % respectively during the recovery phase in comparison to the initial phase of the geomagnetic storm. The estimated radiation results were in a good agreement with observations.

    DOI: 10.1109/JRFID.2022.3163441

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  • Preliminary Modelling of Solar Quiet Geomagnetic Field Average using Non-Linear Autoregressive with Exogeneous Input (NARX)

    Hashim M.H., Jusoh M.H., Burhanudin K., Yassin I.M., Hamid N.S.A., Radzi Z.M., Yoshikawa A.

    Journal of Mechanical Engineering   11 ( Special Issue 1 )   333 - 345   2022   ISSN:18235514

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    This paper discusses geomagnetic field attempt modelling using an Artificial Neural Network (ANN). The local horizontal component of geomagnetic field data was collected on April 2011 (equinox) during a solar quiet day at recent solar cycle inclination-24 using the Magnetic Data Acquisition System (MAGDAS) in Langkawi, Malaysia, in the low latitude region. The calculated average values (mean) of the H component geomagnetic field variation during Equinox 2011 characterised the dominant geomagnetic field during that particular solar cycle. The difference in amplitude of maximum and minimum values shows a regular diurnal variation of the geomagnetic field during Sq in the low latitude region. The output training utilised these calculated mean values during the modelling attempt. Meanwhile, the input training utilised proton density, solar wind plasma speed, plasma flow pressure, and Interplanetary Magnetic Field (IMF) space data using Non-Linear Auto Regressive Input (NARX). The best modelling outputs were 3, 2, and 3 for input delay (nu), output delay (ny), and hidden layer size (h), respectively. Residual test and model fit analysis show an unbiased and high overlap between predicted and actual geomagnetic field average values, suggesting the model can potentially anticipate the geomagnetic field average during solar quiet in November (month of Equinox) on solar cycle inclination.

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  • Preliminary Modelling of Solar Quiet Geomagnetic Field Average using Non-Linear Autoregressive with Exogeneous Input (NARX)

    M. H. Hashim, M. H. Jusoh, K. Burhanudin, I. M. Yassin, N. S.A. Hamid, Z. M. Radzi, A. Yoshikawa

    Journal of Mechanical Engineering   11 ( Special Issue 1 )   333 - 345   2022   ISSN:1823-5514 eISSN:2550-164X

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    This paper discusses geomagnetic field attempt modelling using an Artificial Neural Network (ANN). The local horizontal component of geomagnetic field data was collected on April 2011 (equinox) during a solar quiet day at recent solar cycle inclination-24 using the Magnetic Data Acquisition System (MAGDAS) in Langkawi, Malaysia, in the low latitude region. The calculated average values (mean) of the H component geomagnetic field variation during Equinox 2011 characterised the dominant geomagnetic field during that particular solar cycle. The difference in amplitude of maximum and minimum values shows a regular diurnal variation of the geomagnetic field during Sq in the low latitude region. The output training utilised these calculated mean values during the modelling attempt. Meanwhile, the input training utilised proton density, solar wind plasma speed, plasma flow pressure, and Interplanetary Magnetic Field (IMF) space data using Non-Linear Auto Regressive Input (NARX). The best modelling outputs were 3, 2, and 3 for input delay (nu), output delay (ny), and hidden layer size (h), respectively. Residual test and model fit analysis show an unbiased and high overlap between predicted and actual geomagnetic field average values, suggesting the model can potentially anticipate the geomagnetic field average during solar quiet in November (month of Equinox) on solar cycle inclination.

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  • PSTEP: project for solar–terrestrial environment prediction

    Kanya Kusano, Kiyoshi Ichimoto, Mamoru Ishii, Yoshizumi Miyoshi, Shigeo Yoden, Hideharu Akiyoshi, Ayumi Asai, Yusuke Ebihara, Hitoshi Fujiwara, Tada-Nori Goto, Yoichiro Hanaoka, Hisashi Hayakawa, Keisuke Hosokawa, Hideyuki Hotta, Kornyanat Hozumi, Shinsuke Imada, Kazumasa Iwai, Toshihiko Iyemori, Hidekatsu Jin, Ryuho Kataoka, Yuto Katoh, Takashi Kikuchi, Yûki Kubo, Satoshi Kurita, Haruhisa Matsumoto, Takefumi Mitani, Hiroko Miyahara, Yasunobu Miyoshi, Tsutomu Nagatsuma, Aoi Nakamizo, Satoko Nakamura, Hiroyuki Nakata, Naoto Nishizuka, Yuichi Otsuka, Shinji Saito, Susumu Saito, Takashi Sakurai, Tatsuhiko Sato, Toshifumi Shimizu, Hiroyuki Shinagawa, Kazuo Shiokawa, Daikou Shiota, Takeshi Takashima, Chihiro Tao, Shin Toriumi, Satoru Ueno, Kyoko Watanabe, Shinichi Watari, Seiji Yashiro, Kohei Yoshida, Akimasa Yoshikawa

    Earth, Planets and Space   73 ( 1 )   159   2021.12

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    PSTEP: project for solar–terrestrial environment prediction
    <title>Abstract</title>Although solar activity may significantly impact the global environment and socioeconomic systems, the mechanisms for solar eruptions and the subsequent processes have not yet been fully understood. Thus, modern society supported by advanced information systems is at risk from severe space weather disturbances. Project for solar–terrestrial environment prediction (PSTEP) was launched to improve this situation through synergy between basic science research and operational forecast. The PSTEP is a nationwide research collaboration in Japan and was conducted from April 2015 to March 2020, supported by a Grant-in-Aid for Scientific Research on Innovative Areas from the Ministry of Education, Culture, Sports, Science and Technology of Japan. By this project, we sought to answer the fundamental questions concerning the solar–terrestrial environment and aimed to build a next-generation space weather forecast system to prepare for severe space weather disasters. The PSTEP consists of four research groups and proposal-based research units. It has made a significant progress in space weather research and operational forecasts, publishing over 500 refereed journal papers and organizing four international symposiums, various workshops and seminars, and summer school for graduate students at Rikubetsu in 2017. This paper is a summary report of the PSTEP and describes the major research achievements it produced.

    DOI: 10.1186/s40623-021-01486-1

  • Seasonal variation of inter-hemispheric field-aligned currents deduced from time-series analysis of the equatorial geomagnetic field data during solar cycle 23–24

    Manjula Ranasinghe, Akiko Fujimoto, Akimasa Yoshikawa, Chandana Jayaratne

    Earth, Planets and Space   73 ( 1 )   146-1 - 146-10   2021.12

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    The east–west component of magnetic field variation (∆D-component) at Davao station (Philippines, geomagnetic latitude: – 2.22˚N) are used to investigate the characteristics of the long-term Inter-Hemispheric Field-Aligned Currents (IHFACs) based on the time-series analysis from August 1998 to July 2020. Recent in situ satellite and ground-based observations have reported that dusk-side current polarity of IHFAC is often opposite to that of the noon IHFAC, being inconsistent with Fukushima's IHFACs model. We investigated the consistency of the dusk-side IHFAC polarity derived from the observations with the polarity expected from Fukushima’s IHFACs model and examined the solar cycle dependence of IHFACs. It was confirmed that the dusk-side IHFACs during June and December solstices flow in the same direction of the noontime IHFACs, which was consistent with the IHFAC polarities suggested by the Fukushima model. The dusk-side IHFACs around March and September–November months disagreed with the Fukushima model. The ∆D variations clearly showed seasonal asymmetry in the dawn and noon sectors, whereas the ∆D variations in the dusk sector demonstrated seasonal symmetry. Solar cycle dependence of IHFACs was exhibited in the dusk sector. For the dawn and noon sectors, the yearly peak-to-peak ∆D amplitude in the later solar cycle SC24 decreased by about 35&#37; in comparison with the earlier solar cycle SC23. In contrast, the dusk-side yearly peak-to-peak ∆D amplitude increased by about 200&#37;. The dusk-side IHFAC yearly amplitude tended to be in inverse proportion to solar activity. [Figure not available: see fulltext.]

    DOI: 10.1186/s40623-021-01481-6

  • A statistical analysis of the relationship between Pc4 and Pc5 ULF waves, solar winds and geomagnetic storms for predicting earthquake precursor signatures in low latitude regions

    S. N.A. Syed Zafar, Roslan Umar, N. H. Sabri, M. H. Jusoh, A. Yoshikawa, S. Abe, T. Uozumi

    IOP Conference Series: Earth and Environmental Science   880 ( 1 )   2021.11

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    Short-term earthquake forecasting is impossible due to the seismometer's limited sensitivity in detecting the generation of micro-fractures prior to an earthquake. Therefore, there is a strong desire for a non-seismological approach, and one of the most established methods is geomagnetic disturbance observation. Previous research shows that disturbances in the ground geomagnetic field serves as a potential precursor for earthquake studies. It was discovered that electromagnetic waves (EM) in the Ultra-Low Frequency (ULF) range are a promising tool for studying the seismomagnetic effect of earthquake precursors. This study used a multiple regression approach to analyse the preliminary study on the relationship between Pc4 (6.7-22 mHz) and Pc5 (1.7-6.7 mHz) ULF magnetic pulsations, solar wind parameters and geomagnetic indices for predicting earthquake precursor signatures in low latitude regions. The ground geomagnetic field was collected from Davao station (7.00 N, 125.40 E), in the Philippines, which experiences nearby earthquake events (Magnitude <5.0, depth <100 km and epicentre distance from magnetometer station <100 km). The Pc5 ULF waves show the highest variance with four solar wind parameters, namely SWS, SWP, IMF-Bz, SIE and geomagnetic indices (SYM/H) prior to an earthquake event based on the regression model value of R2 = 0.1510. Furthermore, the IMF-Bz, SWS, SWP, SWE, and SYM/H were found to be significantly correlated with Pc5 ULF geomagnetic pulsation. This Pc5 ULF magnetic pulsation behaviour in solar winds and geomagnetic storms establishes the possibility of using Pc5 to predict earthquakes.

    DOI: 10.1088/1755-1315/880/1/012010

  • Empirical Modeling of Ionospheric Current Using Empirical Orthogonal Function Analysis and Artificial Neural Network

    Charles Owolabi, Haibing Ruan, Yosuke Yamazaki, Jinfeng Li, Jiahao Zhong, A. V. Eyelade, Shishir Priyadarshi, Akimasa Yoshikawa

    Space Weather   19 ( 11 )   2021.11

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    Empirical Modeling of Ionospheric Current Using Empirical Orthogonal Function Analysis and Artificial Neural Network
    Given the potential importance of solar quiet (Sq) ionospheric current in geomagnetic field modeling, it is vital to obtain accurate parameters characterizing its variations, particularly the spatial and temporal variations. In this paper, we derived the Sq current function based on the spherical harmonic analysis (SHA) technique using a 14-year (2006–2019) quiet geomagnetic field record over the American sector. The empirical orthogonal function (EOF) analysis was then applied to deduce temporal and spatial variations of the Sq current. It is observed that the first EOF mode of the Sq current function is dominated by solar activity, while the second and third EOF modes exhibit annual and semiannual variations, respectively. Also, the artificial neural network (ANN) model of Sq current function was constructed to validate the EOF model predictions. While the Sq current intensity predicted by the ANN model is underestimated by 2.83&#37;, the EOF model underpredicted the Sq current intensity by 1.92&#37; relative to the observation. The root mean square error (RMSE) of the EOF model is 0.64 kA. This RMSE is about 79&#37; smaller than that of the ANN model. In addition, both the EOF and ANN models capture the variation of the total Sq current (Jtotal) intensity with respect to solar activity. In principle, the EOF model had an optimal performance at nearly 98&#37; accuracy, with the ANN model exhibiting almost the same degree of accuracy, which appears to be a reference point for ionospheric conditions when looking for space weather applications.

    DOI: 10.1029/2021SW002831

  • Earth's geomagnetic response to solar wind changes associated with solar events at low latitude regions at the TRE MAGDAS Station

    R. Umar, S. N.A.Syed Zafar, N. H. Sabri, M. H. Jusoh, A. Yoshikawa, S. Abe, T. Uozumi

    IOP Conference Series: Earth and Environmental Science   880 ( 1 )   2021.11

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    The Sun's magnetic activity influences disturbances that perturb interplanetary space by producing large fluxes of energetic protons, triggering geomagnetic storms and affecting the ground geomagnetic field. The effect of two solar events, namely Coronal Mass Ejection (CME) and Coronal Holes, on geomagnetic indices (SYM/H), solar wind parameters and ground geomagnetic fields has provided magnetic ground data, which were extracted from the Terengganu (TRE, -4.21 N, 175.91 E) Magnetometer (MAGDAS) station, and investigated in this study. Results show that the physical dynamic mechanism in the Earth's magnetosphere is triggered by various solar wind parameters associated with CMEs and Coronal hole events during the minimum solar cycle of 24 at low latitudes. It is important to study solar wind-magnetosphere coupling because it has an impact on ground-based technological systems and human activities.

    DOI: 10.1088/1755-1315/880/1/012009

  • Effects of solar flares and coronal mass ejections on Earth's horizontal magnetic field and solar wind parameters during the minimum solar cycle 24

    S. N.A. Syed Zafar, R. Umar, N. H. Sabri, M. H. Jusoh, A. N. Dagang, A. Yoshikawa

    Monthly Notices of the Royal Astronomical Society   504 ( 3 )   3812 - 3822   2021.7

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    Previous studies have reported that coronal mass ejections (CMEs) and solar flares lead to the development of huge storms and high-speed streams. Our aim in this paper is to investigate the response of the geomagnetic index SYM/H to the solar wind parameters, such as solar wind speed V, dynamic pressure P, input energy IE and the interplanetary magnetic field (IMF) Bz component, associated with solar flares and CME events. The response of the ground geomagnetic field (H-component) to the solar wind parameters and the IMF Bz component at three low-latitude stations has also been analysed. Our findings show that the delay of the solar wind changes in the Earth's magnetosphere in response to the weak geomagnetic storm (SYM/H = -30 nT) at the beginning of 2014 December 21. A weak storm of SYM/H = -30 nT in the middle of 2014 November 5 is suggested by a low magnetic reconnection process in the magnetosphere. In addition, the strong southward IMF Bz component and high solar wind changes in the magnetosphere system, which were a result of the X2.0 solar flare event and the CMEs on 2014 October 27, responded to the moderate storm (SYM/H = -60 nT) at the beginning of 2014 October 28. This dynamic physical process in the magnetosphere caused by solar wind variation is seen to excite the Earth's H-component through ultra low frequency at the ground-based magnetometers at the BCL (Vietnam), TIR (India) and SCN (Indonesia) stations during the geomagnetic storm. This study relates to seismic investigations and geomagnetic-induced current on the ground.

    DOI: 10.1093/mnras/stab1161

  • Identification of Fractal Properties in Geomagnetic Data of Southeast Asian Region during Various Solar Activity Levels

    Farhan Naufal Rifqi, Nurul Shazana Abdul Hamid, A. Babatunde Rabiu, Akimasa Yoshikawa

    Universe   7 ( 7 )   248   2021.7

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    Identification of fractal properties in geomagnetic data of southeast asian region during various solar activity levels
    The fractal properties of geomagnetic northward component data (H-component) in the equatorial region during various phases of solar activity over Southeast Asia were investigated and then quantified using the parameter of the Hurst exponent (H). This study began with the identification of existence of spectral peaks and scaling properties in international quiet day H-component data which were measured during three levels of solar activity: low, intermediate, and high. Then, various cases of quiet and disturbed days during different solar activity levels were analyzed using the method that performed the best in the preceding part. In all the years analyzed, multifractal scaling and spectral peaks exist, signifying that the data have fractal properties and that there are external factors driving the fluctuations of geomagnetic activity other than solar activity. The analysis of various cases of quiet and disturbed days generally showed that quiet days had anti-persistence tendencies (H < 0.5) while disturbed days had persistence tendencies (H > 0.5)—generally a higher level of Hurst exponent compared to quiet days. As for long-term quiet day H-component data, it had a Hurst exponent value that was near H ≃0.50, while the long-term disturbed day H-component data showed higher values than that of the quiet day.

    DOI: 10.3390/universe7070248

  • The Ionosphere at Middle and Low Latitudes Under Geomagnetic Quiet Time of December 2019

    Jiawei Kuai, Qiaoling Li, Jiahao Zhong, Xu Zhou, Libo Liu, Akimasa Yoshikawa, Lianhuan Hu, Haiyong Xie, Chaoyan Huang, Xumin Yu, Xin Wan, Jun Cui

    Journal of Geophysical Research: Space Physics   126 ( 6 )   2021.6

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    The Ionosphere at Middle and Low Latitudes Under Geomagnetic Quiet Time of December 2019
    The ionospheric electron density shows remarkable day-to-day variability due to solar radiance, geomagnetic activity and lower atmosphere forcing. In this report, we investigated the ionospheric variations at middle and low latitudes during a period under geomagnetic quiet time (Kpmax = 1.7) from November 30 to December 8, 2019. During the quiescent period, the ionosphere is not undisturbed as expected in the Asian-Australian and the American sectors. Total electron content (TEC) has multiple prominent enhancements at middle and low latitudes in the two sectors, and TEC depletions also occur repeatedly in the Asian-Australian sector. The low-latitude electric fields vary significantly, which is likely to be modulated by the notably changing tides in the mesosphere and lower thermosphere region. It is worth noting that the variations of TEC and the electric fields are not consistent in the two sectors, particularly on December 4–6. Further investigation reveals that the increase in TEC depends on altitude. The TEC enhancements are mainly contributed by the altitude below 500 km in both two sectors, which indirectly reflects that the driving sources may come from the lower atmosphere. Especially, a mid-latitude band structure continuously appears at all local times in the North American sector on December 6–8, which is also mainly contributed by the altitude below 500 km.

    DOI: 10.1029/2020JA028964

  • Installation and preliminary data analysis of Penang magnetic data Acquisition system (MAGDAS) in Malaysia Reviewed International journal

    N. A. Zakaria, S. H.M. Yusoff, N. A.M. Rizal, N. S.A. Hamid, M. H. Hashim, Z. Mohd Radzi, M. H. Jusoh, @A. Yoshikawa, @T. Uozumi, @S. Abe

    Advances in Space Research   67 ( 7 )   2199 - 2206   2021.4

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    MAGDAS PEN was established on 19th September 2019 as one of the MAGDAS observatory arrays located at Universiti Sains Malaysia (USM) (5.15°, 100.50°). The main objective of the MAGDAS project is to monitor global electromagnetic and the ambient plasma density in the geospace environment. This installation has contributed to a better understanding of the Sun-Earth coupling system. This paper presents the installation process of one of the MAGDAS magnetometers named YU-8 T magnetic sensor and provides a preliminary analysis of geomagnetic HDZ components amplitude-time that was observed at PEN station. A one-month HDZ-geomagnetic field data was processed from 1st November to 30th November 2019. The daily variations with a consistent pattern in delta H geomagnetic field components are observed throughout the day with eastward electric field effects that are observed during solar peak hours. The delta H-component gradually increases around 0700LT and reaches the maximum reading at 1300LT with a range of value ~ 40-70nT. The value slowly decreases that started from 1400LT until the night time. The reading during the night time shows a constant variation with magnitude varies in between −10nT to + 10nT. The average H-component value of the night time is used as the baseline for the observation system. Overall, the observed trends portray a good sign of solar quiet field and Sq with no solar-terrestrial disturbances.

    DOI: 10.1016/j.asr.2021.01.009

  • Effects of solar activity on ionospheric current system in the Southeast Asia region Reviewed International journal

    N. S.A. Hamid, N. I.M. Rosli, W. N.I. Ismail, @A. Yoshikawa

    Indian Journal of Physics   95 ( 4 )   543 - 550   2021.4

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    The equatorial ionospheric current system is composed of equatorial electrojet (EEJ) and solar quiet (Sq) that flow in the eastward direction. That being mentioned, this study looked into the changes in ionospheric currents stemming from geomagnetic storm disturbances at different levels of solar activity during solar cycle 24. This analysis was performed by employing an EEJ index known as EUEL, which is calculated from northward geomagnetic component data measured using ground-based magnetometer at five different latitudes across the Southeast Asia region. Based on the outcomes, the impacts of geomagnetic storm on EEJ currents were observed at 1200 LT and 1100 LT, respectively, during high and low solar activity levels. Time delay was associated with changes in EEJ peak time at varied activity levels. This case study reveals that EEJ value at peak time of high solar activity decreased significantly during the main phase of geomagnetic storm.

    DOI: 10.1007/s12648-020-01734-2

  • Comparison of EEJ Longitudinal Variation from Satellite and Ground Measurements over Different Solar Activity Levels

    Wan Nur Izzaty Ismail, Nurul Shazana Abdul Hamid, Mardina Abdullah, Akimasa Yoshikawa, Teiji Uozumi, Zahira Mohd Radzi

    Universe   7 ( 2 )   23   2021.2

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    Comparison of eej longitudinal variation from satellite and ground measurements over different solar activity levels
    The longitudinal variability and local time of equatorial electrojet (EEJ) current using simultaneous data recorded by ground and satellite magnetometers at different levels of solar activity were investigated. In this study, we used data from the CHAMP and Swarm satellites to obtain EEJ current measurements around the globe. The ground data were provided by the MAGDAS, INTERMAGNET, and IIG networks. The ground observation was carried out by analyzing magnetometer data in four different sectors: the South American, Indian, African, and Southeast Asian sectors. These ground data were normalized to the dip equator to overcome the latitudinal variation of each station. The analysis for both measurements was performed using quiet day data. Both the ground and satellite data were categorized according to solar activity level; low, moderate, and high. The results revealed that, during the low solar activity, there was a good agreement between the longitudinal profiles of the EEJ measured using the satellite and the ground data. In general, strong correlations were obtained in most of the sectors where ground data were available between 11 and 13 local time (LT). Besides that, our analysis revealed that the different times of maximum EEJ appearances were seasonally dependent only at certain longitude sectors.

    DOI: 10.3390/universe7020023

  • Possibility of robust detrended fluctuation analysis as a method for identifying fractal properties of geomagnetic time series Reviewed International journal

    F. N. Rifqi, N. S.A. Hamid, @A. Yoshikawa

    Journal of Physics: Conference Series   1768 ( 1 )   2021.2

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    Geomagnetic data has been demonstrated to exhibit fractal properties, which are analysed using various fractal methods. These methods allow the characterization of geomagnetic activity during certain periods using the Hurst exponent. In this study, the geomagnetic activity during the quiet period of the month of December 2011 is analysed using the r-DFA method, of which viability to identify fractal properties of geomagnetic data has not been tested yet, and also using its established predecessor; the detrended fluctuation analysis (DFA). The results show that the r-DFA method is indeed viable to be used upon geomagnetic time series, with comparable if not better performance compared to its predecessor.

    DOI: 10.1088/1742-6596/1768/1/012004

  • Defining different type of CEJ currents based on ground-based geomagnetic data record at Langkawi station, Malaysia Reviewed International journal

    N. I.M. Rosli, N. S.A. Hamid, M. Abdullah, @A. Yoshikawa

    Journal of Physics: Conference Series   1768 ( 1 )   2021.2

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    A negative decrement in geomagnetic data in equatorial region is not necessarily cause by the well-known counter electrojet, CEJ but it is also can be affected by solar activity such as a solar flare. Relying on this matter, we did a comparison between CEJ and unusual solar flare effect called as SFE∗ on geomagnetic data before introducing several types of CEJ that can be extracted from EUEL index. This study used ground data from MAGDAS network located in Langkawi (LKW) with 1-minutes resolution during solar cycle 24 and applied EUEL index. From the results, it is crucial to ensure the minimum duration of EUEL depletion is within an hour because less than an hour depletion could be possibly cause by solar activity. Four interval of time that has been introduced in our study composed of several types of CEJ which are morning CEJ, afternoon CEJ and evening CEJ, with additional the controversial CEJ occurrence which is night CEJ. We also successfully demonstrated a rare CEJ occurrence that associated with solar flare effect using EUEL index.

    DOI: 10.1088/1742-6596/1768/1/012005

  • Correlations between Earthquake Properties and Characteristics of Possible ULF Geomagnetic Precursor over Multiple Earthquakes

    Khairul Adib Yusof, Mardina Abdullah, Nurul Shazana Abdul Hamid, Suaidi Ahadi, Akimasa Yoshikawa

    Universe   7 ( 1 )   20   2021.1

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    Correlations between earthquake properties and characteristics of possible ulf geomagnetic precursor over multiple earthquakes
    In this study, we improved and adapted existing signal processing methods on vast geomagnetic field data to investigate the correlations between various earthquake properties and characteristics of possible geomagnetic precursors. The data from 10 magnetometer stations were utilized to detect precursory ultra-low frequency emission and estimate the source direction for 34 earthquakes occurring between the year 2007–2016 in Southeast Asia, East Asia, and South America regions. As a result, possible precursors of 20 earthquakes were identified (58.82&#37; detection rate). Weak correlations were obtained when all precursors were considered. However, statistically significant and strong linear correlations (r ≥ 0.60, p < 0.05) were found when the precursors from two closely located stations in Japan (Onagawa (ONW) and Tohno (TNO)) were exclusively investigated. For these stations, it was found that the lead time of the precursor is strongly (or very strongly) correlated with the earthquake magnitude, the local seismicity index, and the hypocentral depth. In addition, the error percentage of the estimated direction showed a strong correlation with the hypocentral depth. It is concluded that, when the study area is restricted to a specific location, the earthquake properties are more likely to have correlations with several characteristics of the possible precursors.

    DOI: 10.3390/universe7010020

  • 地磁気突然の到来到着時間の近オンライン自動決定のための多重最適化パラメータ技術【JST・京大機械翻訳】

    Elgiddawy Sarah A., Hafez Ali G., Hafez Ali G., Hafez Ali G., Lethy Ahmed, Saad Omar M., Khalaf Ashraf A. M., Yoshikawa Akimasa, Hamed Hesham F. A., Hamed Hesham F. A.

    Arabian Journal for Science and Engineering   46 ( 2 )   901 - 908   2021.1

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    The Multi-Optimized Parameter Technique for Near Online Automatic Determination of Geomagnetic Sudden Commencement Arrival Time
    This paper introduces a new technique in the automatic detection of storm sudden commencement (SC) using the discrete wavelet transform (DWT). A geomagnetic storm is a global simultaneous phenomenon affecting the whole Earth, which means that all ground magnetometers running online will record this event. An algorithm using different characteristic features of the SC is proposed. The selection of an optimal threshold for feature parameters is critical for the success of SC automatic detection. Therefore, this paper uses particle swarm optimization (PSO) to determine the optimal feature threshold values. The developed algorithm is based on data records from a network of ground magnetometers. This algorithm is implemented via multi-resolution analysis (MRA) of the DWT using the Haar wavelet filter. Four-year data sampled at one sample/s from six ground stations from low to high latitudes were analyzed to develop and test this technique. Data representing 450 days from five stations operating simultaneously are available. The confusion matrix of all possible outcomes shows that the accuracy of the proposed algorithm is 97.33&#37;.

    DOI: 10.1007/s13369-020-04773-3

  • Integrating Pre-Earthquake Signatures From Different Precursor Tools

    Essam Ghamry, Emad K. Mohamed, Mohamed S. Abdalzaher, Mohamed Elwekeil, Dedalo Marchetti, Angelo De Santis, Mostafa Hegy, Akimasa Yoshikawa, Adel Fathy

    IEEE Access   9   33268 - 33283   2021.1

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    Integrating Pre-Earthquake Signatures From Different Precursor Tools.
    Potential earthquake precursors include, among others, electromagnetic fields, gas emissions, Land Surface Temperature (LST), Sea Surface Temperature (SST), and Surface Air Temperature (SAT) anomalies. These observables have been individually studied, before earthquakes, by many researchers. The ionospheric studies concerning earthquakes (EQs) using magnetic data from Low Earth Orbit (LEO) satellites are increasingly being used to detect ionospheric anomalies before large EQs. Also, LST, SST, and SAT values retrieved from Moderate Resolution Imaging Spectroradiometer (MODIS) Terra and Aqua satellites and Modern-Era Retrospective analysis for Research and Applications Version 2 (MERRA-2) are considered as physical precursors before EQs. In this work, we jointly analyze magnetic, MODIS, and MERRA-2 data in space and time around the epicenters before the selected EQs in Mexico, Japan, Chile, and Indonesia. Our analyses present interesting findings where anomalies in temperature and magnetic field, preceding the considered EQs, are confirmed through different methods. Particularly, we utilize the Fast Fourier Transform (FFT) and the Discrete Cosine Transform (DCT) for analyzing magnetic data over the designated EQs regions. We use the magnetic data acquired by Swarm satellites in the top side ionosphere along with MODIS and MERRA-2. Five case studies are described to prove the effectiveness of our analyses. Precursory anomalies were observed using these methods in different anomalous days from the considered four regions of interest around the epicenter. It is concluded that these methods could be effective and reliable in detecting anomalies preceding the upcoming EQs.

    DOI: 10.1109/ACCESS.2021.3060348

  • Evolution of field-aligned current in the meridional plane during substorm: multipoint observations from satellites and ground stations Reviewed

    Shun Imajo, Masahito Nosé, Mari Aida, Nana Higashio, Haruhisa Matsumoto, Koga Kiyokazu, Charles Smith, Robert J. MacDowall, Akimasa Yoshikawa

    Earth, Planets and Space   72 ( 1 )   2020.12

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    Evolution of field-aligned current in the meridional plane during substorm: multipoint observations from satellites and ground stations
    We report the propagation of substorm-associated magnetic fluctuations by multipoint magnetic observations from ground and space in the same meridional plane. The first Quasi-Zenith Satellite (QZS-1), which has a unique orbit of quasi-zenith orbit with an inclination of 41 ∘, an apogee of 7.1 RE radial distance, and an orbital period of 24 h, can stay for a long time in the near-earth magnetotail away from the magnetic equator. We examined a substorm event during 15:00–16:00 UT on July 09, 2013 when QZS-1 was located at 31 ∘ dipole latitude and 23.5 h dipole magnetic local time. The Engineering Test Satellite VIII (ETS-VIII), Time History of Events and Macroscale Interactions during Substorms D (THEMIS-D) at a radial distance of ∼ 10 RE, and THEMIS-E at a radial distance of ∼ 7 RE were located near the equator in the similar magnetic meridian. The dipolarization was first observed at THEMIS-D at 15:14:30 UT. Then, ∼ 1 min later, magnetic fluctuations were observed by ETS-VIII and THEMIS-E. At the same time, the magnetic bay and Pi2 pulsation were observed at low-latitude magnetic observatories and the Radiation Belt Storm Probes B satellite in the inner magnetosphere. We found that QZS-1 away from the equator observed a strong azimuthal magnetic field fluctuation with a long delay of 15 min from the first dipolarization at THEMIS-D near the equator. The speed of the poleward propagating magnetic fluctuation between the ionospheric footprints is calculated to be 310 [m / s] , which is consistent with a typical speed of auroral poleward expansion. A similar time delay of the onset of the negative bay was observed between the Tixie (AACGM MLAT = 66. 8 ∘) and Kotelny (AACGM MLAT = 71. 0 ∘) observatories near the ionospheric footprint of satellites. We suggest that the long delay time of the magnetic fluctuation at QZS-1 was associated with the crossing of field-aligned current during the poleward expansion of the substorm current system. The distribution of azimuthal magnetic field variations in the magnetosphere indicates that the east side downward current extended more west side in the higher latitude part of the current wedge.

    DOI: 10.1186/s40623-020-01182-6

  • The impact of coronal mass ejections on the seasonal variation of the ionospheric critical frequency f<inf>0</inf>F2 Reviewed International journal

    Hussein M. Farid, Ramy Mawad, Essam Ghamry, @Akimasa Yoshikawa

    Universe   6 ( 11 )   2020.11

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    We investigated the relations between the monthly average values of the critical frequency (f0F2) and the physical properties of the coronal mass ejections (CMEs), then we examined the seasonal variation of f0F2 values as an impact of the several CMEs properties. Given that, f0F2 were detected by PRJ18 (Puerto Rico) ionosonde station during the period 1996–2013. We found that the monthly average values of f0F2 are varying coherently with the sunspot number (SSN). A similar trend was found for f0F2 with the CMEs parameters such as the CME energy (linear correlation coefficient R = 0.73), width (R = 0.6) and the speed (R = 0.6). The arrived CMEs cause a plasma injection into the ionosphere, in turn, increasing the electron density, and consequently, f0F2 values. This happens in the high latitudes followed by the middle and lower latitudes. By examining the seasonal variation of f0F2, we found that the higher correlation between f0F2 and CMEs parameters occurs in the summer, then the equinoxes (spring and autumn), followed by the winter. However, the faster CMEs affect the ionosphere more efficiently in the spring more than in the summer, then the winter and the autumn seasons.

    DOI: 10.3390/universe6110200

  • Prominent Daytime TEC Enhancements Under the Quiescent Condition of January 2017

    Fuqing Huang, Jiuhou Lei, Ruilong Zhang, Na Li, Shengyang Gu, You Yu, Libo Liu, Charles Owolabi, Baiqi Ning, Guozhu Li, Jiahao Zhong, Tong Dang, Dexin Ren, Wen Yi, Xiaoli Luan, Xianghui Xue, Tao Yu, Faquan Li, Xiankang Dou, Akimasa Yoshikawa

    Geophysical Research Letters   47 ( 14 )   2020.7

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    Prominent Daytime TEC Enhancements Under the Quiescent Condition of January 2017
    It is well known that the ionospheric electron densities in the F-region usually undergo day-to-day variability with the magnitude of ~20–35&#37;, associated with the solar as well as geomagnetic activities and the meteorological forcing from the lower atmosphere. In this study, we reported remarkable enhancements in the total electron content (TEC) from the Beidou geostationary (GEO) satellites during the quiescent geophysical condition of January 2017 prior to the arrival of the sudden stratosphere warming (SSW). The daytime TEC around the equatorial ionization anomaly region increased by 75–160&#37; and lasted for several days. The equatorial electrojet and Sq current in the ionospheric E-region at low and middle latitudes showed the corresponding increase during the TEC enhancement interval. The possible contributions from the variations of solar EUV flux and geomagnetic activity are ruled out. Our further analysis showed that the diurnal tides in the temperature from Sounding of the Atmosphere using Broadband Emission Radiometry and the solar and lunar semidiurnal tides of neutral winds from two radars over China became strong during this period of interest. These results suggest that the lower atmospheric tidal forcing could contribute to the great and long-duration TEC enhancement in the ionosphere even though the SSW had not happened yet.

    DOI: 10.1029/2020GL088398

  • Whole Atmosphere Model Simulations of Ultrafast Kelvin Wave Effects in the Ionosphere and Thermosphere

    Y. Yamazaki, Y. Miyoshi, C. Xiong, C. Stolle, G. Soares, A. Yoshikawa

    Journal of Geophysical Research: Space Physics   125 ( 7 )   2020.7

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    This paper examines the response of the upper atmosphere to equatorial Kelvin waves with a period of ∼3 days, also known as ultrafast Kelvin waves (UFKWs). The whole atmosphere model Ground-to-topside model of Atmosphere and Ionosphere for Aeronomy (GAIA) is used to simulate the UFKW events in the late summer of 2010 and 2011 as well as in the boreal winter of 2012/2013. When the lower layers of the model below 30-km altitude are constrained with meteorological data, GAIA is able to reproduce salient features of the UFKW in the mesosphere and lower thermosphere as observed by the Aura Microwave Limb Sounder. The model also reproduces ionospheric response, as validated through comparisons with total electron content data from the Gravity field and steady-state Ocean Circulation Explorer satellite as well as with earlier observations. Model results suggest that the UFKW produces eastward-propagating ∼3-day variations with zonal wavenumber 1 in the equatorial zonal electric field and F region plasma density. Model results also suggest that for a ground observer, identifying ionospheric signatures of the UFKW is a challenge because of ∼3-day variations due to other sources. This issue can be overcome by combining ground-based measurements from different longitudes. As a demonstration, we analyze ground-based magnetometer data from equatorial stations during the 2011 event. It is shown that wavelet spectra of the magnetic data at different longitudes are only in partial agreement, with or without a ∼3-day peak, but a spectrum analysis based on multipoint observations reveals the presence of the UFKW.

    DOI: 10.1029/2020JA027939

  • The First Pi2 Pulsation Observed by China Seismo-Electromagnetic Satellite. Reviewed International journal

    Essam Ghamry, Dedalo Marchetti, @Akimasa Yoshikawa, @Teiji Uozumi, Angelo De Santis, Loredana Perrone, Xuhui Shen, Adel Fathy

    Remote. Sens.   12 ( 14 )   2300 - 2300   2020.4

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    On 2 February 2018, the China Seismo-Electromagnetic Satellite (CSES) ZhangHeng 01 (ZH-01) was successfully launched, carrying on board, in addition to a suite of plasma and particle physics instruments, a high precision magnetometer package (HPM), able to observe the ultra-low frequency (ULF) waves. In this paper, a night time Pi2 pulsation observed by CSES is reported for the first time. This Pi2 event occurred on 3 September 2018, and began at 14:30 UT (02:37 magnetic local time), when the satellite was in the southern hemisphere between -49 and -13 magnetic latitude (MLAT). Kakioka (KAK) ground station in Japan detected the same Pi2 between 14:30-14:42 UT (23:30-23:42 local time). The Pi2 oscillations in the compressional, toroidal, and poloidal components at the CSES satellite and the H-component at the KAK station are investigated by estimating coherence, amplitude, and cross-phase. We noticed a high degree of similarity between the Pi2 event in the horizontal component at KAK and the ionospheric fluctuations in the compressional component at CSES. This high correlation indicated the magnetospheric source of the Pi2 event. In addition, Pi2 is exhibited clearly in the ffiBy component at CSES, which is highly correlated with the ground H component, so the Pi2 event could be explained by the Substorm Current Wedge (SCW). This interpretation is further confirmed by checking the compressional component of Van Allen Probe (VAP) B satellite inside the plasmasphere, which, for the first time, gives observational support for an earlier model. This ULF wave observation shows the consistency and reliability of the high precision magnetometer (HPM) equipped by two fluxgate magnetometers (FGM1 and FGM2) onboard CSES.

    DOI: 10.3390/rs12142300

  • Normalized Polarization Ratio Analysis for ULF Precursor Detection of the 2009 M7.6 Sumatra and 2015 M6.8 Honshu Earthquakes

    Khairul Adib Yusof, Mardina Abdullah, Nurul Shazana Abdul Hamid, Suaidi Ahadi, Akimasa Yoshikawa

    Jurnal Kejuruteraan   3 ( 1 )   35 - 41   2020.4

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    Normalized Polarization Ratio Analysis for ULF Precursor Detection of the 2009 M 7.6 Sumatra and 2015 M 6.8 Honshu Earthquakes
    The utilization of geomagnetic field data especially in the ultra-low frequency range has been shown by prior studies to have the potential to detect earthquake precursors. The most widely used signal processing method for this purpose is arguably the polarization ratio analysis. In this paper, the method was improved by introducing a new normalization process with dissimilar ranges for the vertical and horizontal components. The normalized method was applied to geomagnetic field data that were recorded at locations near the earthquakes which had occurred in Sumatra, Indonesia on 30th September 2009 (M7.6) and Honshu, Japan on 12th May 2015 (M6.8) to evaluate the method's reliability and effectiveness in two different regions, i.e., the equatorial and mid-latitudinal regions. The results showed that the precursors obtained from the normalized method were less disturbed by random fluctuations and had more distinguishable amplitudes compared to the non-normalized classic method in both studied regions.

    DOI: 10.17576/jkukm-2020-si3(1)-06

  • 2018年8月の磁気嵐中の異なる縦セクターにおける長期昼間TEC強化の持続性【JST・京大機械翻訳】

    Li Qiaoling, Li Qiaoling, Li Qiaoling, Huang Fuqing, Huang Fuqing, Zhong Jiahao, Zhang Ruilong, Zhang Ruilong, Zhang Ruilong, Kuai Jiawei, Lei Jiuhou, Lei Jiuhou, Liu Libo, Liu Libo, Liu Libo, Liu Libo, Ren Dexin, Ren Dexin, Ma Han, Ma Han, Ma Han, Ma Han, Yoshikawa Akimasa, Hu Lianhuan, Hu Lianhuan, Hu Lianhuan, Guo Jiapeng, Li Wenbo, Li Wenbo, Li Wenbo, Li Wenbo, Zhou Xu, Zhou Xu, Zhou Xu, Zhou Xu, Cui Jun

    Journal of Geophysical Research: Space Physics   125 ( 11 )   2020.4

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    Persistence of the Long-Duration Daytime TEC Enhancements at Different Longitudinal Sectors During the August 2018 Geomagnetic Storm
    In this study, the ionospheric responses in the Asian-Australian, American, and African sectors during the August 2018 geomagnetic storm were investigated based on the Beidou geostationary orbit (GEO) satellite and Massachusetts Institute of Technology (MIT) Madrigal total electron contents (TECs), combined with measurements from ionosondes, magnetometers, and Global Ultraviolet Imager (GUVI). The middle- and low-latitude TECs were dominated by positive responses over the three longitudinal sectors during the storm on 26–29 August. It is unique that daytime TECs at the Asian-Australian, American, and African sectors displayed large enhancements larger than 10 TEC units (TECu) on 27–29 August, during the recovery phase, when the ionosphere is usually dominated by plasma depletions due to the ionospheric disturbance dynamo and/or disturbed thermospheric compositions. The combination and competition of the disturbed vertical plasma drifts through the solar wind-magnetosphere-ionosphere (SW-M-I) coupling and disturbed neutral compositions contribute significantly to the daytime TEC responses at different longitudinal sectors on 26 August during the main and early recovery phases. The eastward equatorial electrojet and O/N2 during the recovery phase on 27–29 August are larger than the quiet reference, which suggest that the enhanced upward vertical plasma drifts combining with higher O/N2 make an important contribution on the daytime positive ionospheric storm during the recovery phase. The enhanced vertical plasma drifts could not be driven by the SW-M-I coupling or ionospheric disturbance dynamo associated with the geomagnetic storm. Further studies should be untaken to explore the dominant sources for the enhanced upward vertical drifts during the recovery phase.

    DOI: 10.1029/2020JA028238

  • 2017年9月6日と10日の太陽フレアによる電離層電流変動【JST・京大機械翻訳】

    Owolabi Charles, Owolabi Charles, Lei Jiuhou, Lei Jiuhou, Lei Jiuhou, Bolaji O. S., Bolaji O. S., Ren Dexin, Ren Dexin, Ren Dexin, Yoshikawa Akimasa

    Space Weather   18 ( 11 )   2020.4

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    Ionospheric Current Variations Induced by the Solar Flares of 6 and 10 September 2017
    We examine the global ionospheric current in relation to X9.33 disk and X8.28 limb flares, which had significant differences in their solar X-ray and extreme ultraviolet (EUV) fluxes using the ground-based magnetometer data. At the peak of X9.33 flare, when X-ray and EUV radiations were significantly enhanced, the northern current vortex was situated at (40°N, 12 LT), while the southern current vortex was found at (30°S, 13LT). In comparison to the X8.28 flare, the northern current vortex was seen at (16°N, 12LT), while the southern current vortex was situated at (35°S, 14LT), which was 2 hr earlier in local time compared to those observed in the X9.33 flare. The changes in the total current intensity of the X9.33 flare is about 16&#37; less than that of the X8.28 flare, thus revealing that the current variations relative to both flares are due to solar flux and universal time variations. The daytime X9.33 flare northern current vortex is stronger, while the southern vortex is less intense than the corresponding vortex of X8.28 flare. Even though both flares happened in equinox, the current vortices are nearly symmetric. There were significant hemispheric changes in the focus position leading to the hemispheric asymmetry. Our results indicated that both the enhanced X-ray and EUV fluxes during flares could have impacts on the ionospheric electric field and current, but their relative contributions and the underlying physics need further investigations.

    DOI: 10.1029/2020SW002608

  • 東アジア地域における2013年の成層圏突然昇温に対する大気及び電離層応答の多装置観測【JST・京大機械翻訳】

    Chen Gang, Li Yaxian, Zhang Shaodong, Ning Baiqi, Gong Wanlin, Yoshikawa Akimasa, Hozumi Kornyanat, Tsugawa Takuya, Wang Zhihua

    IEEE Transactions on Geoscience and Remote Sensing   58 ( 2 )   1232 - 1243   2020.4

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    Multi-Instrument Observations of the Atmospheric and Ionospheric Response to the 2013 Sudden Stratospheric Warming Over Eastern Asia Region.
    We investigate the atmospheric and ionospheric response to the 2013 sudden stratospheric warming (SSW) by using multiple instruments located in Eastern Asia. Three meteor radars and five ionosondes are used to investigate the mesospheric zonal wind fields and ionospheric parameters of F -layer virtual height ( h 'F), F2-layer peak height ( h-{m} ext{F}-{2} ), and critical frequency ( f-{o} ext{F}-{2} ) at mid- and low-latitudes (10.7°N to 40.3°N). The vertical total electron content (TEC) data derived from the ground-based global positioning system receiver network are analyzed to study the ionospheric perturbations in the equatorial ionization anomaly (EIA) region. The changes in equatorial electrojet (EEJ) are observed by using the magnetometer data from stations on and off the magnetic equator. The variations of the h-{m} ext{F}-{2} at Sanya and EEJ strength presented the semidiurnal pattern with increase/decrease and eastward/westward currents in the morning/afternoon hours. In addition, the EIA crest moved poleward/equatorward in the morning/afternoon. The f-{o} ext{F}-{2} showed the most significant enhancements during daytime at Wuhan and Shaoyang but the f-{o} ext{F}-{2} at Sanya and Chumphon reduced mildly. Most importantly, based on the time-period wavelet analysis, the diurnal tidal components in the f-{o} ext{F}-{2} over Beijing, Wuhan, and Sanya seemed similar those in zonal winds and the semidiurnal tides in the low-latitude h-{m} ext{F}-{2} showed the similar temporal variations as those in EEJ strength during the later phase of SSW. Therefore, apart from the local tides propagating from lower atmosphere having influence on the mid- and low-latitude ionosphere directly during the early phase, the equatorial fountain effect modulated by the enhanced tides also disturbed the EIA region.

    DOI: 10.1109/TGRS.2019.2944677

  • 成層圏突然昇温時の地磁気日電流変動に関する研究【JST・京大機械翻訳】

    Owolabi Charles, Owolabi Charles, Lei Jiuhou, Lei Jiuhou, Bolaji O. S., Bolaji O. S., Jimoh Oluwaseyi, Jimoh Oluwaseyi, Ruan Haibing, Li Na, Li Na, Niu Xiaojuan, Yoshikawa Akimasa

    Journal of Geophysical Research: Space Physics   124 ( 7 )   6156 - 6172   2019.12

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    Investigation on the Variability of the Geomagnetic Daily Current During Sudden Stratospheric Warmings
    The magnetic field records of the magnetometer networks in the American, East Asian-Australian, and European-African sectors were employed in this present work. We used them to investigate equatorial electrojet (EEJ), counter electrojet (CEJ), tidal variability in EEJ strength and ionospheric current during the 2005/2006 and 2008/2009 sudden stratospheric warming (SSW) events. In addition to the well-investigated tidal variability in EEJ strength over the American and East Asian sectors, we investigated that of the African sector for the first time. Interestingly, the tidal components in EEJ strength during both SSW events clearly exhibit marked longitudinal differences with high, moderate, and low amplitudes in the American, East Asian, and African sectors, respectively. An exception found around day 71 in the African sector after the 2008/2009 SSW event had higher solar diurnal tidal component as compared to that of the Asian sector. Over the American sector, solar and lunar semidiurnal tides were strongly associated with CEJ current during both SSW events, whereas at the African and East Asian sectors such variabilities are not evident. A solar diurnal tidal component was strongly related to a reduction in the EEJ strength over the East Asian sector. In addition, a prolonged period of CEJ occurrence that begins during the SSW precondition and ends when the SSW was evolving characterized the African sector during both SSW events. There is a steady shift in phase at later hours when both SSW events are evolving.

    DOI: 10.1029/2019JA026667

  • 電離層Hall分極による電離層電位パターンの変形【JST・京大機械翻訳】

    Nakamizo Aoi, Yoshikawa Akimasa

    Journal of Geophysical Research: Space Physics   124 ( 9 )   7553 - 7580   2019.12

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    Deformation of Ionospheric Potential Pattern by Ionospheric Hall Polarization
    The present study shows that the ionospheric Hall polarization can deform the high-latitude ionospheric convection field, which is widely considered to be a manifestation of the convection field in the magnetosphere. We perform the Hall polarization field separation with a potential solver by changing the conductance distribution step by step from a uniform one to a more realistic one. We adopt dawn-dusk and north-south symmetric distributions of conductance and region 1 (R1) field-aligned current (FAC). The pair of the primary field of the R1 system and each gradient of off-diagonal component of conductance tensor (Hall conductance) generates the Hall polarization field and consequently causes potential deformations as follows. (a) The equatorward gradient causes clockwise rotation. (b) The gradient across the terminator, together with the effect of the equatorward gradient, causes the dawn-dusk asymmetry. (c) The high conductance band in the auroral region causes kink-type deformations. In particular, a nested structure at the equatorward edge of the band in the midnight sector well resembles the Harang Reversal. Result (a) can explain the clockwise bias inexplicable by the IMF-By effect alone, the combination of (a) and (b) can explain the clearness and unclearness in the round or crescent shapes of the dawn-dusk cells depending on the IMF-By polarity, and (c) suggests that the ionosphere may not need the upward-FAC for the formation of the Harang Reversal. We suggest that the final structure of the ionospheric potential is established by the combined effects of the magnetospheric requirements (external causes) and ionospheric polarization (internal effect).

    DOI: 10.1029/2018JA026013

  • Three Different Episodes of Prompt Equatorial Electric Field Perturbations Under Steady Southward IMF Bz During St. Patrick's Day Storm Reviewed

    S. Tulasi Ram, B. Nilam, N. Balan, Q. Zhang, K. Shiokawa, D. Chakrabarty, Z. Xing, K. Venkatesh, B. Veenadhari, A. Yoshikawa

    Journal of Geophysical Research: Space Physics   124 ( 12 )   10428 - 10443   2019.12

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    Three different episodes of prompt penetration electric field (PPEF) disturbances are observed during the main phase of the St. Patrick's Day storm on 17 March 2015 under steady southward interplanetary magnetic field (IMF) Bz conditions unlike the conventional PPEF associated with southward or northward turnings of IMF Bz. These PPEF events took place during the period when strong disturbance dynamo fields are prevailing in the background. The first event is triggered by a solar wind dynamic pressure pulse that caused a sharp eastward PPEF and strong enhancement of equatorial electrojet current in Brazilian dayside. The second event caused another short but strong westward PPEF on dayside due to the reversal of IMF By from duskward to dawnward under steady IMF Bz. The third event caused a longer eastward PPEF in association with a solar wind dynamic pressure pulse followed by the onset of a substorm, which has led to strong enhancement of equatorial electrojet, quick rejuvenation and symmetric redistribution of equatorial ionization anomaly in the Brazilian sector. The signatures of the PPEF with opposite polarity and smaller magnitudes are also observed in the Asian sector on the nightside. The possible mechanisms for the observed PPEF events under steady IMF Bz are discussed in terms of changes in the high-latitude field-aligned currents and reconfiguration of high-latitude convection fields using Active Magnetosphere and Planetary Electrodynamics Response Experiment and Super Dual Auroral Radar Network high-frequency radar observations.

    DOI: 10.1029/2019JA027069

  • Seasonal dependence of semidiurnal equatorial magnetic variation during quiet and disturbed periods

    Fujimoto, Akiko

    127   02025-1 - 02025-9   2019.11

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  • 静穏期および擾乱期中における半日周赤道磁気変動の季節的依存性

    FUJIMOTO Akiko, YOSHIKAWA Akimasa, UOZUMI Teiji, ABE Shuji

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   127   02025   2019.11

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    Seasonal dependence of semidiurnal equatorial magnetic variation during quiet and disturbed periods
    The analysis of 20-year long-term semidiurnal lunar tidal variations gave the evidence that the semidiurnal variations are completely different between the magnetic quiet and disturbed periods. This is the first time that the seasonal dependence of disturbance-time semidiurnal variation has been provided from the analysis of the EE-index. We found the Kp dependence of semidiurnal variation: For full and new moon phase, counter troughs are amplified during disturbance time, possibly related to disturbance dynamo. For all moon phase, there are positive enhancements in dawn and strong depressions after sunset, resulting from the penetration of polar electric filed. For Seasonal dependence, semidiurnal variations are divided to three seasonal groups, and characterized as deep trough, enhanced crest and weak structure for D-solstice, Equinoxes and J-solstice, respectively. There is no significant longitudinal difference between Ancon and Davao, except for the amplitude of semidiurnal variations. The deep troughs occur during D-solstice and the enhanced crests during Equinoxes, at both Ancon and Davao.

    DOI: 10.1051/e3sconf/201912702025

  • Application of solar quiet (Sq) current in determining mantle conductivity-depth structure in Malaysia Reviewed

    Zamri Zainal Abidin, M. H. Jusoh, M. Abbas, A. Yoshikawa

    Journal of Atmospheric and Solar-Terrestrial Physics   192   2019.10

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    The mantle electrical conductivity-depth structure of Malaysia was determined for the first time using solar quiet day ionospheric current (Sq) variations. Spherical harmonic analysis (SHA) was employed to separate the external and internal field contribution to the Sq variations. A transfer function was applied in estimating the conductivity-depth profile for the paired of external and internal coefficients of the SHA. We observed a downward increase in electrical conductivity with initial magnitude of 0.0065 S/m at a depth of ∼ 56 km which gradually rose to 0.0106 and 0.0140 S/m at 118 and 180 km. Subsequently, the conductivity profile rose to about 0.0228 S/m at 380 km (near the base of the upper mantle) and reached 0.0260 S/m at 435 km, after which a sharp steep increase was observed at 450 km with conductivity profile of 0.0278 S/m. Consequently, the conductivity profile increases significantly to about 0.1367 S/m at a depth of 973 km and reached its peak value 0.1975 S/m at the depth of 1097 km in the lower mantle with no indication of leveling off. An evidence of discontinuity was observed near 390–460 km and 675–746 km. A slight increase in conductivity values at depth between 150 and 300 km corresponds to the region of unusual global low velocity zone with high electrical conductivity. The conductivity profile showed a less steep increase above 450 km below which a steep increase was observed. The present profile showed the deepest penetration depth which may be attributed to the influence of equatorial electrojet current (EEJ) that is actively supported by the conductive properties of the Earth's interior within the study region.

    DOI: 10.1016/j.jastp.2018.01.019

  • Features of horizontal magnetic field intensity over northern island of Malaysia Reviewed

    M. Abbas, Zamri Zainal Abidin, M. H. Jusoh, O. S. Bolaji, A. Yoshikawa

    Indian Journal of Physics   93 ( 10 )   1247 - 1257   2019.10

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    This study utilized magnetic field records of the horizontal component obtained from magnetic data acquisition system at northern island of Malaysia to delineate the diurnal variations of SqH and their monthly mean MSqH for a period of 4 years. The results show that for the entire period of study, the daytime SqH amplitudes increase from ∼ 20 to ∼ 160 nT and their MSqH amplitudes increased from ∼ 40 to about 135 nT in 2008 to 2013, respectively. These variabilities of SqH and MSqH reached peak amplitudes between 10:00 and 12:00 LT hrs. The standard deviation fairly responds to the daily variability of SqH with a phase shift in January 2008 and 2013 which may likely have connection to the sudden stratospheric warming event that occurred in these months. We observed the extension of eastward field that continued beyond the sunset (18:00 LT) hours is more prevalent with higher magnitudes during the deep minimum solar activity and the probable causes are discussed. The observed counter equatorial electrojet associated with late reversal of night-time westward electric field (WEF) shows inverse relationship with increasing solar activity and those that are not associated to late reversal of night-time WEF seems to indicate linear relationship exception of deep minimum solar activity year (2008). We also observed a gradual shift of ECEJ to the morning sector with increasing solar activity. Throughout the years, days with stronger morning counter equatorial electrojet magnitudes generally weaken the expected strong eastward current and shifted its peak to earlier local time. The annual and seasonal variations of SqH show semiannual variation with equinoctial maxima and solstitial minima. About 40&#37; of the SqH shows positive night-time to pre-sunrise variations which suggest the existence of weak electric currents not necessarily of ionospheric origin with appreciable influence at this longitude sector. The extension of eastward field beyond the sunset hours suggests likely modification of the evening side ionosphere over this region.

    DOI: 10.1007/s12648-019-01388-9

  • Assessment of signal processing methods for geomagnetic precursor of the 2012 M6.9 Visayas, Philippines earthquake

    Khairul Adib Yusof, Nurul Shazana Abdul Hamid, Mardina Abdullah, Suaidi Ahadi, Akimasa Yoshikawa

    Acta Geophysica   67 ( 5 )   1297 - 1306   2019.10

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    Assessment of signal processing methods for geomagnetic precursor of the 2012 M6.9 Visayas, Philippines earthquake
    Abstract: This study assessed two signal processing methods on geomagnetic data to detect precursory signals appearing before the M6.9 Visayas, Philippines earthquake on 6 February 2012. It aimed to compare the polarization ratio analysis method with the diurnal variation ratio method in terms of reliability and effectiveness. The geomagnetic data were obtained from the MAGDAS magnetometer network for Cebu (CEB) and Legazpi (LGZ) stations which served as the primary and remote stations, respectively. The polarization ratio analysis method was performed on the primary station data to obtain power spectral density in an ultra-low-frequency range before finding the ratio of vertical to total horizontal component. Meanwhile, the diurnal variation ratio method was used to calculate the difference between the daily maximum and minimum values. Then, the ratio of the daily differences of the primary station to the remote station for each individual component was calculated. The disturbance storm time index which describes global geomagnetic activity originating from the Sun was utilized to verify that any observed geomagnetic fluctuations were not caused by solar-terrestrial effect. A precursory anomaly was found using the polarization ratio analysis method which appeared 2 weeks before the earthquake. It is concluded that this method might be effective and reliable in detecting geomagnetic anomalies preceding upcoming earthquakes. In contrast, although the diurnal variation ratio method did show perceivable fluctuations, the running averages were not statistically significant to be considered a precursor. The discrepancy between the analytical results of the two methods may be attributed to the detectability of the earthquake being studied which had a relatively low magnitude. Hence, future studies which utilize more earthquake events need to be conducted to reach a definitive conclusion. Graphic abstract: [Figure not available: see fulltext.].

    DOI: 10.1007/s11600-019-00319-w

  • Features of the inter-hemispheric field-aligned current system over Malaysia ionosphere Reviewed

    Zamri Zainal Abidin, M. H. Jusoh, M. Abbas, O. S. Bolaji, A. Yoshikawa

    Journal of Atmospheric and Solar-Terrestrial Physics   192   2019.10

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    Magnetic records of the declination (D) component for the solar quiet year 2011–2013 obtained from Magnetic Data Acquisition System (MAGDAS) at Langkawi (Geog. Lon. 99.68∘ E, Geog. Lat. 6.30∘N), Malaysia were utilized in this study. The minutes averages were used to delineate the diurnal (Sq(D)) variation. The monthly mean (MSq(D)) and their seasonal variabilities (SVq(D)) were also analysed. The Sq(D) and their MSq(D) exhibit smooth regular occurring pattern in the month of April–September and became highly perturbed in October–March across the years. The highest positive (∼3.5 arc-min) and the negative (∼−3.0 arc-min) values were observed in August 2011 during the dawn and noon sectors. These maxima shifted to July and September in 2012 with peaks ∼3.2 and −3.0 arc-min. In 2013, the positive maximum (∼3.0 arc-min) and its negative (∼−2.5 arc-min) were again seen in August. This implies that the dawn and noon sectors of August 2011 and 2013 are strongly influenced by IHFACs and this effect shifted to July and September in 2012. IHFACs through the years flow from the winter to summer hemisphere during the noon and dusk sectors and flow in opposite direction during the dawn sector. The day-to-day magnitudes of Sq(D) and MSq(D) seems to suggest the inter-hemispheric imbalance of the ionospheric Sq current earlier established by Van Sabben as the cause of IHFACs is not strongly affected by the changes in annual solar variation. Dusk-side IHFACs were observed to be northbound in all the seasons with the exception of June solstice. The direction of IHFACs does not change except in April and November. The current intensity is not large in solstices except in August 2011 and 2013 but it shifted to July in 2012. The result further showed that the magnitude of the duskside IHFACS is determined to some extent by the strength of the noontime IHFACs. IHFACs were generally observed to be greater during the daytime than night-time hours.

    DOI: 10.1016/j.jastp.2018.01.012

  • Longitudinal profile of equatorial electrojet derived from ground and satellite based magnetometers

    Wan Nur Izzaty Ismail, Nurul Shazana Abdul Hamid, Mardina Abdullah, Akimasa Yoshikawa

    2018 UKM FST Postgraduate Colloquium 2018 UKM FST Postgraduate Colloquium Proceedings of the Universiti Kebangsaan Malaysia, Faculty of Science and Technology 2018 Postgraduate Colloquium   2019.6

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    The intense current that flowing eastward in the dayside in the E layer of ionosphere at dip equator region is known as equatorial electrojet (EEJ). In this work, we attempt to compare the longitudinal profile of EEJ current estimated from the Challenging Minisatellite Payload (CHAMP) and European Space Agency satellite (SWARM) with the ground-based magnetometer network from six equatorial observatory pairs across the globe. Ground magnetometer were obtained from the network such as MAGDAS, INTERMAGNET and IIG. We process our data using the EUEL index during quiet days for ground measurement. Then, correlation coefficient were obtained after applying appropriate normalization techniques for both measurements. Analysis showed the longitudinal variations of EEJ current from ground indicates that this current was strongest at South American (77 °W) and Southeast Asian (99.78°E). Meanwhile, satellite measurement shows four peaks of EEJ current at -100°W, 0°E, 100°E and 180° E which are at North America, Atlantic ocean, Southeast Asian and Pacific ocean respectively.

    DOI: 10.1063/1.5111232

  • Statistical study of equatorial geomagnetic crochets

    Norhani Muhammad Nasir Annadurai, Nurul Shazana Abdul Hamid, Akimasa Yoshikawa

    2018 UKM FST Postgraduate Colloquium 2018 UKM FST Postgraduate Colloquium Proceedings of the Universiti Kebangsaan Malaysia, Faculty of Science and Technology 2018 Postgraduate Colloquium   2019.6

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    This study present the statistical investigation of equatorial geomagnetic crochets due to strong solar flare of class M to X. Our analysis utilized data from eight magnetometer stations provided by MAGnetic Data Acquisition System network (MAGDAS) at different longitudes sector during period from January 2008 to March 2015. We have considered 52 cases of solar flare events. Based on our analysis, 65% of the studied solar flares show no effect on geomagnetic variation with most of it from class M8, M9 and X1. The absence of solar flare effect might due to the influence of coronal mass ejection (CME) on the observation data or due to the station's location is at nighttime. The other 35% shows geomagnetic crochets to the magnetic data variation where majority are mix effect dominated by positive crochets. Apart from that, we also found an interesting solar flare effect where negative geomagnetic crochets were detected from all equatorial magnetometer data. The unique effect is due to X-class solar flare on 9th August 2011. Further investigation using extended latitudinal and longitudinal magnetometer is recommended to observe the whole picture of the solar flare effect to global ionospheric current.

    DOI: 10.1063/1.5111233

  • Magnetic Data Acquisition System (MAGDAS) Malaysia: installation and preliminary data analysis at ESERI, UNISZA Reviewed

    R. Umar, S. F. Natasha, S. S.N. Aminah, K. N. Juhari, M. H. Jusoh, N. S.A. Hamid, M. H. Hashim, Z. M. Radzi, A. N. Ishak, S. N. Hazmin, W. Z.A.W. Mokhtar, M. K.A. Kamarudin, H. Juahir, A. Yoshikawa

    Indian Journal of Physics   93 ( 5 )   553 - 564   2019.5

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    Magnetic Data Acquisition System (MAGDAS) is a magnetometer initiated by the International Center for Space Weather Science and Education in Kyushu University, Japan, to study space weather. The latest of real-time Magnetic Data Acquisition System/Circum-pan Pacific Magnetometer Network was successfully installed at the East Coast Environmental Research Institute in Universiti Sultan Zainal Abidin, Terengganu, Malaysia, by Kyushu University. This is the fifth magnetometer under the MAGDAS network (geographic latitude and longitude: 5.23°, 103.04° and geomagnetic latitude and longitude: − 4.21°, 175.91°). In this study, the results of data plot obtained at Terengganu (TRE) station were shown to have reliable patterns of geomagnetic elements. The amplitude variations for each component were also proximate with other stations and a standard model. This study compared MAGDAS-II data for the H component with solar wind data (input energy, IMF, dynamic pressure and speed).

    DOI: 10.1007/s12648-018-1318-x

  • Statistical Study of Selective Oxygen Increase in High-Energy Ring Current Ions During Magnetic Storms Reviewed

    K. Mitani, K. Seki, K. Keika, M. Gkioulidou, L. J. Lanzerotti, D. G. Mitchell, C. A. Kletzing, A. Yoshikawa, Y. Obana

    Journal of Geophysical Research: Space Physics   124 ( 5 )   3193 - 3209   2019.5

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    Ion transport from the plasma sheet to the ring current is the main cause of the development of the ring current. Energetic (>150 keV) ring current ions are known to be transported diffusively in several days. A recent study suggested that energetic oxygen ions are transported closer to the Earth than protons due to the diffusive transport caused by a combination of the drift and drift-bounce resonances with Pc 3–5 ultralow frequency waves during the 24 April 2013 magnetic storm. To understand the occurrence conditions of such selective oxygen increase (SOI), we investigate the phase space densities (PSDs) between protons and oxygen ions with the first adiabatic invariants (μ) of 0.1–2.0 keV/nT measured by the Radiation Belt Storm Probes Ion Composition Experiment instrument on the Van Allen Probes at L ~ 3–6 during 90 magnetic storms in 2013–2017. We identified the SOI events in which oxygen PSDs increase while proton PSDs do not increase during a period of ~9 hr (one orbital period). Among the 90 magnetic storms, 33&#37; were accompanied by the SOI events. Global enhancements of Pc 4 and Pc 5 waves observed by ground magnetometers during the SOI events suggest that radial transport due to combination of the drift-bounce resonance with Pc 4 oscillations and the drift resonance with Pc 5 oscillations can be the cause of SOIs. The contribution of the SOI events to the magnetic storm intensity is roughly estimated to be ~9&#37; on average.

    DOI: 10.1029/2018JA026168

  • 2017年9月の嵐に対する電離圏-プラズマ圏結合の応答 プラズマ圏は何が激しいのか?【JST・京大機械翻訳】 Reviewed

    Obana Yuki, Maruyama Naomi, Maruyama Naomi, Shinbori Atsuki, Hashimoto Kumiko K., Fedrizzi Mariangel, Fedrizzi Mariangel, Nose Masahito, Otsuka Yuichi, Nishitani Nozomu, Hori Tomoaki, Kumamoto Atsushi, Tsuchiya Fuminori, Matsuda Shoya, Matsuoka Ayako, Kasahara Yoshiya, Yoshikawa Akimasa, Miyoshi Yoshizumi, Shinohara Iku

    Space Weather   17 ( 6 )   861 - 876   2019.4

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    Response of the Ionosphere-Plasmasphere Coupling to the September 2017 Storm: What Erodes the Plasmasphere so Severely?
    We report an extreme erosion of the plasmasphere arising from the September 2017 storm. The cold electron density is identified from the upper limit frequency of upper hybrid resonance waves observed by the Plasma Wave Experiment instrument onboard the Exploration of energization and Radiation in Geospace/Arase satellite. The electron density profiles reveal that the plasmasphere was severely eroded during the recovery phase of the storm and the plasmapause was located at L = 1.6–1.7 at 23 UT 8 September 2017. This is the first report of deep erosion of the plasmasphere (LPP < 2) with the in situ observation of the electron density. The degree of the severity is much more than what is expected from the relatively moderate value of the SYM-H minimum (−146 nT). We attempt to find a possible explanation for the observed severe depletion by using both observational evidence and numerical simulations. Our results suggest that the middle latitude electric field had penetrated from the high-latitude storm time convection for several hours. Such an unusually long-lasting penetration event can cause this observed degree of severity.

    DOI: 10.1029/2019SW002168

  • 赤道の地磁気時計の統計的研究【JST・京大機械翻訳】

    Annadurai Norhani Muhammad Nasir, Hamid Nurul Shazana Abdul, Yoshikawa Akimasa

    AIP Conference Proceedings   2111 ( 1 )   2019.4

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    Statistical study of equatorial geomagnetic crochets
    This study present the statistical investigation of equatorial geomagnetic crochets due to strong solar flare of class M to X. Our analysis utilized data from eight magnetometer stations provided by MAGnetic Data Acquisition System network (MAGDAS) at different longitudes sector during period from January 2008 to March 2015. We have considered 52 cases of solar flare events. Based on our analysis, 65&#37; of the studied solar flares show no effect on geomagnetic variation with most of it from class M8, M9 and X1. The absence of solar flare effect might due to the influence of coronal mass ejection (CME) on the observation data or due to the station's location is at nighttime. The other 35&#37; shows geomagnetic crochets to the magnetic data variation where majority are mix effect dominated by positive crochets. Apart from that, we also found an interesting solar flare effect where negative geomagnetic crochets were detected from all equatorial magnetometer data. The unique effect is due to X-class solar flare on 9th August 2011. Further investigation using extended latitudinal and longitudinal magnetometer is recommended to observe the whole picture of the solar flare effect to global ionospheric current.

    DOI: 10.1063/1.5111233

  • 地上および衛星ベース磁力計から導出した赤道エレクトロジェットの縦方向プロファイル【JST・京大機械翻訳】

    Ismail Wan Nur Izzaty, Hamid Nurul Shazana Abdul, Abdullah Mardina, Yoshikawa Akimasa

    AIP Conference Proceedings   2111 ( 1 )   2019.4

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    Longitudinal profile of equatorial electrojet derived from ground and satellite based magnetometers
    The intense current that flowing eastward in the dayside in the E layer of ionosphere at dip equator region is known as equatorial electrojet (EEJ). In this work, we attempt to compare the longitudinal profile of EEJ current estimated from the Challenging Minisatellite Payload (CHAMP) and European Space Agency satellite (SWARM) with the ground-based magnetometer network from six equatorial observatory pairs across the globe. Ground magnetometer were obtained from the network such as MAGDAS, INTERMAGNET and IIG. We process our data using the EUEL index during quiet days for ground measurement. Then, correlation coefficient were obtained after applying appropriate normalization techniques for both measurements. Analysis showed the longitudinal variations of EEJ current from ground indicates that this current was strongest at South American (77 °W) and Southeast Asian (99.78°E). Meanwhile, satellite measurement shows four peaks of EEJ current at -100°W, 0°E, 100°E and 180° E which are at North America, Atlantic ocean, Southeast Asian and Pacific ocean respectively.

    DOI: 10.1063/1.5111232

  • Variation of equatorial electrojet current profiles over Solar Phases Reviewed

    W. N.I. Ismail, N. S.A. Hamid, M. Abdullah, N. H.M. Shukur, A. Yoshikawa

    ASM Science Journal   12 ( Special Issue 2 )   125 - 133   2019.4

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    Equatorial electrojet (EEJ) current is an intense eastward electric current flowing at about 100- 120km altitude within ±3° latitude in E region of the equatorial ionosphere. This study reported dependence of EEJ longitudinal profile on the three phases of solar cycle 24 (SC-24). The analysis was carried out using EUEL index, calculated from the northward H component of geomagnetic field. This work utilised data from various ground-based magnetometer networks such as MAGDAS, INTERMAGNET and IIG. The results of this study showed that the highest and lowest value of EEJ longitudinal profiles varies with solar phases. The nature of the longitudinal disparity in the EEJ strength indicates that it is strongest in American sector and lowest in African sector during solar minimum in 2008. However, during solar maximum in 2013 the highest EEJ intensity was recorded in Southeast Asian sector. On the other hand, the lowest value of EEJ current was recorded in African sector in 2008 which was found to be shifting to Indian sector started in 2011. In addition, we discovered the transition point of the highest value of EEJ started in 2012, while the transition point of minimum value EEJ started in 2010.

  • Response of Ionospheric Profile Parameters to Equatorial Electrojet Over Peruvian Station Reviewed

    S. A. Bello, M. Abdullah, N. S.A. Hamid, B. W. Reinisch, A. Yoshikawa, A. Fujimoto

    Earth and Space Science   6 ( 4 )   617 - 628   2019.4

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    The response of the ionospheric bottomside electron density profile parameters of the F2 layer, namely, the maximum electron density (NmF2), the maximum height of F2 layer (hmF2), and bottomside thickness (B0) parameter to the equatorial electrojet (EEJ) current is examined for a Peruvian location at the Jicamarca station (12 °S, 76.9 °W) in the South American sector. The results of the analysis show that both hmF2 and B0 increase for ~2 h before sunrise and exhibit a postsunset peak during the equinoctial and summer months. The increase in the peak height, hmF2, is observed to terminate before midday, while B0 continued to increase throughout the daytime. The apparent midday and postnoon peaks in NmF2 occur in all the seasons under study. It was demonstrated that a relationship exists between EEJ and the profile parameters hmF2 and B0 during low and moderate solar conditions. Conversely, the correlation coefficient between EEJ and NmF2 is statistically significant only during solar minimum conditions but correlates poorly, if at all, with EEJ during moderate solar activity.

    DOI: 10.1029/2018EA000537

  • 太陽周期24期間中の赤道対向ジェットの縦方向変動【JST・京大機械翻訳】 Reviewed

    Soares Gabriel, Yamazaki Yosuke, Matzka Juergen, Pinheiro Katia, Stolle Claudia, Stolle Claudia, Alken Patrick, Alken Patrick, Yoshikawa Akimasa, Uozumi Teiji, Fujimoto Akiko, Kulkarni Atul

    Studia Geophysica et Geodaetica   63 ( 2 )   304 - 319   2019.4

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    Longitudinal variability of the equatorial counter electrojet during the solar cycle 24
    Ground and space-based geomagnetic data were used in the investigation of the longitudinal, seasonal and lunar phase dependence of the equatorial counter electrojet (CEJ) occurrence in the Peruvian, Brazilian, African, Indian and Philippine sectors during geomagnetically quiet days from the solar cycle 24 (2008 to 2018). We found that CEJ events occur more frequently during the morning (MCEJ) than in the afternoon (ACEJ). The highest MCEJ and ACEJ occurrence rates were observed for the Brazilian sector. Distinct seasonal dependence was found for each longitudinal sector under investigation. The lunar phase dependence was determined for the first time for the Philippine sector (longitude 125°E), and it was shown to be less pronounced than in the Peruvian, Brazilian and African sectors. We demonstrate that differences in CEJ rates derived from ground-based and satellite data can arise from the longitudinal separation between low-latitude and equatorial stations that are used to determine the signal and its consequent time delay in their sunrise/sunset times at ionospheric heights.

    DOI: 10.1007/s11200-018-0286-0

  • Relationship between plasma bubble and ionospheric current, equatorial electrojet, and equatorial counter electrojet Reviewed

    T. Akiyama, A. Yoshikawa, A. Fujimoto, T. Uozumi

    Journal of Physics: Conference Series   1152 ( 1 )   2019.3

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    In recent years, it has been clarified from previous studies that plasma bubbles and equatorial electrojets (EEJs) are related. In general, EEJs are calculated by subtracting the magnetic field H component of the magnetic equator from that at low latitude. However, in this study, EE-index data at Langkawi (magnetic equator), which includes all local current systems, were used for the analysis during the period from January 1, 2011, to November 8, 2014. By using the EE-index, it was found that plasma bubbles tend to occur for larger EEJ strengths. This result differs from the previous studies. In addition, if an equatorial counter electrojet (CEJ) occurs, it is understood that plasma bubbles will rarely occur due to the westward current; however, we found that when the lunar tidal effect is strong, plasma bubbles can occur even in conjunction with CEJs. Finally, we want to find the relationship between plasma bubbles and ionospheric current to predict them.

    DOI: 10.1088/1742-6596/1152/1/012022

  • The first solar-powered Magdas-9 installation and possible geomagnetically induced currents study at Johor, Malaysia Reviewed

    Zatul Iffah Abd Latiff, Mohamad Huzaimy Jusoh, Farah Adilah Mohd Kasran, Siti Amalina Enche Ab Rahim, Munirah Onn, Aznilinda Zainuddin, Muhammad Asraf Hairuddin, Nurhani Kasuan, Muhammad Muzamil Mustam, Suhana Mohamed, Yoshikawa Akimasa

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018 Journal of Physics: Conference Series   1152 ( 1 )   2019.3

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    The Magnetic Data Acquisition System (MAGDAS-9) was successfully installed at Universiti Teknologi MARA Johor, Pasir Gudang Campus, Malaysia (JOH station), under the joint collaboration between International Center for Space Weather Science and Education (ICSWSE), National Space Agency (ANGKASA) and UiTM Johor. This is the first solar-powered magnetometer under the Magnetic Data Acquisition System of Circum-pan Pacific Magnetometer Network (MAGDAS/CPMN). In this paper, construction process, installation process and analysis of first geomagnetic observations at MAGDAS JOH station are presented. In addition, analysis on time derivative of horizontal component of geomagnetic field (dH/dt) to indicate the possibility of Geomagnetically Induced Currents (GIC) occurrences is also presented in this paper. The obtained geomagnetic components: H, D, Z and Total F are approximately similar to World Magnetic Model 2015 (WMM2015) while the diurnal variation from this geomagnetic observation showing a good variation pattern. The analysis of dH/dt has indicated 2 significant events of GIC.

    DOI: 10.1088/1742-6596/1152/1/012030

  • Relationship between plasma bubble and ionospheric current, equatorial electrojet, and equatorial counter electrojet Reviewed

    T. Akiyama, A. Yoshikawa, A. Fujimoto, T. Uozumi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018 Journal of Physics: Conference Series   1152 ( 1 )   2019.3

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    In recent years, it has been clarified from previous studies that plasma bubbles and equatorial electrojets (EEJs) are related. In general, EEJs are calculated by subtracting the magnetic field H component of the magnetic equator from that at low latitude. However, in this study, EE-index data at Langkawi (magnetic equator), which includes all local current systems, were used for the analysis during the period from January 1, 2011, to November 8, 2014. By using the EE-index, it was found that plasma bubbles tend to occur for larger EEJ strengths. This result differs from the previous studies. In addition, if an equatorial counter electrojet (CEJ) occurs, it is understood that plasma bubbles will rarely occur due to the westward current; however, we found that when the lunar tidal effect is strong, plasma bubbles can occur even in conjunction with CEJs. Finally, we want to find the relationship between plasma bubbles and ionospheric current to predict them.

    DOI: 10.1088/1742-6596/1152/1/012022

  • Electromagnetic induction responses to geomagnetic disturbances at low-and-mid-latitudes Reviewed

    Mio Nakahara, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018 Journal of Physics: Conference Series   1152 ( 1 )   2019.3

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    The geomagnetically induced current (GIC) is one of the most widely recognized phenomena caused by geomagnetic disturbances. Realistic predictions of magnetic field fluctuations may be used to evaluate the induction of electric fields to ground surfaces, and thus to estimate the occurrence of GICs. Although many GICs occur at high latitudes, they are now being studied at low and mid-latitudes as well. The purpose of this research was to understand the dynamics, observation, and prediction in Japan for GICs occurring at the low and mid-latitudes. In this study, the influence of geomagnetic field variations on Earth's electric field was examined. The magnetic field and the electric field components of 3 observation points for 1 year in 2015 are visually examined, and the characteristics of the fluctuations of the magnetic field and the surface electrical field were also analysed.

    DOI: 10.1088/1742-6596/1152/1/012035

  • Characteristic of the Disturbed Days Ionospheric Current System in the 180-Degree Magnetic Meridian Reviewed

    Siti Nurbaiti Ibrahim, Mohammad Huzaimy Jusoh, Ahmad Asari Sulaiman, Akimasa Yoshikawa, Zahira Mohd Radzi

    Journal of Physics: Conference Series   1152 ( 1 )   2019.3

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    The behavior of the ionospheric current during disturbed days using 10 geomagnetic observatories along 180-degree magnetic meridian was analysed. Separation of external and internal current during geomagnetic storm on 12 April until 15 April 2012 data was carried out using spherical harmonic analysis method. The contour of day to day variation of total current, external current and internal current were distinguished based on geomagnetic storm phase. These current then were correlate with the solar wind parameter, IMF Bz, and geomagnetic indices in order to identify their relationship. The results reveal that these current intensities were found higher during the initial phase. This due to the enhancement of the magnetic field during the initial phase caused by the increment of solar wind dynamic pressure and southward IMF Bz. Hence, the induced current identified in the internal current. This study demonstrated that the electric current induction can be obtained from the weak geomagnetic storm.

    DOI: 10.1088/1742-6596/1152/1/012029

  • Assessment of the Geomagnetically Induced Current (GIC) at Low Latitude Region based on MAGDAS Data Reviewed

    N. Mohd Anuar, F. A. Mohd Kasran, M. Abbas, M. H. Jusoh, S. A. Enche Ab Rahim, N. Abdul Hadi, A. Yoshikawa, Z. Mohd Radzi

    Journal of Physics: Conference Series   1152 ( 1 )   2019.3

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    The geomagnetically induced current (GICs) impact is no longer concentrated at high latitude region strictly. The objective of this study was to extend the GICs observation conducted at equatorial region using geomagnetic data extracted from magnetometer installed at Langkawi National Observatory (LNO), Malaysia for the long-term analysis involving the solar cycle 24. The observation is now continued with the GICs comparison between LKW stations with five low latitude station which is BCL, PTN, MND, DAW, and TWV obtained from the magnetic data acquisition system (MAGDAS). The assessment of the GICs behavior revealed the possibility of LKW station experiences GICs is high, based on the time derivative of the horizontal component (dH/dt) value. Extend from that, the GICs estimation was successful done by applying the plane wave method as a model to calculate the North-South and the East-West component, Ex and Ey respectively. The equation of the GICs was provided by excluding the topology constant parameters, which is a and b constant and the value of the underground conductivity for low latitude station. Subsequently, the comparison was limited in years of 2008 - 2014 due to insufficient geomagnetic data. Indeed, the GICs calculation is able to derive the GICs estimation and showed a good agreement with the corresponding value of the time derivative of the horizontal component. However, the accurate current value (A) is able to gain by conducting a direct measurement of the high voltage power transmission system.

    DOI: 10.1088/1742-6596/1152/1/012028

  • The first solar-powered Magdas-9 installation and possible geomagnetically induced currents study at Johor, Malaysia Reviewed International journal

    Zatul Iffah Abd Latiff, Mohamad Huzaimy Jusoh, Farah Adilah Mohd Kasran, Siti Amalina Enche Ab Rahim, Munirah Onn, Aznilinda Zainuddin, Muhammad Asraf Hairuddin, Nurhani Kasuan, Muhammad Muzamil Mustam, Suhana Mohamed, Yoshikawa Akimasa

    Journal of Physics: Conference Series   1152 ( 1 )   012030   2019.3

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    The first solar-powered Magdas-9 installation and possible geomagnetically induced currents study at Johor, Malaysia
    The Magnetic Data Acquisition System (MAGDAS-9) was successfully installed at Universiti Teknologi MARA Johor, Pasir Gudang Campus, Malaysia (JOH station), under the joint collaboration between International Center for Space Weather Science and Education (ICSWSE), National Space Agency (ANGKASA) and UiTM Johor. This is the first solar-powered magnetometer under the Magnetic Data Acquisition System of Circum-pan Pacific Magnetometer Network (MAGDAS/CPMN). In this paper, construction process, installation process and analysis of first geomagnetic observations at MAGDAS JOH station are presented. In addition, analysis on time derivative of horizontal component of geomagnetic field (dH/dt) to indicate the possibility of Geomagnetically Induced Currents (GIC) occurrences is also presented in this paper. The obtained geomagnetic components: H, D, Z and Total F are approximately similar to World Magnetic Model 2015 (WMM2015) while the diurnal variation from this geomagnetic observation showing a good variation pattern. The analysis of dH/dt has indicated 2 significant events of GIC.

    DOI: 10.1088/1742-6596/1152/1/012030

  • Electromagnetic induction responses to geomagnetic disturbances at low-and-mid-latitudes Reviewed

    Mio Nakahara, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto

    Journal of Physics: Conference Series   1152 ( 1 )   2019.3

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    The geomagnetically induced current (GIC) is one of the most widely recognized phenomena caused by geomagnetic disturbances. Realistic predictions of magnetic field fluctuations may be used to evaluate the induction of electric fields to ground surfaces, and thus to estimate the occurrence of GICs. Although many GICs occur at high latitudes, they are now being studied at low and mid-latitudes as well. The purpose of this research was to understand the dynamics, observation, and prediction in Japan for GICs occurring at the low and mid-latitudes. In this study, the influence of geomagnetic field variations on Earth's electric field was examined. The magnetic field and the electric field components of 3 observation points for 1 year in 2015 are visually examined, and the characteristics of the fluctuations of the magnetic field and the surface electrical field were also analysed.

    DOI: 10.1088/1742-6596/1152/1/012035

  • Characteristic of the Disturbed Days Ionospheric Current System in the 180-Degree Magnetic Meridian Reviewed International journal

    Siti Nurbaiti Ibrahim, Mohammad Huzaimy Jusoh, Ahmad Asari Sulaiman, Akimasa Yoshikawa, Zahira Mohd Radzi

    Journal of Physics: Conference Series   1152 ( 1 )   2019.1

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    The behavior of the ionospheric current during disturbed days using 10 geomagnetic observatories along 180-degree magnetic meridian was analysed. Separation of external and internal current during geomagnetic storm on 12 April until 15 April 2012 data was carried out using spherical harmonic analysis method. The contour of day to day variation of total current, external current and internal current were distinguished based on geomagnetic storm phase. These current then were correlate with the solar wind parameter, IMF Bz, and geomagnetic indices in order to identify their relationship. The results reveal that these current intensities were found higher during the initial phase. This due to the enhancement of the magnetic field during the initial phase caused by the increment of solar wind dynamic pressure and southward IMF Bz. Hence, the induced current identified in the internal current. This study demonstrated that the electric current induction can be obtained from the weak geomagnetic storm.

    DOI: 10.1088/1742-6596/1152/1/012028

  • Modeling Geomagnetically Induced Currents in Australian Power Networks Using Different Conductivity Models Reviewed

    R. A. Marshall, L. Wang, G. A. Paskos, G. Olivares-Pulido, T. Van Der Walt, C. Ong, D. Mikkelsen, G. Hesse, B. McMahon, E. Van Wyk, G. Ivanovich, D. Spoor, C. Taylor, A. Yoshikawa

    Space Weather   2019.1

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    Space weather manifests in power networks as quasi-DC currents flowing in and out of the power system through the grounded neutrals of high-voltage transformers, referred to as geomagnetically induced currents. This paper presents a comparison of modeled geomagnetically induced currents, determined using geoelectric fields derived from four different impedance models employing different conductivity structures, with geomagnetically induced current measurements from within the power system of the eastern states of Australia. The four different impedance models are a uniform conductivity model (UC), one-dimensional n-layered conductivity models (NU and NW), and a three-dimensional conductivity model of the Australian region (3DM) from which magnetotelluric impedance tensors are calculated. The modeled 3DM tensors show good agreement with measured magnetotelluric tensors obtained from recently released data from the Australian Lithospheric Architecture Magnetotelluric Project. The four different impedance models are applied to a network model for four geomagnetic storms of solar cycle 24 and compared with observations from up to eight different locations within the network. The models are assessed using several statistical performance parameters. For correlation values greater than 0.8 and amplitude scale factors less than 2, the 3DM model performs better than the simpler conductivity models. When considering the model performance parameter, P, the highest individual P value was for the 3DM model. The implications of the results are discussed in terms of the underlying geological structures and the power network electrical parameters.

    DOI: 10.1029/2018SW002047

  • Investigation on the Variability of the Geomagnetic Daily Current During Sudden Stratospheric Warmings Reviewed

    Charles Owolabi, Jiuhou Lei, O. S. Bolaji, Oluwaseyi Jimoh, Haibing Ruan, Na Li, Xiaojuan Niu, Akimasa Yoshikawa

    Journal of Geophysical Research: Space Physics   124 ( 7 )   6156 - 6172   2019.1

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    The magnetic field records of the magnetometer networks in the American, East Asian-Australian, and European-African sectors were employed in this present work. We used them to investigate equatorial electrojet (EEJ), counter electrojet (CEJ), tidal variability in EEJ strength and ionospheric current during the 2005/2006 and 2008/2009 sudden stratospheric warming (SSW) events. In addition to the well-investigated tidal variability in EEJ strength over the American and East Asian sectors, we investigated that of the African sector for the first time. Interestingly, the tidal components in EEJ strength during both SSW events clearly exhibit marked longitudinal differences with high, moderate, and low amplitudes in the American, East Asian, and African sectors, respectively. An exception found around day 71 in the African sector after the 2008/2009 SSW event had higher solar diurnal tidal component as compared to that of the Asian sector. Over the American sector, solar and lunar semidiurnal tides were strongly associated with CEJ current during both SSW events, whereas at the African and East Asian sectors such variabilities are not evident. A solar diurnal tidal component was strongly related to a reduction in the EEJ strength over the East Asian sector. In addition, a prolonged period of CEJ occurrence that begins during the SSW precondition and ends when the SSW was evolving characterized the African sector during both SSW events. There is a steady shift in phase at later hours when both SSW events are evolving.

    DOI: 10.1029/2019JA026667

  • Estimation of time derivative of horizontal geomagnetic component for GIC assesment in Malaysia during quiet period

    Nornabilah Mohd Anuar, Farah Adilah Mohd Kasran, Zatul Iffah Abdul Latif, Siti Amalina Ence Ab Rahim, Arif Manut, Mohamad Huzaimy Jusoh, Normi Abdul Hadi, Akimasa Yoshikawa

    8th International Conference on System Engineering and Technology, ICSET 2018 ICSET 2018 - 2018 IEEE 8th International Conference on System Engineering and Technology, Proceedings   118 - 122   2019.1

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    This paper presents the preliminary observation on the possible Geomagnetic Induced Current (GIC) activities at Malaysia region during the quiet period of solar cycle 24 (year 2017). In fact, the damage of power system operation might lead to the malfunction of the transformer, which is the main component of the power system. Previously, the cause of the damage has been identified in the long-term investigation, where it drives from the space weather effect so-called (GIC). In this work, the quiet period has been selected by respecting the value of K-Planetary index (Kp) must be less than 3 extracted from OMNIWeb data source. The main objective of the current work is to investigate the behavior of the GIC amplitude at Malaysia region as well as to identify the parameter (ionospheric current and magnetospheric current) that contribute significantly towards the GIC activity at Malaysia region. The type of analysis was carried out using the data of geomagnetic field by extracting the time derivative of the horizontal component (dH/dt) as the indicator for GIC activity. The geomagnetic data was obtained from the MAGDAS observatories at Langkawi (LKW), Perak (PER), and Johor (JOH) stations. Subsequently, the dH/dt value is less than 30 nT/min represent no GIC activity occurred during that particular date for all three stations. However, the results revealed that the ionospheric current, DP2 corresponds well to the dH/dt amplitude. Plus, the latitudinal correlation gave the best representation of the control factor of GIC activity.

    DOI: 10.1109/ICSEngT.2018.8606390

  • Variation of equatorial electrojet current profiles over Solar Phases Reviewed

    W. N.I. Ismail, N. S.A. Hamid, M. Abdullah, N. H.M. Shukur, A. Yoshikawa

    ASM Science Journal   12 ( Special Issue 2 )   125 - 133   2019.1

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    Equatorial electrojet (EEJ) current is an intense eastward electric current flowing at about 100- 120km altitude within ±3° latitude in E region of the equatorial ionosphere. This study reported dependence of EEJ longitudinal profile on the three phases of solar cycle 24 (SC-24). The analysis was carried out using EUEL index, calculated from the northward H component of geomagnetic field. This work utilised data from various ground-based magnetometer networks such as MAGDAS, INTERMAGNET and IIG. The results of this study showed that the highest and lowest value of EEJ longitudinal profiles varies with solar phases. The nature of the longitudinal disparity in the EEJ strength indicates that it is strongest in American sector and lowest in African sector during solar minimum in 2008. However, during solar maximum in 2013 the highest EEJ intensity was recorded in Southeast Asian sector. On the other hand, the lowest value of EEJ current was recorded in African sector in 2008 which was found to be shifting to Indian sector started in 2011. In addition, we discovered the transition point of the highest value of EEJ started in 2012, while the transition point of minimum value EEJ started in 2010.

  • Assessment of the Geomagnetically Induced Current (GIC) at Low Latitude Region based on MAGDAS Data Reviewed International journal

    NM Anuar, FAM Kasran, M Abbas, MH Jusoh, SAE Ab Rahim, N Abdul Hadi, A Yoshikawa, Z Mohd Radzi

    Journal of Physics: Conference Series   1152 ( 1 )   2019.1

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    The geomagnetically induced current (GICs) impact is no longer concentrated at high latitude region strictly. The objective of this study was to extend the GICs observation conducted at equatorial region using geomagnetic data extracted from magnetometer installed at Langkawi National Observatory (LNO), Malaysia for the long-term analysis involving the solar cycle 24. The observation is now continued with the GICs comparison between LKW stations with five low latitude station which is BCL, PTN, MND, DAW, and TWV obtained from the magnetic data acquisition system (MAGDAS). The assessment of the GICs behavior revealed the possibility of LKW station experiences GICs is high, based on the time derivative of the horizontal component (dH/dt) value. Extend from that, the GICs estimation was successful done by applying the plane wave method as a model to calculate the North-South and the East-West component, Ex and Ey respectively. The equation of the GICs was provided by excluding the topology constant parameters, which is a and bconstant and the value of the underground conductivity for low latitude station. Subsequently, the comparison was limited in years of 2008 – 2014 due to insufficient geomagnetic data. Indeed, the GICs calculation is able to derive the GICs estimation and showed a good agreement with the corresponding value of the time derivative of the horizontal component. However, the accurate current value (A) is able to gain by conducting a direct measurement of the high voltage power transmission system.

    DOI: 10.1088/1742-6596/1152/1/012029

  • Theory, modeling, and integrated studies in the Arase (ERG) project Reviewed

    Kanako Seki, Yoshizumi Miyoshi, Yusuke Ebihara, Yuto Katoh, Takanobu Amano, Shinji Saito, Masafumi Shoji, Aoi Nakamizo, Kunihiro Keika, Tomoaki Hori, Shin ya Nakano, Shigeto Watanabe, Kei Kamiya, Naoko Takahashi, Yoshiharu Omura, Masahito Nose, Mei Ching Fok, Takashi Tanaka, Akimasa Ieda, Akimasa Yoshikawa

    Earth, Planets and Space   70 ( 1 )   70:17 (WEB ONLY)   2018.12

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    Understanding of underlying mechanisms of drastic variations of the near-Earth space (geospace) is one of the current focuses of the magnetospheric physics. The science target of the geospace research project Exploration of energization and Radiation in Geospace (ERG) is to understand the geospace variations with a focus on the relativistic electron acceleration and loss processes. In order to achieve the goal, the ERG project consists of the three parts: the Arase (ERG) satellite, ground-based observations, and theory/modeling/integrated studies. The role of theory/modeling/integrated studies part is to promote relevant theoretical and simulation studies as well as integrated data analysis to combine different kinds of observations and modeling. Here we provide technical reports on simulation and empirical models related to the ERG project together with their roles in the integrated studies of dynamic geospace variations. The simulation and empirical models covered include the radial diffusion model of the radiation belt electrons, GEMSIS-RB and RBW models, CIMI model with global MHD simulation REPPU, GEMSIS-RC model, plasmasphere thermosphere model, self-consistent wave–particle interaction simulations (electron hybrid code and ion hybrid code), the ionospheric electric potential (GEMSIS-POT) model, and SuperDARN electric field models with data assimilation. ERG (Arase) science center tools to support integrated studies with various kinds of data are also briefly introduced.[Figure not available: see fulltext.].

    DOI: 10.1186/s40623-018-0785-9

  • Theory, modeling, and integrated studies in the Arase (ERG) project Reviewed

    Kanako Seki, Yoshizumi Miyoshi, Yusuke Ebihara, Yuto Katoh, Takanobu Amano, Shinji Saito, Masafumi Shoji, Aoi Nakamizo, Kunihiro Keika, Tomoaki Hori, Shin ya Nakano, Shigeto Watanabe, Kei Kamiya, Naoko Takahashi, Yoshiharu Omura, Masahito Nose, Mei Ching Fok, Takashi Tanaka, Akimasa Ieda, Akimasa Yoshikawa

    earth, planets and space   70 ( 1 )   2018.12

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    Understanding of underlying mechanisms of drastic variations of the near-Earth space (geospace) is one of the current focuses of the magnetospheric physics. The science target of the geospace research project Exploration of energization and Radiation in Geospace (ERG) is to understand the geospace variations with a focus on the relativistic electron acceleration and loss processes. In order to achieve the goal, the ERG project consists of the three parts: the Arase (ERG) satellite, ground-based observations, and theory/modeling/integrated studies. The role of theory/modeling/integrated studies part is to promote relevant theoretical and simulation studies as well as integrated data analysis to combine different kinds of observations and modeling. Here we provide technical reports on simulation and empirical models related to the ERG project together with their roles in the integrated studies of dynamic geospace variations. The simulation and empirical models covered include the radial diffusion model of the radiation belt electrons, GEMSIS-RB and RBW models, CIMI model with global MHD simulation REPPU, GEMSIS-RC model, plasmasphere thermosphere model, self-consistent wave–particle interaction simulations (electron hybrid code and ion hybrid code), the ionospheric electric potential (GEMSIS-POT) model, and SuperDARN electric field models with data assimilation. ERG (Arase) science center tools to support integrated studies with various kinds of data are also briefly introduced.[Figure not available: see fulltext.].

    DOI: 10.1186/s40623-018-0785-9

  • Longitudinal Development of Poleward Boundary Intensifications (PBIs) of Auroral Emission Reviewed

    S. Ohtani, T. Motoba, J. W. Gjerloev, J. M. Ruohoniemi, E. F. Donovan, A. Yoshikawa

    Journal of Geophysical Research: Space Physics   123 ( 11 )   9005 - 9021   2018.11

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    We have investigated the longitudinal propagation and extension of the poleward boundary intensifications (PBIs) of auroral emission by examining four events, Events 1–4, which show different spatiotemporal structures. In Event 1 an auroral form extended both eastward and westward immediately following the arrival of a fast polar cap flow and became dynamic as the polar cap flow enhancement continued. The PBI extended 3 hr in local time in a few minutes, which questions the conventional idea that the PBIs are an ionospheric manifestation of distant reconnection. In Events 2 and 3, an auroral form was already dynamic and was collocated with an upward field-aligned current (FAC), which, along with an adjacent downward FAC, formed a longitudinal flow channel confined near the poleward boundary of the auroral oval. Auroral structures propagated in the direction of this longitudinal convection flow. In Event 4, as a transient westward convection flow arrived, a new auroral form developed and extended also westward but noticeably faster than the convection flow, and it faded as it extended. These results suggest that the longitudinal ionospheric convection plays a critical role in the formation and development of the PBIs. They are consistent with a recently proposed idea that the PBIs are an effect of the ionospheric electrostatic polarization, which deflects the enhanced polar cap flow from equatorward to along the auroral oval at its poleward boundary. The contrast between Events 1 and 4 suggests that morphological differences of the PBIs reflect different durations and intensities of the polar cap flow enhancement.

    DOI: 10.1029/2017JA024375

  • Investigation of Unusual Solar Flare Effect on the Global Ionospheric Current System Reviewed

    N. M.N. Annadurai, N. S.A. Hamid, Y. Yamazaki, A. Yoshikawa

    Journal of Geophysical Research: Space Physics   123 ( 10 )   8599 - 8609   2018.10

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    In this paper, we present our investigation of geomagnetic crochets observed following the X-class solar flare events on 9 August 2011 (X6.9) and 24 September 2011 (X1.4). Both events occurred during geomagnetically quiet times (Kp ≤ 3). The analysis of the geomagnetic crochets near the magnetic equator revealed very different responses in the ionospheric currents between these two events. During the 9 August 2011 event, a reduction of the eastward equatorial electrojet was observed in all daytime stations studied, while the daytime eastward equatorial electrojet was observed to enhance during the 24 September 2011 event. A spherical harmonic analysis was applied to the observations from nearly 160 ground stations at middle and low latitudes to derive the equivalent ionospheric current system for the geomagnetic crochets as well as background solar-quiet (Sq) variations for both events. The equivalent current system of the geomagnetic crochets for the 24 September 2011 event showed a similar pattern with the background Sq current system and thus can be attributed to the enhancement of Sq currents. However, the crochet current system for the 9 August 2011 event revealed a different pattern from the background Sq current system in both Northern and Southern Hemispheres. It is suggested that unusual geomagnetic crochets during the 9 August 2011 event may be dominated by the ionospheric currents at D-region altitudes.

    DOI: 10.1029/2018JA025601

  • Changes in Ionospheric Currents System at Southeast Asia Region during Geomagnetic Storm in Solar's Minimum Phase Reviewed

    Hamid Nurul Shazana Abdul, Wen Viksuthorn Ai, Rosli Nur Izzati Mohd, Yoshikawa Akimasa

    SAINS MALAYSIANA   47 ( 8 )   1923 - 1929   2018.8

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    Changes in ionospheric currents system at southeast Asia region during geomagnetic storm in solar's minimum phase
    Equatorial ionospheric current system consists of equatorial electrojet (EEJ) and solar quiet (Sq). EEJ current is a ribbon of current flowing eastwards along the dip equator region. On the other hand, Sq current is a loop of current that flows at the Earth's northern and southern hemispheres in different directions. This study is focusing on analysing the effects of a solar event on the latitudinal profile of the current system, specifically in Southeast Asian region. Data used in this study are geomagnetic data from five magnetometer stations in MAGDAS network which are Muntinlupa (MUT), Cebu (CEB), Davao (DAV), Manado (MND) and Pare Pare (PRP). The EEJ current intensity is known to be highest around noon time between 1000 and 1100 LT during solar minimum and thus this study analyses the current system from 1000 to 1400 LT. The analysis showed that the geomagnetic storm occurred on 23 April 2008, which is caused by coronal mass ejection (CME), gives rises to the currents on that day. This increment is clearly observed on the currents at the southern hemisphere stations, which are MND and PRP. Our analysis also found that this geomagnetic storm gives increment to the current at the non-peak time. Apart from that, the current profile on this day is compared with the current profile from a quiet day on 21 April 2008.

    DOI: 10.17576/jsm-2018-4708-34

  • 磁気嵐期間中のULF波の全球分布:ARASE,地上観測,BATSRUS+CRCMシミュレーションの比較【JST・京大機械翻訳】 Reviewed

    Takahashi Naoko, Seki Kanako, Teramoto Mariko, Fok Mei-Ching, Zheng Yihua, Matsuoka Ayako, Higashio Nana, Shiokawa Kazuo, Baishev Dmitry, Yoshikawa Akimasa, Nagatsuma Tsutomu

    Geophysical Research Letters   45 ( 18 )   9390 - 9397   2018.7

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    Global Distribution of ULF Waves During Magnetic Storms: Comparison of Arase, Ground Observations, and BATSRUS + CRCM Simulation
    During 26–29 March 2017 magnetic storm, the Arase satellite observed typical ultra low frequency (ULF) waves and acceleration of relativistic electrons. We simulate the global distribution of these ULF waves using CRCM with BATSRUS global magnetospheric magnetohydrodynamic model. The simulation can qualitatively reproduce the ULF waves observed by Arase at frequencies of 2–3 mHz. However, the simulated ULF wave power is 1–2 orders of magnitude smaller than the observation. The simulated ULF wave activity has a good correlation with the solar-wind dynamic pressure variation, while the wave activity on the ground is enhanced even during the recovery phase, possibly due to the Kelvin-Helmholtz instability and/or substorms. We also study the 3–6 April 2017 magnetic storm, in which low ULF wave activity and weak acceleration of relativistic electrons are seen. We suggest that the existence of ULF waves plays an important role in accelerating electrons up to relativistic energies.

    DOI: 10.1029/2018GL078857

  • 運動論的Alfven波との結合からの頂部電離層における電子音波の発生:新しい電子エネルギー化機構【JST・京大機械翻訳】 Reviewed

    Shi Run, Ni Binbin, Summers Danny, Liu Huixin, Yoshikawa Akimasa, Zhang Beichen

    Geophysical Research Letters   45 ( 11 )   5299 - 5304   2018.6

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    Generation of Electron Acoustic Waves in the Topside Ionosphere From Coupling With Kinetic Alfven Waves: A New Electron Energization Mechanism
    Results from a new drift kinetic model in the topside ionosphere capture the mode conversion from kinetic Alfven waves to electron acoustic waves. When the kinetic Alfven waves propagate into the transition region, where the electron density of ionospheric origin becomes comparable to that of magnetospheric origin, the steep temperature gradient leads to the mode conversion. The electron acoustic waves are short-lived by dissipating their energy into the electron energization, thus revealing a new type of electron acceleration in the topside ionosphere.

    DOI: 10.1029/2018GL077898

  • Study of the Solar Wind Influence on the Jovian Inner Magnetosphere Using an Ionospheric Potential Solver Reviewed

    Terada K, Tao C, Terada N, Kasaba Y, Kita H, Nakamizo A, Yoshikawa A, Ohtani S, Tsuchiya F, Kagitani M

    Lunar and Planetary Science Conference   49   2018.6

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    Study of the Solar Wind Influence on the Jovian Inner Magnetosphere Using an Ionospheric Potential Solver

  • Anomalous ultra low frequency signals possibly linked with seismic activities in Sumatra, Indonesia Reviewed

    Takla EM, Khashaba A, Zaher M Abdel, Yoshikawa A, Uozumi T

    NRIAG Journal of Astronomy and Geophysics   2018.5

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    Anomalous ultra low frequency signals possibly linked with seismic activities in Sumatra, Indonesia

  • Earth's Ionosphere—Theory and Phenomenology of Cowling Channels Invited Reviewed

    Akimasa Yoshikawa, Ryoichi Fujii

    Electric Currents in Geospace and Beyond   235   427 - 443   2018.4

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    Earth's ionosphere: Theory and phenomenology of cowling channels
    The Cowling channel is a generic name of a current system forming inside a high conductivity band in which a secondary polarization electric field modifies the current flow. The polarization field is excited when a divergent part of Hall current driven by the primary electric field is prevented from flowing out to the magnetosphere as the field-aligned current. The purpose of this chapter is to review the recent development of the Cowling channel model. Recent work provides an extension of the theoretical description of the classical Cowling channel with respect to the following aspects: (1) taking into account the 3D nature of the ionosphere by introducing two current layers at different altitudes, and (2) considering finite length of the Cowling channel by introducing a conductance boundary not only at the meridional borders of the Cowling channel, but also at its zonal boundaries. Using this improved model, we discuss current closure and the energy principle for evolution of the Cowling channel. Energy flow inside the Cowling channel and impact of the polarization effect on Joule dissipation in the more general M-I coupling scheme are also provided. We also clarify how shear Alfvén waves interact to the Cowling channel and their application to the global magnetosphere- ionosphere coupling simulations.

    DOI: 10.1002/9781119324522.ch25

  • The Time Derivative of the Horizontal Geomagnetic Field for the Low Latitude MAGDAS Langkawi Station for the Estimation of Geomagnetically Induced Current Reviewed

    Kasran Farah, Adilah Mohd, Jusoh Mohamad Huzaimy, Yoshikawa Akimasa, Radzi Zahira Mohd

    Space Science and Communication for Sustainability   57 - 71   2018.4

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    The Time Derivative of the Horizontal Geomagnetic Field for the Low Latitude MAGDAS Langkawi Station for the Estimation of Geomagnetically Induced Current

    DOI: 10.1007/978-981-10-6574-3_6

  • 静穏期のマレーシアにおけるGIC評価のための水平地磁気成分の時間微分の推定【JST・京大機械翻訳】

    Anuar Nornabilah Mohd, Kasran Farah Adilah Mohd., Latif Zatul Iffah Abdul, Rahim Siti Amalina Ence Ab, Manut Arif, Jusoh Mohamad Huzaimy, Hadi Normi Abdul, Yoshikawa Akimasa

    IEEE Conference Proceedings   2018 ( ICSET )   118 - 122   2018.4

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    Estimation of Time Derivative of Horizontal Geomagnetic Component for GIC Assesment in Malaysia during Quiet Period
    This paper presents the preliminary observation on the possible Geomagnetic Induced Current (GIC) activities at Malaysia region during the quiet period of solar cycle 24 (year 2017). In fact, the damage of power system operation might lead to the malfunction of the transformer, which is the main component of the power system. Previously, the cause of the damage has been identified in the long-term investigation, where it drives from the space weather effect so-called (GIC). In this work, the quiet period has been selected by respecting the value of K-Planetary index (Kp) must be less than 3 extracted from OMNIWeb data source. The main objective of the current work is to investigate the behavior of the GIC amplitude at Malaysia region as well as to identify the parameter (ionospheric current and magnetospheric current) that contribute significantly towards the GIC activity at Malaysia region. The type of analysis was carried out using the data of geomagnetic field by extracting the time derivative of the horizontal component (dH/dt) as the indicator for GIC activity. The geomagnetic data was obtained from the MAGDAS observatories at Langkawi (LKW), Perak (PER), and Johor (JOH) stations. Subsequently, the dH/dt value is less than 30 nT/min represent no GIC activity occurred during that particular date for all three stations. However, the results revealed that the ionospheric current, DP2 corresponds well to the dH/dt amplitude. Plus, the latitudinal correlation gave the best representation of the control factor of GIC activity.

    DOI: 10.1109/ICSEngT.2018.8606390

  • Observation of ionospheric current during strong solar flare using ground based magnetometer Reviewed

    N. M.N. Annadurai, N. S.A. Hamid, A. Yoshikawa

    Sains Malaysiana   47 ( 3 )   595 - 601   2018.3

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    Solar flare is referring to sun's activity define as sudden intense bright light coming from its surface. It can immediately affect earth's ionosphere system thus perturb any currents flowing in the layer. The activity can be monitored using ground based magnetometer data. Regularly, the event will enhance the ionospheric conductivity thus increase the magnitude of the currents however the opposite effect has been reported recently. There were studies reported that a solar flare is capable to increase current intensity at some location and reduces it at other location. Previous study were focused on solar flare effect at some particular area sector or locally. Therefore, our approach is to analyze solar flare feature and its effect using extensive magnetometer data distribution which involve stations from five sectors. Data are obtained from Magnetic Data Acquisition System/Circum-pan Pacific Magnetometer Network (MAGDAS/CPMN) and solar flare is identified using Geostationary Operational Environmental Satellite 15 (GOES 15) X-ray flux data. Our study discovered a new effect of solar flare which is reduction of current intensity at all magnetic equator data and the proposed factor is existence of counter electrojet current. Apart from that, we also found that this solar flare occurred on geomagnetic storm recovery phase during June solstice in inclining phase of solar cycle.

    DOI: 10.17576/jsm-2018-4703-21

  • Skin Effect of Rotating Magnetic Fields in Liquid Bridge Reviewed International journal

    Yi Zhang, Z. Zeng, L. Yao, Y. Yokota, Y. Kawazoe, and @A. Yoshikawa

    Journal of Magnetics   22 ( 2 )   333 - 343   2018.2

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    DOI: DOI10.4283/ JMAG.2017.22.2.333.

  • Nighttime Pc3 pulsations: MM100 and MAGDAS observations Reviewed

    Nadezda V. Yagova, Balazs Heilig, Vyacheslav A. Pilipenko, Akimasa Yoshikawa, Nataliya S. Nosikova, Kiyohumi Yumoto, Jan Reda

    Earth, Planets and Space   69 ( 1 )   69:61 (WEB ONLY)   2017.12

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    Nighttime Pc3 pulsations: MM100 and MAGDAS observations
    In this paper, we present a statistical and case analysis of nighttime Pc3 pulsations observed from middle to equatorial latitudes during the year 2003. We found two groups of nighttime Pc3 pulsations. Pc3s of the first group are in fact the nightside counterpart of morning Pc3 pulsations with large azimuthal scales slowly attenuating toward midnight. Such night signatures of morning Pc3 waves are observed during the periods of fast solar wind (V > 500 km/s). The second type is the locally generated night Pc3 pulsations. They can be observed under moderate solar wind velocities. Maximal occurrence rates and amplitudes for these pulsations are recorded at middle geomagnetic latitudes near the local magnetic midnight. Probably, they are associated with auroral activations or local non-substorm bursty processes.

    DOI: 10.1186/s40623-017-0647-x

  • Characteristics of Schumann Resonance Parameters at Kuju Station Reviewed

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe, Hiromasa Nozawa, Manabu Shinohara

    E3S Web of Conferences   20   1004   2017.10

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    Characteristics of Schumann Resonance Parameters at Kuju Station
    The ground magnetic field variation in the extremely low frequency (ELF) range has been measured by an induction magnetometer at Kuju, Japan (KUJ; M.Lat. = 23.4 degrees, M. Lon. = 201.0 degrees) since 2003. The first mode of the Schumann resonance (SR) around 8 Hz can be seen at KUJ. The SR in H (horizontal northward component) shows maximum peaks around 08 UT and 15 UT. In the case of D (horizontal eastward component), the SR shows its maximum peak around 08 UT. These peaks are coincident with the enhancement of lightning activity in Africa and Asia. Thus, we found the influence of the lightning activity on the observed SR at KUJ.

    DOI: 10.1051/e3sconf/20172001004

  • Modeling geomagnetic induced currents in Australian power networks Reviewed

    R. A. Marshall, A. Kelly, T. Van Der Walt, A. Honecker, C. Ong, D. Mikkelsen, A. Spierings, G. Ivanovich, A. Yoshikawa

    Space Weather   15 ( 7 )   895 - 916   2017.7

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    Geomagnetic induced currents (GICs) have been considered an issue for high-latitude power networks for some decades. More recently, GICs have been observed and studied in power networks located in lower latitude regions. This paper presents the results of a model aimed at predicting and understanding the impact of geomagnetic storms on power networks in Australia, with particular focus on the Queensland and Tasmanian networks. The model incorporates a “geoelectric field” determined using a plane wave magnetic field incident on a uniform conducting Earth, and the network model developed by Lehtinen and Pirjola (1985). Model results for two intense geomagnetic storms of solar cycle 24 are compared with transformer neutral monitors at three locations within the Queensland network and one location within the Tasmanian network. The model is then used to assess the impacts of the superintense geomagnetic storm of 29–31 October 2003 on the flow of GICs within these networks. The model results show good correlation with the observations with coefficients ranging from 0.73 to 0.96 across the observing sites. For Queensland, modeled GIC magnitudes during the superstorm of 29–31 October 2003 exceed 40 A with the larger GICs occurring in the south-east section of the network. Modeled GICs in Tasmania for the same storm do not exceed 30 A. The larger distance spans and general east-west alignment of the southern section of the Queensland network, in conjunction with some relatively low branch resistance values, result in larger modeled GICs despite Queensland being a lower latitude network than Tasmania.

    DOI: 10.1002/2017SW001613

  • Variations of B0 and B1 with the solar quiet Sq-current system and comparison with IRI-2012 model at Ilorin Reviewed

    S. A. Bello, M. Abdullah, N. S.A. Hamid, A. Yoshikawa, A. O. Olawepo

    Advances in Space Research   60 ( 2 )   307 - 316   2017.7

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    The ionospheric thickness (B0) and shape (B1) are bottomside profile parameters introduced by the International Reference Ionosphere (IRI) model. We have validated these parameters with the latest version of the IRI-2012 model and compared them with the solar quiet of geomagnetic H-component (SqH). The B0, B1 and SqH are calculated from the measurements obtained from digisonde DPS-4 sounder and the Magnetic Data Acquisition System (MAGDAS) magnetometer, respectively at Ilorin (geo latitude 8.50°N, geo longitude 4.68°E, and Magnetic dip 4.1°S) an equatorial station in the African sector. The study was for the year 2010, a year of low solar activity (with 27-day averaged solar index, F10.7 = 80 sfu). The results show that B0 for the entire months was higher during the daytime than during the night time. On the other hand, the magnitude of B1during the daytime period is lower than nighttime values and exhibit oscillatory pattern. By comparing the experimental observations of the profile parameters with the IRI-2012 model prediction, we found that B0 was fairly represented by the IRI model options during the nighttime period while discrepancies exist between the model estimates and the experimental values during the morning till midday. A close agreement exists between the observed B1 values and IRI model options. We observed a positive and significant correlation coefficient between B0 and SqH indicating a plausible relationship between these parameters while a weak and negative correlation coefficient between B1 and SqH was observed. We concluded that the difference in the relationship of SqH and the profile parameters B0 and B1 observed can be attributed to their sensitivity to the electric field which is responsible for the E × B drift which in turn modulate the height of the F2.

    DOI: 10.1016/j.asr.2017.02.003

  • Longitudinal Variation of EEJ Current during Different Phases of Solar Cycle Reviewed

    W. N.I. Ismail, N. S.A. Hamid, M. Abdullah, A. Yoshikawa, T. Uozumi

    Journal of Physics: Conference Series   852 ( 1 )   12019   2017.6

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    The equatorial electrojet (EEJ) is an eastward current flow around the dip equator in E-region of the ionosphere within the range of 90 to 120 km altitude. The longitudinal variation of EEJ was studied using the ground-based measurement from six different longitudinal sectors. The ground magnetometer data were provided by magnetometer networks such as those from Magnetic Data Acquisition System (MAGDAS) /Circum-pan Pacific Magnetometer Network (CPMN), Indian Institute of Geomagnetism (IIG) and International Real-time Magnetic Observatory Network (INTERMAGNET). The EUEL index used in this study was calculated from geomagnetic northward H component. The H-component was normalized to the dip equator using the CM4 model. This study present results of the longitudinal variation of EEJ during the three phases of solar cycle 24: solar minimum (2008), inclination phase (2011) and solar maximum (2014). Results show that EEJ current is higher in the American sector and lowest between African and Indian sector in 2008 and 2011. On the other hand, during the year of solar maximum, this current component is comparable in American and Southeast Asian sector.

    DOI: 10.1088/1742-6596/852/1/012019

  • Peak time of equatorial electrojet from different longitude sectors during fall solar minimum Reviewed

    N. S.A. Hamid, H. Liu, T. Uozumi, A. Yoshikawa, N. M.N. Annadurai

    Journal of Physics: Conference Series   852 ( 1 )   12015   2017.6

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    Equatorial electrojet is an eastward flowing current at about ±3° dip equator. This current intensity is always higher during noontime as it is greatly influenced by the ionization of Earth ionosphere. Apart from that, previous study had shown that EEJ current varies with longitude and latitude as well as solar cycle. The aim of this study is to investigate the peak time of EEJ current at different longitude sectors using simultaneous data in 2009. By eliminating Sq current contribution and normalizing ground-based data from MAGDAS/CPMN, IIG and WDC network, we managed to reach our purpose and gain reliable output. We found out that EEJ is strongest in South American sector. Our results show that the peak EEJ during fall solar minimum is observed at 11 LT for South American, Indian and Southeast Asian sector but it is 1 hr earlier in African sector.

    DOI: 10.1088/1742-6596/852/1/012015

  • Contribution of storm time substorms to the prompt electric field disturbances in the equatorial ionosphere Reviewed

    Debrup Hui, D. Chakrabarty, R. Sekar, G. D. Reeves, A. Yoshikawa, K. Shiokawa

    Journal of Geophysical Research: Space Physics   122 ( 5 )   5568 - 5578   2017.5

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    This study tries to bring out the fact that storm time substorms can compete and at times significantly contribute to the geomagnetically disturbed time prompt penetration electric field effects on low and equatorial latitudes. Observations of unusual equatorial plasma drift data from Jicamarca Unattended Long-term Investigations of the Ionosphere and Atmosphere during two space weather events show that substorms can induce both eastward and westward penetration electric fields under steady southward interplanetary magnetic field (IMF Bz) conditions. During the first event on 2 January 2005, the enhancement of the daytime eastward electric field over Jicamarca due to substorm is found to be comparable with the Sq and interplanetary electric field (IEFy) generated electric fields combined. During the second event on 19 August 2006, the substorm is seen to weaken the daytime eastward field thereby inducing a westward field in spite of the absence of northward turning of IMF Bz (overshielding). The westward electric field perturbation in the absence of any overshielding events is observationally sparse and contrary to the earlier results. Further, the substorm-induced field is found to be strong enough to compete or almost nullify the effects of storm time IEFy fields. This study also shows quantitatively that at times substorm contribution to the disturbed time prompt electric fields can be significant and thus should be taken into consideration in evaluating penetration events over low latitudes.

    DOI: 10.1002/2016JA023754

  • Analysis of Magnetic Field Variations Produced by Equatorial Electro-Jets Reviewed International journal

    E López, F Aldás, @A Yoshikawa

    arXiv:1507.04509v1   2017.5

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  • Longitudinal variation of equatorial electrojet and the occurrence of its counter electrojet Reviewed

    A. Babatunde Rabiu, Olanike Olufunmilayo Folarin, Teiji Uozumi, Nurul Shazana Abdul Hamid, Akimasa Yoshikawa

    Annales Geophysicae   35 ( 3 )   535 - 545   2017.4

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    Longitudinal variation of equatorial electrojet and the occurrence of its counter electrojet
    We examined the longitudinal variability of the equatorial electrojet (EEJ) and the occurrence of its counter electrojet (CEJ) using the available records of the horizontal component H of the geomagnetic field simultaneously recorded in the year 2009 (mean annual sunspot number Rz Combining double low line 3.1) along the magnetic equator in the South American, African, and Philippine sectors. Our results indicate that the EEJ undergoes variability from one longitudinal representative station to another, with the strongest EEJ of about 192.5nT at the South American axis at Huancayo and a minimum peak of 40.7nT at Ilorin in western Africa. Obtained longitudinal inequality in the EEJ was explicable in terms of the effects of local winds, dynamics of migratory tides, propagating diurnal tide, and meridional winds. The African stations of Ilorin and Addis Ababa registered the greatest &#37; of CEJ occurrence. Huancayo in South America, with the strongest electrojet strength, was found to have the least occurrence of the CEJ. It is suggested that activities that support strong EEJ inhibits the occurrence of the CEJ. Percentage of occurrence of the CEJ varied with seasons across the longitudes. The order of seasonal variation of morning occurrence does not tally with the evening occurrence order at any station. A semiannual equinoctial maximum in percentage of morning occurrence of the CEJ was obtained at Huancayo and Addis Ababa. Only Addis Ababa recorded equal equinoctial maxima in percentage of evening occurrence of the CEJ. The seasonal distribution of the occurrences of the CEJ at different time regimes implies a seasonal variability of causative mechanisms responsible for the occurrence of the CEJ.

    DOI: 10.5194/angeo-35-535-2017

  • Meridional movement of northern and southern equatorial ionization anomaly crests in the East-Asian sector during 2002-2003 SSW Reviewed

    Mo XiaoHua, Zhang DongHe, Larisa Goncharenko, Zhang ShunRong, Hao YongQiang, Xiao Zuo, Pei JiaZheng, Akimasa Yoshikawa, Chau HaDuyen

    SCIENCE CHINA-EARTH SCIENCES   60 ( 4 )   776 - 785   2017.4

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    The present paper investigates the asymmetrical variability of the location of the north and the south equatorial ionization anomaly (EIA) crests in the East-Asian sector, along with their association with simultaneous observations of equatorial electrojet (EEJ) strength, geomagnetic activity index, and solar flux index during the 2002-2003 sudden stratospheric warming (SSW) event. Analysis of these observations indicates the existence of a large-scale quasi 16-day periodic meridional movement in both EIA crests, and also reveals a strong correlation between the quasi 16-day oscillation in geomagnetic latitudes of the EIA crest and EEJ strength. The latitude of the northern/southern EIA crest and the EEJ strength indicate that obvious synchronous periodic oscillations were in-phase in the northern and southern hemisphere when the SSW occurred. In addition, it is also found that both the EIA crest location and amplitude of the periodic movement of the EIA locations exhibit hemispheric asymmetry. The amplitude of the periodic movement of the EIA location in the southern hemisphere is larger than that of the northern hemisphere, and the southern EIA crest is further off from the equator than the north one. Understanding these asymmetries requires a combination of mechanisms that involve at least trans-equator meridional winds and the position of a sub-solar point; however, potential disturbances in neutral winds associated with the SSW may additionally complicate the equatorial ionospheric dynamics.

    DOI: 10.1007/s11430-016-0096-y

  • Longitudinal variation of equatorial electrojet and the occurrence of its counter electrojet Reviewed

    A. Babatunde Rabiu, Olanike Olufunmilayo Folarin, Teiji Uozumi, Nurul Shazana Abdul Hamid, @Akimasa Yoshikawa

    Annales Geophysicae   35 ( 3 )   535 - 545   2017.4

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    We examined the longitudinal variability of the equatorial electrojet (EEJ) and the occurrence of its counter electrojet (CEJ) using the available records of the horizontal component H of the geomagnetic field simultaneously recorded in the year 2009 (mean annual sunspot number Rz Combining double low line 3.1) along the magnetic equator in the South American, African, and Philippine sectors. Our results indicate that the EEJ undergoes variability from one longitudinal representative station to another, with the strongest EEJ of about 192.5nT at the South American axis at Huancayo and a minimum peak of 40.7nT at Ilorin in western Africa. Obtained longitudinal inequality in the EEJ was explicable in terms of the effects of local winds, dynamics of migratory tides, propagating diurnal tide, and meridional winds. The African stations of Ilorin and Addis Ababa registered the greatest % of CEJ occurrence. Huancayo in South America, with the strongest electrojet strength, was found to have the least occurrence of the CEJ. It is suggested that activities that support strong EEJ inhibits the occurrence of the CEJ. Percentage of occurrence of the CEJ varied with seasons across the longitudes. The order of seasonal variation of morning occurrence does not tally with the evening occurrence order at any station. A semiannual equinoctial maximum in percentage of morning occurrence of the CEJ was obtained at Huancayo and Addis Ababa. Only Addis Ababa recorded equal equinoctial maxima in percentage of evening occurrence of the CEJ. The seasonal distribution of the occurrences of the CEJ at different time regimes implies a seasonal variability of causative mechanisms responsible for the occurrence of the CEJ.

    DOI: 10.5194/angeo-35-535-2017

  • Meridional movement of northern and southern equatorial ionization anomaly crests in the East-Asian sector during 2002窶_003 SSW Reviewed

    Mo XiaoHua, Zhang DongHe, Goncharenko Larisa, Zhang ShunRong, Hao YongQiang, Xiao Zuo, Pei JiaZheng, Yoshikawa Akimasa, Chau HaDuyen

    Science China Earth Sciences   60 ( 4 )   776 - 785   2017.4

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    Meridional movement of northern and southern equatorial ionization anomaly crests in the East-Asian sector during 2002–2003 SSW
    The present paper investigates the asymmetrical variability of the location of the north and the south equatorial ionization anomaly (EIA) crests in the East-Asian sector, along with their association with simultaneous observations of equatorial electrojet (EEJ) strength, geomagnetic activity index, and solar flux index during the 2002–2003 sudden stratospheric warming (SSW) event. Analysis of these observations indicates the existence of a large-scale quasi 16-day periodic meridional movement in both EIA crests, and also reveals a strong correlation between the quasi 16-day oscillation in geomagnetic latitudes of the EIA crest and EEJ strength. The latitude of the northern/southern EIA crest and the EEJ strength indicate that obvious synchronous periodic oscillations were in-phase in the northern and southern hemisphere when the SSW occurred. In addition, it is also found that both the EIA crest location and amplitude of the periodic movement of the EIA locations exhibit hemispheric asymmetry. The amplitude of the periodic movement of the EIA location in the southern hemisphere is larger than that of the northern hemisphere, and the southern EIA crest is further off from the equator than the north one. Understanding these asymmetries requires a combination of mechanisms that involve at least trans-equator meridional winds and the position of a sub-solar point; however, potential disturbances in neutral winds associated with the SSW may additionally complicate the equatorial ionospheric dynamics.

    DOI: 10.1007/s11430-016-0096-y

  • High-latitude Pi2 pulsations associated with kink-like neutral sheet oscillations Reviewed

    G. Q. Wang, M. Volwerk, T. L. Zhang, D. Schmid, A. Yoshikawa

    Journal of Geophysical Research: Space Physics   122 ( 3 )   2889 - 2899   2017.3

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    A kink-like neutral sheet oscillation event observed by Cluster between 1436 and 1445 UT on 15 October 2004 has been investigated. The oscillations with periods between 40 and 60 s, observed at (−13.1, 8.7, −0.5) RE, are dominant in BX and BY. And they propagate mainly duskward with a velocity of (86, 147, 46) km/s. Their periods and velocity can be explained by the magnetic double-gradient instability. These oscillations are accompanied by strong field-aligned currents (FACs), which prefer to occur near the strongly tilted current sheet, and local maximum FAC tends to occur near the neutral sheet. The FACs show one-to-one correlated with a high-latitude Pi2 pulsation event recorded by KTN and TIK stations with a delay time of ~60 and 90 s, respectively. Both the Pi2 and oscillations propagate westward with a comparative conjunctive speed. These findings suggest a strong relation between the FACs and Pi2, and we infer that the Pi2 is caused by the FACs. The periods of the FACs are modulated by the oscillations but not exactly equal, which is one possible reason that the period of the Pi2 caused by the FACs could be different from the oscillations. We speculate that a current circuit between the plasma sheet and ionosphere can be formed during strongly tilted current sheet, and successive tilted current sheet could generate quasiperiodic multiple FAC systems, which can generate high-latitude Pi2 pulsations and control their periods.

    DOI: 10.1002/2016JA023370

  • High-latitude Pi2 pulsations associated with kink-like neutral sheet oscillations

    G. Q. Wang, M. Volwerk, T. L. Zhang, D. Schmid, A. Yoshikawa

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   122 ( 3 )   2889 - 2899   2017.3

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    A kink-like neutral sheet oscillation event observed by Cluster between 1436 and 1445 UT on 15 October 2004 has been investigated. The oscillations with periods between 40 and 60s, observed at (-13.1, 8.7, -0.5) R-E, are dominant in B-X and B-Y. And they propagate mainly duskward with a velocity of (86, 147, 46)km/s. Their periods and velocity can be explained by the magnetic double-gradient instability. These oscillations are accompanied by strong field-aligned currents (FACs), which prefer to occur near the strongly tilted current sheet, and local maximum FAC tends to occur near the neutral sheet. The FACs show one-to-one correlated with a high-latitude Pi2 pulsation event recorded by KTN and TIK stations with a delay time of -60 and 90s, respectively. Both the Pi2 and oscillations propagate westward with a comparative conjunctive speed. These findings suggest a strong relation between the FACs and Pi2, and we infer that the Pi2 is caused by the FACs. The periods of the FACs are modulated by the oscillations but not exactly equal, which is one possible reason that the period of the Pi2 caused by the FACs could be different from the oscillations. We speculate that a current circuit between the plasma sheet and ionosphere can be formed during strongly tilted current sheet, and successive tilted current sheet could generate quasiperiodic multiple FAC systems, which can generate high-latitude Pi2 pulsations and control their periods.

    DOI: 10.1002/2016JA023370

  • First geomagnetic observation at sabah, malaysia by using MAGDAS array Reviewed International journal

    Siti Nurbaiti Ibrahim, Mohamad Huzaimy Jusoh, Ahmad Asari Sulaiman, Siti Noor Aisyah Ahmad, Mohd Zul Hilmey Makmud, Baba Musta, Mardina Abdullah, Mhd Fairos Asillam, Nyanasegari Bhoo Pathy, Mohd Helmy Hashim, @Akimasa Yoshikawa

    International Journal of Simulation: Systems, Science and Technology   17 ( 41 )   30.1 - 30.8   2017.2

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    MAGDAS (Magnetic Data Acquisition System) is a magnetometer initiated by Kyushu University used to study space weather. The latest of real-time Magnetic Data Acquisition System of Circum-pan Pacific Magnetometer Network was successfully installed at University Malaysia Sabah (UMS) Sabah, Malaysia by International Center for Space Weather Science and Education, ICSWSE, Kyushu University, Japan. This is the second magnetometer under MAGDAS after Langkawi station (LKW) (geographic latitude and longitude: 6.30º, 99.78º and geomagnetic latitude and longitude: -2.32º, 171.29º). This paper reports on first analysis of geomagnetic observation of MAGDAS at Sabah station. The geomagnetic components: H, D, Z and total F obtained from MAGDAS’s magnetometer are presented. The diurnal variation of geomagnetic elements during initial measurement at Sabah indicates a good variation pattern. The validation of amplitude variation with the nearest station also significantly relative.

    DOI: 10.5013/IJSSST.a.17.41.30

  • Longitudinal Profile of the Equatorial Electrojet Current and Its Dependence on Solar Activity Reviewed

    Nurul Shazana Abdul Hamid, Wan Nur Izzaty Ismail, Akimasa Yoshikawa

    Advanced Science Letters   23 ( 2 )   1357 - 1360   2017.2

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    Longitudinal profile of the equatorial electrojet current and its dependence on solar activity
    The equatorial electrojet (EEJ) is a strong eastward ionosphere current flowing in a narrow band along dip equator. It is flowing eastward in the dayside of equatorial E region of about 600 km wide and within 90 to 130 km altitude. The objectives of this research is to study the variations Equatorial Electrojet (EEJ) current measured from ground_based magnetometer. The data were provided by magnetometer network such as Magnetic Data Acquisition System (MAGDAS)/Circum-pan Pacific Magnetometer Network (CPMN), Indian Institute of Geomagnetism (IIG), International Real-time Magnetic Observatory Network (INTERMAGNET). We also request the data from the single observation station such as Fuquene (FUQ). The analysis is carried out using the EUEL index and normalization technique is applied to yield better results with the aids of CM4 current model. This involves fourteen stations in South America, African, Indian and Southeast Asian sectors. The analysis done are including longitudinal and solar activity dependence where the years revolves are 2008 and 2011. These two years represents the minimum phases of solar activity (2008) and inclining phases of solar activity (2011). The results obtained show that EEJ varies with longitudes and solar activity. EEJ current is found to be highest at the American sector and lowest between African and Indian sector. This current is also highest in inclination phase during 2011 compared to 2008 (solar minimum).

    DOI: 10.1166/asl.2017.8372

  • Latitudinal Variation of Ionospheric Currents in Southeast Asian Sector Reviewed

    Nurul Shazana Abdul Hamid, Wan Nur Izzaty Ismail, Akimasa Yoshikawa

    Advanced Science Letters   23 ( 2 )   1444 - 1447   2017.2

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    Latitudinal variation of ionospheric currents in Southeast Asian sector
    The equatorial electrojet (EEJ) is a current system caused by the enhanced ionospheric conductivity near the dayside magnetic dip equator. In this study, we attempt to obtain the latitudinal profile of Sq and total current component (EEJ+Sq) and consequently attain the EEJ latitudinal variation. Analysis is carried on using magnetic data recorded at six stations in Southeast Asian sector. The data used are equatorial electrojet index, EUEL, which were calculated from geomagnetic northward, H, component on geomagnetically quiet days. We further compared latitudinal profile of Sq and total current during solar minimum (2008) and solar maximum (2014) in order to study their solar cycle dependence. Furthermore, we examined the EEJ circuit for both solar activity period. Result shows that as the EEJ strength increase with solar activity, it contribute to higher increase in total current during 2014, and consequently contribute to significant difference in the total current latitudinal profile during 2008 and 2014. On the other hand, the EEJ latitudinal variation illustrates the current circuit where the reverse current was observed to start on the flanks of dip equator at about 5° and terminate at less than 10° latitude in both hemispheres.

    DOI: 10.1166/asl.2017.8358

  • Analysis of Magnetic Field Variations Produced by Equatorial Electro-Jets Reviewed

    Ericson López, Franklin Aldás, Akimasa Yoshikawa

    Proceedings of the International Astronomical Union   13 ( S335 )   125 - 127   2017.1

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    The Equatorial Electrojet (EEJ) is a narrow band of electrons flowing from east to west at daytime at low latitudes. The electron current produces a magnetic field variation that can be measured at different latitudes. In this work, we have used the data analysis in order to quantify the solar and lunar contributions to those variations and study the morphology of the EEJ current.

    DOI: 10.1017/S1743921318000662

  • Evolution of the current system during solar wind pressure pulses based on aurora and magnetometer observations Reviewed

    Yukitoshi Nishimura, Takashi Kikuchi, Yusuke Ebihara, Akimasa Yoshikawa, Shun Imajo, Wen Li, Hisashi Utada

    Earth, Planets and Space   68 ( 1 )   144   2016.12

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    We investigated evolution of ionospheric currents during sudden commencements using a ground magnetometer network in conjunction with an all-sky imager, which has the advantage of locating field-aligned currents much more accurately than ground magnetometers. Preliminary (PI) and main (MI) impulse currents showed two-cell patterns propagating antisunward, particularly during a southward interplanetary magnetic field (IMF). Although this overall pattern is consistent with the Araki (solar wind sources of magnetospheric ultra-low-frequency waves. Geophysical monograph series, vol 81. AGU, Washington, DC, pp 183-200, 1994. doi:10.1029/GM081p0183) model, we found several interesting features. The PI and MI currents in some events were highly asymmetric with respect to the noon- midnight meridian; the post-noon sector did not show any notable PI signal, but only had an MI starting earlier than the pre-noon MI. Not only equivalent currents but also aurora and equatorial magnetometer data supported the much weaker PI response. We suggest that interplanetary shocks impacting away from the subsolar point caused the asymmetric current pattern. Additionally, even when PI currents form in both pre- and post-noon sectors, they can initiate and disappear at different timings. The PI currents did not immediately disappear but coexisted with the MI currents for the first few minutes of the MI. During a southward IMF, the MI currents formed equatorward of a preexisting DP-2, indicating that the MI currents are a separate structure from a preexisting DP-2. In contrast, the MI currents under a northward IMF were essentially an intensification of a preexisting DP-2. The magnetometer and imager combination has been shown to be a powerful means for tracing evolution of ionospheric currents, and we showed various types of ionospheric responses under different upstream conditions.

    DOI: 10.1186/s40623-016-0517-y

  • Solar terminator effects on middle- to low-latitude Pi2 pulsations Reviewed International journal

    #Shun Imajo, @Akimasa Yoshikawa, @Teiji Uozumi, Shinichi Ohtani, Aoi Nakamizo, Sodnomsambuu Demberel, Boris Mikhailovich Shevtsov

    Earth, Planets and Space   68 ( 1 )   2016.12

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    To clarify the effect of the dawn and dusk terminators on Pi2 pulsations, we statistically analyzed the longitudinal phase and amplitude structures of Pi2 pulsations at middle- to low-latitude stations (GMLat = 5.30°-46.18°) around both the dawn and dusk terminators. Although the H (north-south) component Pi2s were affected by neither the local time (LT) nor the terminator location (at 100 km altitude in the highly conducting E region), some features of the D (east-west) component Pi2s depended on the location of the terminator rather than the LT. The phase reversal of the D component occurred 0.5-1 h after sunrise and 1-2 h before sunset. These phase reversals can be attributed to a change in the contributing currents from field-aligned currents (FACs) on the nightside to the meridional ionospheric currents on the sunlit side of the terminator, and vice versa. The phase reversal of the dawn terminator was more frequent than that of the dusk terminator. The D-to-H amplitude ratio on the dawn side began to increase at sunrise, reaching a peak approximately 2 h after sunrise (the sunward side of the phase reversal region), whereas the ratio on the dusk side reached a peak at sunset (the antisunward side). The dawn-dusk asymmetric features suggest that the magnetic contribution of the nightside FAC relative to the meridional ionospheric current on the dusk side is stronger than that on the dawn side, indicating that the center of Pi2-associated FACs, which probably corresponds to the Pi2 energy source, tends to be shifted duskward on average. Different features and weak sunrise/sunset dependences at the middle-latitude station (Paratunka, GMLat = 46.18°) can be attributed to the larger annual variation in the sunrise/sunset time and a stronger magnetic effect because of closeness from FACs. The D-to-H amplitude ratio decreased with decreasing latitude, suggesting that the azimuthal magnetic field produced by the FACs in darkness and the meridional ionospheric current in sunlight also decreased with decreasing latitude.

    DOI: 10.1186/s40623-016-0514-1

  • The initiation of the poleward boundary intensification of auroral emission by fast polar cap flows: A new interpretation based on ionospheric polarization Reviewed

    S. Ohtani, A. Yoshikawa

    Journal of Geophysical Research: Space Physics   121 ( 11 )   10,910 - 10,928   2016.11

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    The auroral intensification at the poleward boundary of the auroral oval is often considered to be the ionospheric manifestation of the distant reconnection. In the present study, however, we propose that the poleward boundary intensifications (PBIs) are initiated by ionospheric polarization due to fast polar cap flows, which are known to be well correlated with PBIs. The current continuity at the ionosphere can be described in two different ways, that is, the reflection of an Alfvén wave and the closure of Pedersen and Hall currents with field-aligned currents (FACs). The required consistency between the two approaches sets a framework for modeling the ionospheric polarization, and we numerically test the aforementioned idea focusing on an induced upward FAC as indicative of PBIs. The results show that in case the polar cap flow channel approaches the auroral oval perpendicularly from poleward, (i) upward and downward FACs are induced at the poleward boundary to the west and east of the longitudinal center of the flow channel, respectively; (ii) those induced FACs extend much wider in longitude than the flow channel; (iii) the peak densities of those induced FACs are significantly larger than those of the incident FACs; (iv) those induced FACs are distributed almost symmetrically in longitude, indicating that the Pedersen polarization dominates the Hall polarization; and (v) if the polar cap flow inclined dawnward (duskward), an upward (downward) FAC is induced first. These results are consistent with the reported characteristics of PBIs, which are rather difficult to explain otherwise.

    DOI: 10.1002/2016JA023143

  • Propagation of ULF waves from the upstream region to the midnight sector of the inner magnetosphere Reviewed International journal

    Kazue Takahashi, Michael D. Hartinger, David M. Malaspina, Charles W. Smith, Kiyokazu Koga, Howard J. Singer, Dennis Frühauff, Dmitry G. Baishev, Alexey V. Moiseev, @Akimasa Yoshikawa

    Journal of Geophysical Research   121 ( 9 )   8428 - 8447   2016.9

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    Ultralow frequency (ULF) waves generated in the ion foreshock are a well-known source of Pc3-Pc4 waves (7–100 mHz) observed in the dayside magnetosphere. We use data acquired on 10 April 2013 by multiple spacecraft to demonstrate that ULF waves of upstream origin can propagate to the midnight sector of the inner magnetosphere. At 1130–1730 UT on the selected day, the two Van Allen Probes spacecraft and the geostationary ETS-VIII satellite detected compressional 20 to 40 mHz magnetic field oscillations between L ∼ 4 and L ∼ 7 in the midnight sector, along with other spacecraft located closer to noon. Upstream origin of the oscillations is concluded from the wave frequency that matches a theoretical model, globally coherent amplitude modulation, and duskward propagation that is consistent with expected entry of the upstream wave energy through the dawnside flank under the observed interplanetary magnetic field. The oscillations are attributed to magnetohydrodynamic fast-mode waves based on their propagation velocity of ∼300 km/s and the relationship between the electric and magnetic field perturbations. The magnitude of the azimuthal wave number is estimated to be ∼30. There is no evidence that the oscillations propagated to the ground in the midnight sector.

    DOI: 10.1002/2016JA022958

  • Solar quiet current response in the African sector due to a 2009 sudden stratospheric warming event Reviewed

    O. S. Bolaji, E. O. Oyeyemi, O. P. Owolabi, Y. Yamazaki, A. B. Rabiu, D. Okoh, A. Fujimoto, C. Amory-Mazaudier, G. K. Seemala, A. Yoshikawa, O. K. Onanuga

    Journal of Geophysical Research: Space Physics   121 ( 8 )   8055 - 8065   2016.8

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    We present solar quiet (Sq) variation of the horizontal (H) magnetic field intensity deduced from Magnetic Data Acquisition System (MAGDAS) records over Africa during an unusual strong and prolonged 2009 sudden stratospheric warming (SSW) event. A reduction in the SqH magnitude that enveloped the geomagnetic latitudes between 21.13°N (Fayum FYM) in Egypt and 39.51°S (Durban DRB) in South Africa was observed, while the stratospheric polar temperature was increasing and got strengthened when the stratospheric temperature reached its maximum. Another novel feature associated with the hemispheric reduction is the reversal in the north-south asymmetry of the SqH, which is indicative of higher SqH magnitude in the Northern Hemisphere compared to the Southern Hemisphere during SSW peak phase. The reversal of the equatorial electrojet (EEJ) or the counter electrojet (CEJ) was observed after the polar stratospheric temperature reached its maximum. The effect of additional currents associated with CEJ was observed in the Southern Hemisphere at middle latitude. Similar changes were observed in the EEJ at the South America, Pacific Ocean, and Central Asia sectors. The effect of the SSW is largest in the South American sector and smallest in the Central Asian sector.

    DOI: 10.1002/2016JA022857

  • Initial deflection of middle-latitude Pi2 pulsations in the premidnight sector: Remote detection of oscillatory upward field-aligned current at substorm onset

    Teiji Uozumi, A. Yoshikawa, S. Ohtani, S. Imajo, D. G. Baishev, A. V. Moiseev, K. Yumoto

    Journal of Geophysical Research: Space Physics   121 ( 7 )   6324 - 6340   2016.7

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    In this study, we examined middle- and low-latitude Pi2 events to address the following two issues regarding the well-known substorm current wedge (SCW) model for Pi2 pulsations: (1) the center of the SCW, which is estimated using the Pi2 polarization pattern, is not always collocated with that determined using the magnetic bay pattern; and (2) although ideally Pi2 hodograms would be linear, they tend to become circular. In this study, auroral breakup events were identified from Polar Ultraviolet Imager data. We assumed that the ionospheric footprint of the upward field-aligned current (FAC) in each event was located at the position of the auroral breakup and subsequently calculated the signature of the magnetic variation at the middle-latitude station Zyryanka (ZYK; GMLAT = 59.6°) that was generated by the upward FAC. In order to examine the magnetic effects of the upward FAC, we selected Pi2 events that were observed when ZYK was located on the duskward side of the auroral breakup location. A total of 112 events were selected and analyzed in this study. It was found that the location of the upward FAC of the SCW could be estimated more accurately by using an azimuth value predicted based on the initial deflection of the middle-latitude Pi2. Our results suggest that the circular shapes of Pi2 polarization curves are caused by the delayed driven Alfvénic waves that are superimposed on the geomagnetic northward components of SCW oscillations.

    DOI: 10.1002/2015JA021698

  • 複数のサブストーム発症時の深夜後セクターにおいて観察された東方に拡大するオーロラサージ Reviewed

    TANAKA Yoshimasa, TANAKA Yoshimasa, OGAWA Yasunobu, OGAWA Yasunobu, KADOKURA Akira, KADOKURA Akira, PARTAMIES Noora, PARTAMIES Noora, WHITER Daniel, ENELL Carl-Fredrik, BRAENDSTROEM Urban, SERGIENKO Tima, GUSTAVSSON Bjoern, KOZLOVSKY Alexander, MIYAOKA Hiroshi, MIYAOKA Hiroshi, YOSHIKAWA Akimasa

    Earth, Planets and Space (Web)   67 ( Nov )   182   2016.7

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    Eastward-expanding auroral surges observed in the post-midnight sector during a multiple-onset substorm
    We present three eastward-expanding auroral surge (EEAS) events that were
    observed intermittently at intervals of about 15 min in the post-midnight
    sector (01:55-02:40 MLT) by all-sky imagers and magnetometers in northern
    Europe. It was deduced that each surge occurred just after each onset of a
    multiple-onset substorm, which was small-scale and did not clearly expand
    westward, because they were observed almost simultaneously with Pi 2 pulsations
    at the magnetic equator and magnetic bay variations at middle-to-high latitudes
    associated with the DP-1 current system. The EEASs showed similar properties to
    omega bands or torches reported in previous studies, such as recurrence
    intervals of about 15 min, concurrence with magnetic pulsations with amplitudes
    of several tens of nanotesla, horizontal scales of 300-400 km, and occurrence
    of a pulsating aurora in a diffuse aurora after the passage of the EEASs.
    Furthermore, the EEASs showed similar temporal evolution to the omega bands,
    during which eastward-propagating auroral streamers occurred simultaneously in
    the poleward region, followed by the formation of north-south-aligned auroras,
    which eventually connected with the EEASs. Thus, we speculate that EEASs may be
    related to the generation process of omega bands. (Continued)

    DOI: 10.1186/s40623-015-0350-8

  • Initial deflection of middle-latitude Pi2 pulsations in the premidnight sector: Remote detection of oscillatory upward field-aligned current at substorm onset Reviewed

    Teiji Uozumi, A. Yoshikawa, S. Ohtani, S. Imajo, D. G. Baishev, A. V. Moiseev, K. Yumoto

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   121 ( 7 )   6324 - 6340   2016.7

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    In this study, we examined middle- and low-latitude Pi2 events to address the following two issues regarding the well-known substorm current wedge (SCW) model for Pi2 pulsations: (1) the center of the SCW, which is estimated using the Pi2 polarization pattern, is not always collocated with that determined using the magnetic bay pattern; and (2) although ideally Pi2 hodograms would be linear, they tend to become circular. In this study, auroral breakup events were identified from Polar Ultraviolet Imager data. We assumed that the ionospheric footprint of the upward field-aligned current (FAC) in each event was located at the position of the auroral breakup and subsequently calculated the signature of the magnetic variation at the middle-latitude station Zyryanka (ZYK; GMLAT=59.6 degrees) that was generated by the upward FAC. In order to examine the magnetic effects of the upward FAC, we selected Pi2 events that were observed when ZYK was located on the duskward side of the auroral breakup location. A total of 112 events were selected and analyzed in this study. It was found that the location of the upward FAC of the SCW could be estimated more accurately by using an azimuth value predicted based on the initial deflection of the middle-latitude Pi2. Our results suggest that the circular shapes of Pi2 polarization curves are caused by the delayed driven Alfvenic waves that are superimposed on the geomagnetic northward components of SCW oscillations.

    DOI: 10.1002/2015JA021698

  • The prolonged southward IMF-B<inf>z</inf> event of 2–4 May 1998: Solar, interplanetary causes and geomagnetic consequences

    Susanta Kumar Bisoi, D. Chakrabarty, P. Janardhan, R. G. Rastogi, A. Yoshikawa, K. Fujiki, M. Tokumaru, Y. Yan

    Journal of Geophysical Research A: Space Physics   121 ( 5 )   3882 - 3904   2016.5

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    The prolonged southward IMF-B<inf>z</inf> event of 2–4 May 1998: Solar, interplanetary causes and geomagnetic consequences
    A detailed investigation is carried out to understand the prolonged (∼44 h) weakly southward interplanetary magnetic field (IMF-Bz) condition during 2–4 May 1998. In situ observations, during the period, show the passage of an expanding magnetic cloud embedded in an interplanetary coronal mass ejection (ICME), followed up by a shock and an interplanetary discontinuity driven by another ICME. It is the arrival of the ICMEs and the upfront shocks that caused the prolonged southward IMF-Bz condition. The magnetic configuration of the source regions of the IMF associated with the ICME interval was also examined, which showed open magnetic field structures, emanating from a small active region on the north of the heliospheric current sheet (HCS). The structures remained constantly to the north of the HCS, both on 29 April and 1 May, suggesting no change in their polarity. The draping of these outward directed radial field lines around the propagating CMEs in the shocked plasma explains the observed polarity changes of the IMF-Bz at 1 AU. In addition, multiple enhancements were also detected in the geomagnetic field variations, which showed a distinct one-to-one correspondence with the density pulses observed at 1 AU, during 0700–1700 UT on 3 May. The spectral analyses of both the variations showed the same discrete frequencies of 0.48, 0.65, and 0.75 mHz, demonstrating that the solar wind density enhancements can cause detectable global geomagnetic disturbances. The observations, thus, provide a deeper insight into the possible causes and geomagnetic consequences of a prolonged weakly southward IMF-Bz condition.

    DOI: 10.1002/2015JA022185

  • The prolonged southward IMF-B-z event of 2-4 May 1998: Solar, interplanetary causes and geomagnetic consequences Reviewed

    Susanta Kumar Bisoi, D. Chakrabarty, P. Janardhan, R. G. Rastogi, A. Yoshikawa, K. Fujiki, M. Tokumaru, Y. Yan

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   121 ( 5 )   3882 - 3904   2016.5

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    A detailed investigation is carried out to understand the prolonged (approximate to 44h) weakly southward interplanetary magnetic field (IMF-B-z) condition during 2-4 May 1998. In situ observations, during the period, show the passage of an expanding magnetic cloud embedded in an interplanetary coronal mass ejection (ICME), followed up by a shock and an interplanetary discontinuity driven by another ICME. It is the arrival of the ICMEs and the upfront shocks that caused the prolonged southward IMF-B-z condition. The magnetic configuration of the source regions of the IMF associated with the ICME interval was also examined, which showed open magnetic field structures, emanating from a small active region on the north of the heliospheric current sheet (HCS). The structures remained constantly to the north of the HCS, both on 29 April and 1 May, suggesting no change in their polarity. The draping of these outward directed radial field lines around the propagating CMEs in the shocked plasma explains the observed polarity changes of the IMF-B-z at 1 AU. In addition, multiple enhancements were also detected in the geomagnetic field variations, which showed a distinct one-to-one correspondence with the density pulses observed at 1 AU, during 0700-1700 UT on 3 May. The spectral analyses of both the variations showed the same discrete frequencies of 0.48, 0.65, and 0.75 mHz, demonstrating that the solar wind density enhancements can cause detectable global geomagnetic disturbances. The observations, thus, provide a deeper insight into the possible causes and geomagnetic consequences of a prolonged weakly southward IMF-B-z condition.

    DOI: 10.1002/2015JA022185

  • Long-term EEJ Variations by Using the Improved EE-index Reviewed International journal

    @Fujimoto, @A, Akimasa Yoshikawa, @T. Uozumi, @S. Abe, #H. Matsushita

    Sun and Geosphere   11 ( 1 )   2016.4

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  • Eastward-expanding auroral surges observed in the post-midnight sector during a multiple-onset substorm

    Yoshimasa Tanaka, Yasunobu Ogawa, Akira Kadokura, Noora Partamies, Daniel Whiter, Carl Fredrik Enell, Urban Brändström, Tima Sergienko, Björn Gustavsson, Alexander Kozlovsky, Hiroshi Miyaoka, Akimasa Yoshikawa

    Earth, Planets and Space   67 ( 1 )   WEB ONLY   2015.12

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    We present three eastward-expanding auroral surge (EEAS) events that were observed intermittently at intervals of about 15 min in the post-midnight sector (01:55-02:40 MLT) by all-sky imagers and magnetometers in northern Europe. It was deduced that each surge occurred just after each onset of a multiple-onset substorm, which was small-scale and did not clearly expand westward, because they were observed almost simultaneously with Pi 2 pulsations at the magnetic equator and magnetic bay variations at middle-to-high latitudes associated with the DP-1 current system. The EEASs showed similar properties to omega bands or torches reported in previous studies, such as recurrence intervals of about 15 min, concurrence with magnetic pulsations with amplitudes of several tens of nanotesla, horizontal scales of 300-400 km, and occurrence of a pulsating aurora in a diffuse aurora after the passage of the EEASs. Furthermore, the EEASs showed similar temporal evolution to the omega bands, during which eastward-propagating auroral streamers occurred simultaneously in the poleward region, followed by the formation of north-south-aligned auroras, which eventually connected with the EEASs. Thus, we speculate that EEASs may be related to the generation process of omega bands. On the other hand, the EEASs we observed had several properties that were different from those of omega bands, such as greater eastward propagation speed (3-4 km/s), shorter associated magnetic pulsation periods (4-6 min), and a different ionospheric equivalent current direction. The fast eastward propagation speed of the EEASs is consistent with the speed of eastward expansion fronts of the substorm current wedge reported in previous studies. The difference in the ionospheric current between the EEASs and omega bands may be caused by a large temporal variation of the surge structure, compared with the more stable wavy structure of omega bands.

    DOI: 10.1186/s40623-015-0350-8

  • NmF2 and hmF2 measurements at 95° e and 127° e around the EIA northern crest during 2010-2014 Reviewed International journal

    Bitap Raj Kalita, Pradip Kumar Bhuyan, @Akimasa Yoshikawa

    Earth, Planets and Space   67 ( 1 )   2015.12

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    The characteristics of the F2 layer parameters NmF2 and hmF2 over Dibrugarh (27.5° N, 95° E, 17° N geomagnetic, 43° dip) measured by a Canadian Advanced Digital Ionosonde (CADI) for the period of August 2010 to July 2014 are reported for the first time from this low mid-latitude station lying within the daytime peak of the longitudinal wave number 4 structure of equatorial anomaly (EIA) around the northern edge of anomaly crest. Equinoctial asymmetry is clearly observed at all solar activity levels whereas the midday winter anomaly is observed only during high solar activity years and disappears during the temporary dip in solar activity in 2013 but forenoon winter anomaly can be observed even at moderate solar activity. The NmF2/hmF2 variations over Dibrugarh are compared with that of Okinawa (26.5° N, 127° E, 17° N geomagnetic), and the eastward propagation speed of the wave number 4 longitudinal structure from 95° E to 127° E is estimated. The speed is found to be close to the theoretical speed of the wave number 4 (WN4) structure. The correlation of daily NmF2 over Dibrugarh and Okinawa with solar activity exhibits diurnal and seasonal variations. The highest correlation in daytime is observed during the forenoon hours in equinox. The correlation of daily NmF2 (linear or non-linear) with solar activity exhibits diurnal variation. A tendency for amplification with solar activity is observed in the forenoon and late evening period of March equinox and the postsunset period of December solstice. NmF2 saturation effect is observed only in the midday period of equinox. Non-linear variation of neutral composition at higher altitudes and variation of recombination rates with solar activity via temperature dependence may be related to the non-linear trend. The noon time maximum NmF2 over Dibrugarh exhibits better correlation with equatorial electrojet (EEJ) than with solar activity and, therefore, new low-latitude NmF2 index is proposed taking both solar activity and EEJ strength into account.

    DOI: 10.1186/s40623-015-0355-3

  • Empirical model of equatorial electrojet based on ground-based magnetometer data during solar minimum in fall 3. Space science Reviewed

    Nurul Shazana Abdul Hamid, Huixin Liu, Teiji Uozumi, Akimasa Yoshikawa

    Earth, Planets and Space   67 ( 1 )   205   2015.12

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    In this study, we constructed an empirical model of the equatorial electrojet (EEJ), including local time and longitudinal dependence, based on simultaneous data from 12 magnetometer stations located in six longitude sectors. An analysis was carried out using the equatorial electrojet index, EUEL, calculated from the geomagnetic northward H component. The magnetic EEJ strength is calculated as the difference between the normalized EUEL index of the magnetic dip equator station and the normalized EUEL index of the off-dip equator station located beyond the EEJ band. Analysis showed that this current is always strongest in the South American sector, regardless of local time (LT), and weakest in the Indian sector during 0900 and 1000 LT, but shifted to the African sector during 1100 to 1400 LT. These longitude variations of EEJ roughly follow variations of the inversed main field strength along the dip equator, except for the Indian and Southeast Asian sectors. The result showed that the EEJ component derived from the model exhibits a similar pattern with measured EEJ from ground data during noontime, mainly before 1300 LT.

    DOI: 10.1186/s40623-015-0373-1

  • Lorentz Dispersion Law from classical Hydrogen electron orbits in AC electric field via geometric algebra Reviewed International journal

    Uzziel Perez, @Akimasa Yoshikawa, Quirino M. Sugon, Jr., Daniel J. McNamara

    arXiv:1507.04509v1   2015.10

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    We studied the orbit of an electron revolving around an infinitely massive nucleus of a large classical Hydrogen atom subject to an AC electric field oscillating perpendicular to the electron’s circular orbit. Using perturbation theory in geometric algebra, we show that the equation of motion of the electron perpendicular to the unperturbed orbital plane satisfies a forced simple harmonic oscillator equation found in Lorentz dispersion law in Optics. We show that even though we did not introduce a damping term, the initial orbital position and velocity of the electron results to a solution whose absorbed energies are finite at the dominant resonant frequency ω = ω0; the electron slowly increases its amplitude of oscillation until it becomes ionized. We computed the average power absorbed by the electron both at the perturbing frequency and at the electron’s orbital frequency. We graphed the trace of the angular momentum vector at different frequencies. We showed that at different perturbing frequencies, the angular momentum vector traces epicyclical patterns.

  • The 2011 eruption of Aso volcano, Japan, and its signature on the geomagnetic field measurements Reviewed

    E. M. Takla, H. Odah, E. M. Abd Elaal, A. Yoshikawa, H. Kawano, T. Uozumi

    Arabian Journal of Geosciences   8 ( 10 )   8497 - 8503   2015.10

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    High-resolution (1-s) geomagnetic data from the MAGDAS Network, Kyushu University, Japan, were examined to detect any local anomalous geomagnetic behavior that is possibly linked with the eruption of the Aso volcano, Kyushu Island, Japan, during 2011. Geomagnetic data recorded in the vicinity of the Aso volcano at the Kuju (KUJ) station, Japan, were analyzed and compared with those recorded at the Darwin (DAW) station in Australia, near the conjugate point of the KUJ station. The KUJ station is located about 20 km northeast of the Aso volcano. The amplitude range of daily variations was calculated and examined for the three geomagnetic components (H-, D-, and Z-components) along with the amplitude of ultra–low-frequency emissions in the Pc3-4 ranges (Pc3; 10–45 s and Pc4; 45–150 s). Data possessing and analysis reveal some local anomalous geomagnetic variations at the KUJ station during the 2011 volcanic activities of the Aso volcano. On the other hand, no anomalous changes were observed at the DAW station during that time. Therefore, the observed anomalous geomagnetic variations are considered to be of a local volcanic origin.

    DOI: 10.1007/s12517-015-1858-8

  • A Prolonged Southward IMF-Bz Event of May 02--04, 1998: Solar, Interplanetary Causes and Geomagnetic Consequences Reviewed International journal

    Susanta Kumar Biso, D Chakrabarty, P Janardhan, RG Rastogi, @Akimasa Yoshikawa, K Fujiki, M Tokumaru, Y Yan, A

    arXiv:1604.04959   2015.10

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  • Magnetic and ionospheric observations in the Far Eastern region of Russia during the magnetic storm of 5 April 2010 Reviewed International journal

    Baishev D.G, Moiseyev A.V, Boroyev R.N, Kobyakova S.E, Stepanov A.E, Mandrikova O.V, Solovev I.S, Khomutov S.Yu, Polozov Yu.A, @Akimasa Yoshikawa, @Kiyohumi Yumoto

    Cosmic Research   10 ( 2 )   133 - 140   2015.9

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    Magnetic and ionospheric disturbances in the far eastern region of Russia during the magnetic storm of 5 April 2010 are studied using data of geophysical stations operated by IKFIA SB RAS and IKIR FEB RAS. By performing wavelet analysis of experimental data, the wavelet powers of geomagnetic perturbations at different stations are estimated, in an attempt to investigate the dynamical development of a geomagnetic storm. It is shown that, though weak geomagnetic disturbances were present prior to the main phase of magnetic storm, the variations of the magnetic field during a storm development were found to be rather strong. The highest intensity of geomagnetic disturbances during the interplanetary shock at the Earth's magnetosphere was observed at KTN (L~9) while at ZYK (L~4) strongest geomagnetic perturbations
    occurred during the magnetospheric substorm with the onset at 09:03 UT. Large geomagnetic fluctuations were recorded at TIX and CHD (L~5-6), when the High-Intensity Long-Duration Continuous AE Activity (HILDCAA) was observed on 6 April 2010. Ionospheric conditions at YAK (L~3.4) and PET (L~2.2) were characterized by a pre-storm enhancement in the electron density in the F2 layer on 4 April 2010 and prolonged negative phase of the ionospheric storm during the main and recovery phases of magnetic storm on 6-8 April 2010. These experimental results underscore the importance of multiinstrumental observations and provide clues to the complex interactive processes.

  • Variations of ULF and VLF during moderate geomagnetic storm at equatorial region Reviewed

    S. N.A. Ahmad, M. H. Jusoh, F. A.M. Kasran, M. Abdullah, B. Veenadhari, T. Uozumi, S. Abe, A. Yoshikawa, M. G. Cardinal

    International Conference on Space Science and Communication, IconSpace   2015-September   256 - 261   2015.9

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    This paper presents variations of Ultra Low Frequency (ULF) and Very Low Frequency (VLF) during moderate geomagnetic storm using ground based observatories, Magnetic Data Acquisition System (MAGDAS)/Circum-Pan Magnetic Network (CPMN) magnetometer and Atmospheric Weather Electromagnetic System for Observation Modeling and Education (AWESOME) VLF receiver. In this analysis, the recorded ULF horizontal (H)-component are extracted from MAGDAS magnetometer at Yap Island (YAP), Federated States of Micronesia, Davao (DAV), Philippines, and Tirunelveli (TIR), India stations. VLF amplitude data were observed from VLF receiver at UKM while the transmitters are located at Katabomman (VTX), India, North West Cape (NWC), Australia and Lualualei, Hawaii (NPM), USA. The observations of the space weather conditions in this study are divided into two categories: quiet day (10 April 2010) and moderate geomagnetic storm (6 April 2010). The results show that the ULF and VLF variations are significantly affected during geomagnetic storm which geomagnetic activities are closely related with the solar parameters.

    DOI: 10.1109/IconSpace.2015.7283762

  • Longitudinal and solar activity dependence of equatorial electrojet at Southeast Asian sector Reviewed

    N. S.A. Hamid, H. Liu, T. Uozumi, G. K. Gopir, H. A. Hadin, A. Yoshikawa

    International Conference on Space Science and Communication, IconSpace   2015-September   262 - 266   2015.9

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    In the E layer of equatorial ionosphere, the equatorial electrojet (EEJ) current interacts with the global Sq current and caused abnormally large amplitude of geomagnetic field component measured at the magnetic dip equator station. In this study, we attempted to separate EEJ and Sq at dip equator using the EUEL index derived from MAGDAS/CPMN stations. Moreover, we normalized the observation data to overcome the uncertainties due to the latitudinal variation of both EEJ and Sq currents which are neglected in most of previous studies. This new approach allowed the study of longitudinal dependence of EEJ. Analysis is performed using data from stations at East and West of Southeast Asian sector for a year of 2011. Additionally, we examined the solar activity dependence of EEJ during this inclining phase of solar cycle.

    DOI: 10.1109/IconSpace.2015.7283763

  • Longitudinal and Solar Activity Dependence of Equatorial Electrojet At Southeast Asian Sector Invited Reviewed International journal

    Hamid, N. S. A., @Huixin Liu,@Uozumi, T., Gopir, G. K., Hadin, H. A, @Akimasa Yoshikawa

    2015 INTERNATIONAL CONFERENCE ON SPACE SCIENCE AND COMMUNICATION (ICONSPACE)   262 - 266   2015.8

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  • Longitudinal and Solar Activity Dependence of Equatorial Electrojet At Southeast Asian Sector Reviewed International journal

    Hamid, N. S. A., @Huixin Liu, @Uozumi, T, Gopir, G. K., Hadin, H. A., @Akimasa Yoshikawa

    2015 INTERNATIONAL CONFERENCE ON SPACE SCIENCE AND COMMUNICATION (ICONSPACE)   262 - 266   2015.8

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  • Variations of ULF and VLF During Moderate Geomagnetic Storm At Equatorial Region Invited Reviewed International journal

    Ahmad, S. N. A., Jusoh, M. H., Kasran, F. A. M, Abdullah, M., Veenadhari, B., @Uozumi, T., @Abe, S., @Akimasa Yoshikawa, @MARIA GRACITA CARDINAL

    2015 INTERNATIONAL CONFERENCE ON SPACE SCIENCE AND COMMUNICATION (ICONSPACE)   256 - 261   2015.8

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  • Generation of different long-period geomagnetic pulsations during a sudden impulse Reviewed

    A. V. Moiseyev, V. I. Popov, V. A. Mullayarov, S. N. Samsonov, A. Du, A. Yoshikawa

    Cosmic Research   53 ( 4 )   257 - 266   2015.7

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    The space–time characteristics of geomagnetic pulsations during a sudden impulse on August 4, 2010 have been analyzed using ground-based and satellite observations. It has been indicated that two types of geomagnetic pulsations with different spatial extensions, oscillation frequencies, and generations were observed at that time. It has been found that geomagnetic pulsations with identical oscillation frequencies (∼4.5 mHz) at different latitudes were observed, with a maximal amplitude in the dusk sector. Oscillations with close frequencies were registered in the solar wind in the IMF B<inf>z</inf> component. Higher-frequency (7–10 mHz) pulsations dependent on latitude were registered on the dawn side. It is assumed that geomagnetic pulsations with frequencies of ∼4.5 mHz were caused by oscillations penetrating from the interplanetary medium, and higher-frequency pulsations were Alfvén resonance oscillations generated during the compression of the magnetosphere. An asymmetric oscillation amplitude distribution relative to noon was caused by the IMF orthospiral orientation in this event.

    DOI: 10.1134/S001095251504005X

  • Spatial variability of solar quiet fields along 96° magnetic meridian in Africa: Results from MAGDAS

    O. S. Bolaji, A. B. Rabiu, A. B. Rabiu, O. R. Bello, A. Yoshikawa, K. Yumoto, O. O. Odeyemi, O. Ogunmodimu

    Journal of Geophysical Research: Space Physics   120 ( 5 )   3883 - 3898   2015.5

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    Spatial variability of solar quiet fields along 96° magnetic meridian in Africa: Results from MAGDAS
    We have used chains of Magnetic Data Acquisition System (MAGDAS) magnetometer records of the horizontal (H) and vertical (Z) magnetic field intensities during September 2008 to August 2009 (year of deep minimum) across Africa to study their variability during the quietest international days, which coincidently associated with the sudden stratospheric warming (SSW) event in January 2009. This selection of the most international quiet days is indicative of 80&#37; that are strongly associated with days when unusually strong and prolonged sudden SSW event occurs in January 2009. Interestingly, in January, a significant magnitude depletion of solar quiet (Sq) equivalent current was observed near noon hours around the magnetic equator (Addis Ababa, ABB) compared to any other months along with a consistent significantly reduced value across the Northern Hemisphere and moderate decrease at the Southern Hemisphere. Also, we found that Nairobi and Dar es Salaam at the Southern Hemisphere, which are close to ABB (dip equator), are strongly prone to westward electric field compared to the magnetic equator and Khartoum at the Northern Hemisphere. Significant negative values of MSq(Z) magnitudes observed near noon hours at Hermanus indicate the presence of induced currents that suggest ocean effects along with reversal to significant positive values in the afternoon, which subsided before 1800-LT in almost all the months, indicate stronger influence of ionospheric currents. On seasonal variability of Sq(H), a slight depression at ABB during September equinox is one of the evidences of seasonal Sq focus shift. Latitudinal variability of Sq near-noon hours was also investigated. Key Points Abnormal intensification of electric currents Latitudinal sections of the African stations Highest and positive magnitude in February

    DOI: 10.1002/2014JA020728

  • Spatial variability of solar quiet fields along 96 degrees magnetic meridian in Africa: Results from MAGDAS Reviewed

    O. S. Bolaji, A. B. Rabiu, O. R. Bello, A. Yoshikawa, K. Yumoto, O. O. Odeyemi, O. Ogunmodimu

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   120 ( 5 )   3883 - 3898   2015.5

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    We have used chains of Magnetic Data Acquisition System (MAGDAS) magnetometer records of the horizontal (H) and vertical (Z) magnetic field intensities during September 2008 to August 2009 (year of deep minimum) across Africa to study their variability during the quietest international days, which coincidently associated with the sudden stratospheric warming (SSW) event in January 2009. This selection of the most international quiet days is indicative of 80&#37; that are strongly associated with days when unusually strong and prolonged sudden SSW event occurs in January 2009. Interestingly, in January, a significant magnitude depletion of solar quiet (S-q) equivalent current was observed near noon hours around the magnetic equator (Addis Ababa, ABB) compared to any other months along with a consistent significantly reduced value across the Northern Hemisphere and moderate decrease at the Southern Hemisphere. Also, we found that Nairobi and Dar es Salaam at the Southern Hemisphere, which are close to ABB (dip equator), are strongly prone to westward electric field compared to the magnetic equator and Khartoum at the Northern Hemisphere. Significant negative values of MSq(Z) magnitudes observed near noon hours at Hermanus indicate the presence of induced currents that suggest ocean effects along with reversal to significant positive values in the afternoon, which subsided before 1800 LT in almost all the months, indicate stronger influence of ionospheric currents. On seasonal variability of S-q(H), a slight depression at ABB during September equinox is one of the evidences of seasonal S-q focus shift. Latitudinal variability of Sq near-noon hours was also investigated.

    DOI: 10.1002/2014JA020728

  • Pi2 pulsations observed around the dawn terminator Reviewed

    #S. Imajo, @Akimasa Yoshikawa, @T. Uozumi, S. Ohtani, A. Nakamizo, R. Marshall, B. M. Shevtsov, V. A. Akulichev, U. Sukhbaatar, A. Liedloff, @K. Yumoto

    Journal of Geophysical Research   120 ( 3 )   2088 - 2098   2015.3

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    We examined Pi2 pulsations observed simultaneously at low-latitude stations (L = 1.15 - 2.33) around the dawn terminator. Those Pi2 pulsations observed in the sunlit region were polarized in the azimuthal (D, positive eastward) direction. We found that the D component oscillations in the dark and sunlit regions were in antiphase, whereas the H component oscillated in phase. A statistical analysis indicates that these D component phase reversals occurred about 0.5 h sunward of the dawn terminator at 100 km in altitude, corresponding to the highly conducting E layer. The azimuthal polarization and D component phase reversals related to the dawn terminator cannot be explained by the existing models of low-latitude Pi2s (e.g., cavity resonance or substorm current wedge oscillations). Similar D component phase reversals were also found on the dusk side although the amplitude of the D component is smaller than that of the H component. We suggest that the meridional ionospheric current in the sunlit region adjacent to the dawn terminator drives the D component oscillations in antiphase with those D oscillations produced by the oscillatory field-aligned current (FAC) on the postmidnight side. The meridional current is expected to form a part of a current system that extends from the postmidnight FAC to the equatorial Cowling current. The D component oscillations in the Northern and Southern Hemispheres are also in antiphase, indicating that the current system is symmetric with respect to the equator. Key Points We examined Pi2 pulsations observed at low latitudes around the dawn terminator Phase reversals of the east-west component occur near the dawn terminator We suggest that meridional ionospheric current drives the east-west oscillation

    DOI: 10.1002/2013JA019691

  • 低緯度朝側昼夜境界付近で観測されるPi2型地磁気脈動と湾型磁場変動 Reviewed

    IMAJO Shun, YOSHIKAWA Akimasa, UOZUMI Teiji, OHTANI Shinichi, NAKAMIZO Aoi

    地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM)   120 ( 3 )   2088 - 2098   2015.3

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    Pi2 pulsations observed around the dawn terminator
    We examined Pi2 pulsations observed simultaneously at low-latitude stations (L = 1.15 - 2.33) around the dawn terminator. Those Pi2 pulsations observed in the sunlit region were polarized in the azimuthal (D, positive eastward) direction. We found that the D component oscillations in the dark and sunlit regions were in antiphase, whereas the H component oscillated in phase. A statistical analysis indicates that these D component phase reversals occurred about 0.5 h sunward of the dawn terminator at 100 km in altitude, corresponding to the highly conducting E layer. The azimuthal polarization and D component phase reversals related to the dawn terminator cannot be explained by the existing models of low-latitude Pi2s (e.g., cavity resonance or substorm current wedge oscillations). Similar D component phase reversals were also found on the dusk side although the amplitude of the D component is smaller than that of the H component. We suggest that the meridional ionospheric current in the sunlit region adjacent to the dawn terminator drives the D component oscillations in antiphase with those D oscillations produced by the oscillatory field-aligned current (FAC) on the postmidnight side. The meridional current is expected to form a part of a current system that extends from the postmidnight FAC to the equatorial Cowling current. The D component oscillations in the Northern and Southern Hemispheres are also in antiphase, indicating that the current system is symmetric with respect to the equator. Key Points We examined Pi2 pulsations observed at low latitudes around the dawn terminator Phase reversals of the east-west component occur near the dawn terminator We suggest that meridional ionospheric current drives the east-west oscillation

    DOI: 10.1002/2013JA019691

  • CDF data archive and integrated data analysis platform for ERG-related ground data developed by ERG Science Center (ERG-SC) Reviewed

    Hori, T, Y. Miyashita, Y. Miyoshi, K. Seki, T. Segawa, Y.-M. Tanaka, K. Keika, M. Shoji, I. Shinohara, K. Shiokawa, Y. Otsuka, S. Abe, A. Yoshikawa, K. Yumoto, Y. Obana, N. Nishitani, A. S. Yukimatu, T. Nagatsuma, M. Kunitake, K. Hosokawa, Y. Ogawa, K. T. Murata, M. Nose, H. Kawano, T. Sakanoi

    宇宙航空研究開発機構研究開発報告: 宇宙科学情報解析論文誌   4 (JAXA-RR-14-009)   75 - 89   2015.3

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    CDF data archive and integrated data analysis platform for ERG-related ground data developed by ERG Science Center (ERG-SC)
    The Exploration of energization and Radiation in Geospace project Science Center (ERG-SC) has developed the science data file archive and integrated data analysis tool for the ground network observation data of the ERG project. We have organized data design consortiums to develop and elaborate the standard metadata and data variable sets for each type of the ERG-related ground data being archived as Common Data Format (CDF) files. The integrated data analysis software for the project has also been developed on the basis of the Space Physics Environment Data Analysis Software (SPEDAS) which works in concert with the CDF data file repository. The software tools, which are provided as plug-in libraries for SPEDAS, are made available to the international science community so that scientists and students are ready to proceed to integrated studies combining the ground data with other satellite and simulation data seamlessly. The integrated data analysis software can make scientific activities more productive and help the ERG project achieve the scientific goals.

  • Near-equatorial Pi2 and Pc3 waves observed by CHAMP and on SAMBA/MAGDAS stations Reviewed International journal

    Cuturrufo, F, Pilipenko, V, Heilig, B, Stepanova, M, Luehr, H, Vega, P, @Akimasa Yoshikawa

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   55 ( 4 )   2015.2

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    DOI: 10.1016/j.asr.2014.11.010

  • Near-equatorial Pi2 and Pc3 waves observed by CHAMP and on SAMBA/MAGDAS stations Reviewed

    F. Cuturrufo, V. Pilipenko, B. Heilig, M. Stepanova, H. Lühr, P. Vega, A. Yoshikawa

    Advances in Space Research   55 ( 4 )   1180 - 1189   2015.2

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    We have examined simultaneous ULF activity in the Pi2 and Pc3 bands at the near-equatorial magnetic stations in South America from SAMBA and MAGDAS arrays and low-orbiting CHAMP satellite during its passage over this meridional network. At the nighttime, both Pi2 and Pc3 waves in the upper ionosphere and on the ground are nearly of the same magnitude and in-phase. At the same time, the daytime Pc3 pulsations on the ground and in space are nearly out-of-phase. Comparison of observational results with the theoretical notions on the MHD wave interaction with the system ionosphere-atmosphere-ground suggests that nighttime low-latitude Pi2 and Pc3 wave signatures are produced by magnetospheric fast compressional mode. The daytime near-equatorial Pc3 waves still resist a quantative interpretation. These waves may be produced by a combination of two mechanisms: compressional mode leakage through the ionosphere, and by oscillatory ionospheric current spreading towards equatorial latitudes.

    DOI: 10.1016/j.asr.2014.11.010

  • Anomalous ULF emissions and their possible association with the strong earthquakes in sumatra, Indonesia, during 2007-2012 Reviewed International journal

    Suaidi Ahadi, Nanang Tyasbudi Puspito, Gunawan Ibrahim, Sarmoko Saroso, Kiyohumi Yumoto, @Akimasa Yoshikawa, L. Muzli

    Journal of Mathematical and Fundamental Sciences   47 ( 1 )   84 - 103   2015.1

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    Eleven strong Sumatran earthquakes, with their epicenter less than 550 km away from the Kototabang (KTB) geomagnetic station (2007-2012), were studied to examine the occurrence of anomalous ultra-low frequency emissions (ULF-EM). Anomalous ULF signals, possibly associated with the earthquake’s precursors, were determined by the Welch ratio SZ/SH at 0.06 Hz at the KTB station. These ULF anomalies were then compared with geomagnetic data observed from two reference stations in Darwin and Davao, to prevent misinterpretation of global geomagnetic disturbances as precursors. This study aims to analyze the relationship between earthquake magnitude and hypocenter radius, and seismic index against lead time during ULF-EM anomalies. We used the polarization ratio Welch method in terms of power spectrum density to evaluate the geomagnetic data by overlapping windows and applying fast Fourier transform (FFT). The results showed anomalous variations in onset and lead time, determined using the standard deviation controlling the SZ/SH power pattern. Our positive correlation between lead time of ULF emission and earthquake magnitude as well as between lead time and seismic index. It shows a negative correlation between hypocenter distances to KTB station against lead time.

    DOI: 10.5614/j.math.fund.sci.2015.47.1.7

  • Approximate forms of daytime ionospheric conductance Reviewed

    A. Ieda, S. Oyama, H. Vanhamäki, R. Fujii, A. Nakamizo, O. Amm, T. Hori, M. Takeda, G. Ueno, A. Yoshikawa, R. J. Redmon, W. F. Denig, Y. Kamide, N. Nishitani

    Journal of Geophysical Research: Space Physics   119 ( 12 )   10,397 - 10,415   2014.12

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    The solar zenith angle (SZA) dependence of the conductance is studied and a simple theoretical form for the Hall-to-Pedersen conductance ratio is developed, using the peak plasma production height. The European Incoherent Scatter (EISCAT) radar observations at Tromsø (67 MLAT) on 30 March 2012 were used to calculate the conductance. The daytime electric conductance is associated with plasma created by solar extreme ultraviolet radiation incident on the neutral atmosphere of the Earth. However, it has been uncertain whether previous conductance models are consistent with the ideal Chapman theory for such plasma productions. We found that the SZA dependence of the conductance is consistent with the Chapman theory after simple modifications. The Pedersen conductance can be understood by approximating the plasma density height profile as being flat in the topside E region and by taking into account the upward gradient of atmospheric temperature. An additional consideration is necessary for the Hall conductance, which decreases with increasing SZA more rapidly than the Pedersen conductance. This rapid decrease is presumably caused by a thinning of the Hall conductivity layer from noon toward nighttime. We expressed this thinning in terms of the peak production height in the Chapman theory. Key Points Solar zenith angle dependence of the conductance is theoretically studied The dependence is different between the Hall and the Pedersen conductances The Hall conductivity layer thins from noon to sunset

    DOI: 10.1002/2014JA020665

  • Flapping current sheet with superposed waves seen in space and on the ground Reviewed

    G. Q. Wang, M. Volwerk, R. Nakamura, P. Boakes, T. L. Zhang, A. Yoshikawa, D. G. Baishev

    Journal of Geophysical Research: Space Physics   119 ( 12 )   10,078 - 10,091   2014.12

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    A wavy current sheet event observed on 15 October 2004 between 1235 and 1300 UT has been studied by using Cluster and ground-based magnetometer data. Waves propagating from the tail center to the duskside flank with a period ∼30 s and wavelength ∼1 RE are superimposed on a flapping current sheet, accompanied with a bursty bulk flow. Three Pi2 pulsations, with onset at ∼1236, ∼1251, and ∼1255 UT, respectively, are observed at the Tixie station located near the foot points of Cluster. The mechanism creating the Pi2 (period ∼40 s) onset at ∼1236 UT is unclear. The second Pi2 (period ∼90 s, onset at ∼1251 UT) is associated with a strong field-aligned current, which has a strong transverse component of the magnetic field, observed by Cluster with a time delay ∼60 s. We suggest that it is caused by bouncing Alfvén waves between the northern and southern ionosphere which transport the field-aligned current. For the third Pi2 (period ∼60 s) there is almost no damping at the first three periods. They occur in conjunction with periodic field-aligned currents one-on-one with 72 s delay. We suggest that it is generated by these periodic field-aligned currents. We conclude that the strong field-aligned currents generated in the plasma sheet during flapping with superimposed higher-frequency waves can drive Pi2 pulsations on the ground, and periodic field-aligned currents can even control the period of the Pi2s. Key Points Flapping superimposed on waves (∼30 s) are accompanied with BBF during substorm The waves propagate from the tail center to the duskside flank Field-aligned currents drive Pi2s on the ground, even control their period

    DOI: 10.1002/2014JA020526

  • Relationship between the equatorial electrojet and global Sq currents at the dip equator region Reviewed International journal

    Hamid, Nurul Shazana Abdu, @Huixin Liu, @Teiji Uozumi, @Kiyohumi Yumoto, @Akimasa Yoshikawa, Veenadhari, Bhaskara, Avendano Sanchez

    EARTH PLANETS AND SPACE   66   2014.10

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    DOI: 10.1186/s40623-014-0146-2

  • Data processing method to classify Pc5 ULF pulsations due to solar wind perturbations at equatorial region Reviewed

    Siti Noor Aisyah Ahmad, Mohamad Huzaimy Jusoh, Khairul Khaizi Mohd Shariff, Mardina Abdullah, Mhd Fairos Asillam, B. Veenadhari, @T. Uozumi, @. Abe, @Akimasa Yoshikawa, @M. G. Cardinal

    WSEAS Transactions on Signal Processing   10 ( 1 )   337 - 344   2014.10

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    Space weather study has increasingly attracts the attention of many scientists to explore the interaction between solar activity and geomagnetic activity. Observation on Pc5 geomagnetic pulsations with periods ranging from 150-600seconds due to solar wind perturbations at the equatorial region currently not widely explored. In this paper, we will briefly discuss the data processing methods involve in order to analyze the geomagnetic data observed by magnetometer from geomagnetic observation stations; Tirunelveli (TIR), India, Langkawi (LKW), Malaysia and Yap Island (YAP), Federated States of Micronesia which are located at equatorial region. The explanation of the processing methods is based on the 24-hour data with 1 second sampling interval extracted during quiet and disturbed days. The result indicates that the higher amplitude of H geomagnetic field is recorded during daytime and maintain during nighttime at all analyzed stations. In addition, Pc5 ULF pulsations are corresponding well with the solar wind perturbations.

  • Capacity building: A tool for advancing space weather science Reviewed

    M. G. Cardinal, A. Yoshikawa, H. Kawano, H. Liu, M. Watanabe, S. Abe, T. Uozumi, G. Maeda, T. Hada, K. Yumoto

    Space Weather   12 ( 10 )   571 - 576   2014.10

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    DOI: 10.1002/2014SW001110

  • Anomalous Geomagnetic Variations Associated with the Volcanic Activity of the Mayon Volcano, Philippines during 2009-2010 Reviewed International journal

    Takla, E.M, @Akimasa Yoshikawa, @Hideaki Kawano, @Teiji Uozumi, @Shuji Abe

    NRIAG Journal of Astronomy and Geophysics, DOI 10.1016/j.nrjag.2014.09.001.   2014.9

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    DOI: 10.1016/j.nrjag.2014.09.001

  • A case study of ionospheric storm effects during long-lasting southward IMF B<inf>z</inf>-driven geomagnetic storm Reviewed

    Jing Liu, Libo Liu, Takuji Nakamura, Biqiang Zhao, Baiqi Ning, A. Yoshikawa

    Journal of Geophysical Research: Space Physics   119 ( 9 )   7716 - 7731   2014.9

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    Multiple instrumental observations including GPS total electron content (TEC), foF2 and hmF2 from ionosondes, vertical ion drift measurements from Communication/Navigation Outage Forecasting System, magnetometer data, and far ultraviolet airglow measured by Thermosphere, Ionosphere, Mesosphere Energetics and Dynamics/Global Ultraviolet Imager (TIMED/GUVI) are used to investigate the profound ionospheric disturbances at midlatitude and low latitude during the 14-17 July 2012 geomagnetic storm event, which was featured by prolonged southward interplanetary geomagnetic field component for about 30h below -10 nT. In the East Asian/Australian sector, latitudinal profile of TEC variations in the main phase were characterized by three bands of increments and separated by weak depressions in the equatorial ionospheric anomaly (EIA) crest regions, which were caused by the combined effects of disturbance dynamo electric fields (DDEF) and equatorward neutral winds. In the recovery phase, strong inhibition of EIA occurred and the summer crest of EIA disappeared on 16 July due to the combined effects of intrusion of neutral composition disturbance zone as shown by the TIMED/GUVI O/N2 measurements and long-lasting daytime westward DDEF inferred from the equatorial electrojet observations. The transit time of DDEF over the dip equator from westward to eastward is around 2200 LT. In the American longitude, the salient ionospheric disturbances in the summer hemisphere were characterized by daytime periodical intrusion of negative phase for three consecutive days in the recovery phase, preceded by storm-enhanced density plume in the initial phase. In addition, multiple short-lived prompt penetration electric fields appeared during stable southward interplanetary magnetic field (IMF) Bz in the recovery phase and were responsible for enhanced the EIA and equatorial ionospheric uplift around sunset. Key Points Multiple PPEF occur when the IMF Bz was stable southwardThe negative ionospheric phase oscillated in the American sectorInhibitation of EIA was caused by O/N2 changes and DDEF

    DOI: 10.1002/2014JA020273

  • A case study of ionospheric storm effects during long-lasting southward IMF B-z-driven geomagnetic storm

    Jing Liu, Libo Liu, Takuji Nakamura, Biqiang Zhao, Baiqi Ning, A. Yoshikawa

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   119 ( 9 )   7716 - 7731   2014.9

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    Multiple instrumental observations including GPS total electron content (TEC), f(o)F(2) and h(m)F(2) from ionosondes, vertical ion drift measurements from Communication/Navigation Outage Forecasting System, magnetometer data, and far ultraviolet airglow measured by Thermosphere, Ionosphere, Mesosphere Energetics and Dynamics/Global Ultraviolet Imager (TIMED/GUVI) are used to investigate the profound ionospheric disturbances at midlatitude and low latitude during the 14-17 July 2012 geomagnetic storm event, which was featured by prolonged southward interplanetary geomagnetic field component for about 30 h below -10 nT. In the East Asian/Australian sector, latitudinal profile of TEC variations in the main phase were characterized by three bands of increments and separated by weak depressions in the equatorial ionospheric anomaly (EIA) crest regions, which were caused by the combined effects of disturbance dynamo electric fields (DDEF) and equatorward neutral winds. In the recovery phase, strong inhibition of EIA occurred and the summer crest of EIA disappeared on 16 July due to the combined effects of intrusion of neutral composition disturbance zone as shown by the TIMED/GUVI O/N-2 measurements and long-lasting daytime westward DDEF inferred from the equatorial electrojet observations. The transit time of DDEF over the dip equator from westward to eastward is around 2200 LT. In the American longitude, the salient ionospheric disturbances in the summer hemisphere were characterized by daytime periodical intrusion of negative phase for three consecutive days in the recovery phase, preceded by storm-enhanced density plume in the initial phase. In addition, multiple short-lived prompt penetration electric fields appeared during stable southward interplanetary magnetic field (IMF) B-z in the recovery phase and were responsible for enhanced the EIA and equatorial ionospheric uplift around sunset.

    DOI: 10.1002/2014JA020273

  • Pi2 pulsation simultaneously observed in the E and F region ionosphere with the SuperDARN Hokkaido radar Reviewed

    M. Teramoto, N. Nishitani, V. Pilipenko, T. Ogawa, K. Shiokawa, T. Nagatsuma, A. Yoshikawa, D. Baishev, K. T. Murata

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   119 ( 5 )   3444 - 3462   2014.5

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    We investigated Pi2 pulsations in the nightside ionosphere that began at 14:15 UT (2315 LT) on 11 July 2010, and they were observed with high-temporal (8s) resolution by beam 4 of the Super Dual Auroral Radar Network (SuperDARN) Hokkaido radar. These pulsations were simultaneously observed in both the ground/sea scatter echoes reflected from the F region height and in ionospheric echoes from field-aligned irregularities in the sporadic Es region. They had the same period of 110s and approximately no phase lag. From the radar observations and the International Geomagnetic Reference Field model, the amplitude of the eastward (EEW) component of the electric field of the Pi2 pulsations in the ionosphere was estimated similar to 8.0mV/m in the F region and similar to 2.0mV/m in the E region. Corresponding Pi2 pulsations appeared dominantly in the horizontal northward magnetic field component (H) at nearby ground stations, Moshiri (MSR), St. Paratunka (PTK), and Stecolny (STC), with amplitudes ranging from 6 nT (MSR) to 10 nT (STC). At the dominant frequency of 8.8 mHz, the coherences between H and EEW were high (>0.9), the cross phases of EEW relative to H were -56 degrees and -45 degrees, and the amplitude ratios were 2.7x105m/s and 8.4x105m/s, in the E and F regions, respectively. Based on a comparison of these results with theoretical predictions, we suggest that the concept of a pure cavity mode is not sufficient to explain the combined observations for midlatitude Pi2 waves and that the contribution of an Alfven waves must be taken in account.

    DOI: 10.1002/2012JA018585

  • Pi2 pulsation simultaneously observed in the e and F region ionosphere with the SuperDARN Hokkaido radar Reviewed

    M. Teramoto, N. Nishitani, V. Pilipenko, T. Ogawa, K. Shiokawa, T. Nagatsuma, A. Yoshikawa, D. Baishev, K. T. Murata

    Journal of Geophysical Research: Space Physics   119 ( 5 )   3444 - 3462   2014.5

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    We investigated Pi2 pulsations in the nightside ionosphere that began at 14:15 UT (2315 LT) on 11 July 2010, and they were observed with high-temporal (8 s) resolution by beam 4 of the Super Dual Auroral Radar Network (SuperDARN) Hokkaido radar. These pulsations were simultaneously observed in both the ground/sea scatter echoes reflected from the F region height and in ionospheric echoes from field-aligned irregularities in the sporadic Es region. They had the same period of 110 s and approximately no phase lag. From the radar observations and the International Geomagnetic Reference Field model, the amplitude of the eastward (EEW) component of the electric field of the Pi2 pulsations in the ionosphere was estimated ~8.0 mV/m in the F region and ~2.0 mV/m in the E region. Corresponding Pi2 pulsations appeared dominantly in the horizontal northward magnetic field component (H) at nearby ground stations, Moshiri (MSR), St. Paratunka (PTK), and Stecolny (STC), with amplitudes ranging from 6 nT (MSR) to 10 nT (STC). At the dominant frequency of 8.8 mHz, the coherences between H and EEW were high (>0.9), the cross phases of EEW relative to H were -56° and -45°, and the amplitude ratios were 2.7 × 105 m/s and 8.4 × 105 m/s, in the E and F regions, respectively. Based on a comparison of these results with theoretical predictions, we suggest that the concept of a pure cavity mode is not sufficient to explain the combined observations for midlatitude Pi2 waves and that the contribution of an Alfvén waves must be taken in account. Key Points Midlatitude SuperDARN radar observed Pi2 pulsations in the E and F regions The electric field of Pi2 pulsations in the ionosphere are estimated The conception of pure cavity mode is not sufficient ©2014. American Geophysical Union. All Rights Reserved.

    DOI: 10.1002/2012JA018585

  • Analysis of propagation delays of compressional Pi 2 waves between geosynchronous altitude and low latitudes Reviewed International journal

    #Imajo Shun, @Kiyofumi @Yumoto, @Hideaki Kawano, @Teiji Uozumi, @Abe Shuji, @Akimasa Yoshikawa

    EARTH PLANETS AND SPACE   66   2014.4

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    DOI: 10.1186/1880-5981-66-20

  • Ground magnetic effects of the equatorial electrojet simulated by the TIE‐GCM driven by TIMED satellite data Reviewed

    Yosuke Yamazaki, Arthur D. Richmond, Astrid Maute, Qian Wu, David A. Ortland, Akimasa Yoshikawa, Isaac Abiodun Adimula, Babatunde Rabiu, Manabu Kunitake, Takuya Tsugawa

    Journal of Geophysical Research: Space Physics   119 ( 4 )   3150 - 3161   2014.4

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    Ground magnetic effects of the equatorial electrojet simulated by the TIE-GCM driven by TIMED satellite data
    Quiet time daily variations of the geomagnetic field near the magnetic equator due to the equatorial electrojet are simulated using the National Center for Atmospheric Research Thermosphere-Ionosphere Electrodynamics General Circulation Model (TIE-GCM) and compared to those observed by ground-based magnetometers. Simulations are run both with and without tidal forcing at the height of the model lower boundary (∼97km). When the lower boundary forcing is off, the wind that generates an electromotive force in the model is primarily the vertically nonpropagating diurnal tide, which is excited in the thermosphere due to daytime solar ultraviolet heating. The lower boundary tidal forcing adds the effect of upward propagating tides, which are excited in the lower atmosphere and propagate vertically to the thermosphere. The main objective of this study is to evaluate the relative importance of these thermospherically generated tides and upward propagating tides in the generation of the equatorial electrojet. Fairly good agreement is obtained between model and observations when the model is forced by realistic lower boundary tides based on temperature and wind measurements from the Thermosphere-Ionosphere- Mesosphere Energetics and Dynamics (TIMED) satellite, as determined by Wu et al. (2012). The simulation results show that the effect of upward propagating tides increases the range of the geomagnetic daily variation in the magnetic-northward component at the magnetic equator approximately by 100&#37;. It is also shown that the well-known semiannual change in the daily variation is mostly due to upward propagating tides, especially the migrating semidiurnal tide. These results indicate that upward propagating tides play a substantial role in producing the equatorial electrojet and its seasonal variability. Key Points The ground magnetic effect of the equatorial electrojet is simulated Upward propagating tides explain about 50&#37; the magnetic effect The semiannual variation is mainly due to upward propagating tides ©2014. American Geophysical Union. All Rights Reserved.

    DOI: 10.1002/2013JA019487

  • Pc5 magnetic pulsations during the outer electron radiation belt Reviewed

    L. Muhammad K. Musafar, Triyanta, W. Sugitomo, T. Djamaluddin, @Akimasa Yoshikawa, @T. Uozumi

    International Journal of Technology   5 ( 3 )   269 - 276   2014.1

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    Since the discovery of the radiation belt decades ago, there still remain some fundamental questions as to which one is the mechanism responsible for the acceleration of electrons. Groundbased Pc5 magnetic pulsation during the process of increasing of 2-MeV electron fluxes has been analyzed. First, a filter bandpass in the period range of 150-600 seconds has been used to localize the Pc5 waves. Second, we then applied a wavelet transform procedure, whereby the Morlet function as a mother wavelet was selected to analyze Pc5 wave packets. First, we show that dynamic pressure of solar wind controls the power of Pc5 magnetic pulsations. Second, by performing a cross-spectrum analysis of Pc5 wavelet during electron radiation belts we show that the wavelet power of Pc5 magnetic pulsations which is associated with a maximum wavelet cross spectrum show a similar change of Pc5 pulsations occurs during radiation belt events. Increasing of electron fluxes which is initiated by the presence of large power of Pc5 magnetic pulsations has been observed. This indicates that Pc5 magnetic pulsations could play a role in the acceleration and transport mechanism of the electron radiation belt. Also, 4-5 days from the beginning of increasing of electron fluxes we observed globally, a depression in the power of Pc5 magnetic pulsations as well as a monotonically decreasing of the solar wind dynamic pressure. On the other hand, during the end period of the electron belt, we also observed a sudden increasing of Pc5 power. We suggest that during the expansion periode of the outer electron radiation belt outward to interplanetary electron belt pressure that will reduce the solar wind dynamic pressure and consequently a decrease occurs in the power of Pc5 magnetic pulsation. And, in the end period of the electron radiation belt the electron fluxes back to its normal level and consequently a sudden increase of the Pc5 solar wind dynamic pressure occurs and that sudden increase also drives the sudden increasing power of Pc5 magnetic pulsations.

    DOI: 10.14716/ijtech.v5i3.612

  • MAGDAS Capacity Building Activities for Space Weather Research at ICSWSE Reviewed International journal

    Akimasa Yoshikawa, M.G. Cardina, Tohru Hada, Kiyohumi Yumoto

    Research Note, Space Research Today, Volume 188, December 2013, Pages 18-20, ISSN 1752-9298, http://dx.doi.org/10.1016/j.srt.2013.11.007   188 ( 10 )   18 - 20   2013.11

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    DOI: 10.1016/j.srt.2013.11.007.

  • Illustration of Cowling channel coupling to the shear Alfven wave Reviewed

    A. Yoshikawa, O. Amm, H. Vanhamäki, R. Fujii

    Journal of Geophysical Research: Space Physics   118 ( 10 )   6405 - 6415   2013.10

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    Decomposition of horizontally extended current system into components in the polarization processes and extraction of Cowling channel defined in the companion paper embedded in the total current system are numerically demonstrated. We successfully visualize the background and polarization components in the magnetosphere-ionosphere coupling process by using the proposed theoretical framework. As a fundamental response, the polarization charge produced by the Pedersen current divergence has a role to cancel and intensify the ambient background electric field inside and outside the high-conductivity band, respectively. In contrast, the polarization charge produced by the Hall current divergence has a role to rotate the electric field from the background electric field, which causes a meandering of ionospheric convection flow along the boundary of a high-conductivity band. The Hall and Pedersen currents are always perpendicular to each other. They never close each other when conductances are homogeneous, but they can do that at the conductivity gradient region. This is the reason why a Hall polarization charge is induced and a resultant Cowling channel is formed. Key Points Illustration of Cowling channel Hall and Pedersen current close each other at the conductivity gradient region Identify the Hall polarization field and Alfven conductance ©2013. American Geophysical Union. All Rights Reserved.

    DOI: 10.1002/jgra.50513

  • Theory of Cowling channel formation by reflection of shear Alfven waves from the auroral ionosphere Reviewed

    A. Yoshikawa, O. Amm, H. Vanhamäki, A. Nakamizo, R. Fujii

    Journal of Geophysical Research: Space Physics   118 ( 10 )   6416 - 6425   2013.10

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    We present the first complete formulation of the coupling between the ionospheric horizontal currents (including Hall currents) and the field-aligned currents (FAC) via shear Alfven waves, which can describe the formation of a Cowling channel without any a priori parameterization of the secondary (Hall polarization) electric field strength. Our theory reorganizes the Cowling channel by "primary" and "secondary" fields. Until now there are no theoretical frameworks, which can derive these separated components from observed or given total conductance, electric field, and FAC distributions alone. But when a given incident where Alfven wave is considered as the driver, the reflected wave can be uniquely decomposed into the primary and secondary components. We show that the reflected wave can, depending on actual conditions, indeed carry FAC that connect to divergent Hall currents. With this new method, we can identify how large the secondary electric field becomes, how efficiently the divergent Hall current is closed within the ionosphere, and how much of the Hall current continues out to the magnetosphere as FAC. In typical ionospheric situations, only a small fraction of FAC is connected to Hall currents at conductance gradients, i.e., the secondary field is relatively strong. But when conductances are relatively low compared with Alfven conductance and/or horizontal scales smaller than ~10 km, the Hall FAC may become significant. Key Points Formation of Cowling channel coupling to the shear Alfven wave Identify the polarization field is generated to close the Hall current Our theory separates the Cowling channel into primary and secondary components ©2013. American Geophysical Union. All Rights Reserved.

    DOI: 10.1002/jgra.50514

  • The relation between amplitudes of a global-mode Pc 5 pulsations and geosynchronous electron fluxes

    #Magdi E Yousif Suliman, @Akimasa Yoshikawa, @K. Yumoto, @Hideaki Kawano, @Teiji Uozumi, @S. Abe, @M. G. Cardinal, Paolo Palangio, Lynn Kaisan

    2013 3rd IEEE International Conference on Space Science and Communication, IconSpace 2013 International Conference on Space Science and Communication, IconSpace   150 - 155   2013.7

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    Associative relationship between magnetospheric ULF waves in the Pc 5 range (1.7-6.7 mHz) and high energetic particles on the geosynchronous orbit has been investigated in detail in past studies. In particular, there has been interest in the efficiency of global Pc 5 waves, i.e., those having small m-numbers, in accelerating particles [1]. In this paper we investigated this feature by using energetic electron fluxes at geosynchronous orbits, and by using low-latitude global-mode Pc 5 pulsations: We used superposed epoch analyses to show correlations.

    DOI: 10.1109/IconSpace.2013.6599453

  • Coupling of electrons and inertial Alfven waves in the topside ionosphere Reviewed

    Run Shi, Huixin Liu, A. Yoshikawa, Beichen Zhang, Binbin Ni

    Journal of Geophysical Research: Space Physics   118 ( 6 )   2903 - 2910   2013.6

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    A one-dimensional kinetic model is constructed to simulate the electron acceleration by inertial Alfven waves. The electrons are divided into cold and hot electrons and treated separately. Cold components are described by the fluid equation and hot ones by the Vlasov equation, both carrying field-aligned currents. Intense variation of Alfven speed has been introduced by inclusion of cold electrons. The model results show that the exponential decrease of the plasma density plays a key role, which leads to the sharp gradient of both Alfven velocity and electron inertial length. When Alfven waves encounter this sharp gradient at lower altitudes, the electrons accelerated by the waves become super-Alfvenic, and the width of burst structures becomes much wider than the electron inertial length. Consequently, the background electrons carry the oppositely field-aligned current due to plasma oscillation. It is demonstrated that the current carried by the electrons exceeding the wavefront is balanced by the reverse current carried by background electrons. This mechanism can be used to reasonably explain observations of the electron bursts accompanied by little net field-aligned current. Furthermore, our simulation indicates another type of Alfven wave reflection due to mirror force and wave-particle interaction. Key Points Kinetic model which separates the electrons into cold and hot parts Explain the electron bursts accompanied by little net field-aligned current Another type of Alfven wave reflection due to wave-particle interaction ©2013. American Geophysical Union. All Rights Reserved.

    DOI: 10.1002/jgra.50355

  • Coupling of electrons and inertial Alfven waves in the topside ionosphere Reviewed

    Run Shi, Huixin Liu, A. Yoshikawa, Beichen Zhang, Binbin Ni

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   118 ( 6 )   2903 - 2910   2013.6

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    A one-dimensional kinetic model is constructed to simulate the electron acceleration by inertial Alfven waves. The electrons are divided into cold and hot electrons and treated separately. Cold components are described by the fluid equation and hot ones by the Vlasov equation, both carrying field-aligned currents. Intense variation of Alfven speed has been introduced by inclusion of cold electrons. The model results show that the exponential decrease of the plasma density plays a key role, which leads to the sharp gradient of both Alfven velocity and electron inertial length. When Alfven waves encounter this sharp gradient at lower altitudes, the electrons accelerated by the waves become super-Alfvenic, and the width of burst structures becomes much wider than the electron inertial length. Consequently, the background electrons carry the oppositely field-aligned current due to plasma oscillation. It is demonstrated that the current carried by the electrons exceeding the wavefront is balanced by the reverse current carried by background electrons. This mechanism can be used to reasonably explain observations of the electron bursts accompanied by little net field-aligned current. Furthermore, our simulation indicates another type of Alfven wave reflection due to mirror force and wave-particle interaction.

    DOI: 10.1002/jgra.50355

  • 惑星間磁場Bzの階段状変化に対する昼間側赤道ジェット電流の反応

    OHTANI Shinichi, UOZUMI Teiji, KAWANO Hideaki, YOSHIKAWA Akimasa, YUMOTO Kiyohumi, KIYOHUMI Yumoto

    地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM)   118 ( 6 )   3637 - 3646   2013.6

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    The response of the dayside equatorial electrojet to step-like changes of IMF B<inf>Z</inf>
    The equatorial electrojet (EEJ) is driven by zonal electric fields, which are known to be well correlated with the interplanetary electric field and therefore with the interplanetary magnetic field (IMF) BZ component. In the present study, we investigate how the equatorial H magnetic component, and therefore the EEJ, responds to step-like changes of IMF BZ. The reduction of southward IMF BZ (northward turning) and that of northward IMF BZ (southward turning) are examined separately. The result shows that for the northward turnings, the EEJ immediately starts to weaken with the accuracy of the estimates of the travel times of the IMF changes. The time constant of the response is much longer, and the equatorial H component decreases continuously by 40 nT for 30 min after the northward turnings. In contrast, the response of the EEJ to the southward turnings is far less clear in both magnitude and timing, and it does not depend on whether or not IMF BZ actually becomes southward. The difference in the EEJ response to the northward and southward turnings reflects at least partially the fact that the magnetosphere-ionosphere system is more sensitive to IMF B Z when IMF is southward than northward. It is suggested that the electric field penetrates from the polar region to the dip equator through a global current system that connects the auroral electrojets and the EEJ, and the ionospheric conductance in the polar region may play an important role in the formation of such a current system. Key Points EEJ starts to weaken within 1 min from the arrival of northward IMF turnings. The time constant of EEJ response to northward turnings is ~30 minutes. The response of EEJ to southward turnings is not clear in magnitude or timing. ©2013. American Geophysical Union. All Rights Reserved.

    DOI: 10.1002/jgra.50318

  • General solution for calculating polarization electric fields in the auroral ionosphere and application examples Reviewed

    O. Amm, R. Fujii, H. Vanhamäki, A. Yoshikawa, A. Ieda

    Journal of Geophysical Research: Space Physics   118 ( 5 )   2428 - 2437   2013.5

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    We devise an approach to calculate the polarization electric field in the ionosphere, when the ionospheric conductances, the primary (modeled) or the total (measured) electric field, and the Cowling efficiency are given. In contrast to previous studies, our approach is a general solution which is not limited to specific geometrical setups, and all parameters may have any kind of spatial dependence. The solution technique is based on spherical elementary current (vector) systems (SECS). This way, we avoid the need to specify explicit boundary conditions for the searched polarization electric field of its potential which would be required if the problem was solved in a differential equation approach. Instead, we solve an algebraic matrix equation, and the implicit boundary condition that the divergence of the polarization electric field vanishes outside our analysis area is sufficient. In order to illustrate our theory, we then apply it to two simple models of auroral electrodynamic situations, the first being a mesoscale strong conductance enhancement in the early morning sector within a relatively weak southward primary electric field, and a morning sector auroral arc with only a weak conductance enhancement, but a large southward primary electric field at the poleward flank of the arc. While the significance of the polarization electric field for maximum Cowling efficiency is large for the first case, it is rather minor for the second one. Both models show that the polarization electric field effect may not only change the magnitude of the current systems but also their overall geometry. Furthermore, the polarization electric field may extend into regions where the primary electric field is small, thus even dominating the total electric field in these regions. For the first model case, the total Joule heating integrated over the analysis area decreases by a factor of about 4 for maximum Cowling efficiency as compared to the case of vanishing Cowling efficiency. Furthermore, for this case the resulting total electric field structurally shows a strong resemblance to that frequently observed during auroral omega band events. ©2013. American Geophysical Union. All Rights Reserved.

    DOI: 10.1002/jgra.50254

  • Resonant Cavities and Waveguides in the Ionosphere and Atmosphere

    R. L. Lysak, A. Yoshikawa

    Magnetospheric ULF Waves: Synthesis and New Directions   169   289 - 306   2013.3

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    The strong inhomogeneities in plasma parameters in the ionosphere and adjacent regions can trap waves in the upper end of the ULF range (Pc1/Pi1). The topside ionosphere is characterized by a rapidly increasing Alfvén speed with a scale height on the order of 1000 km. Shear-mode Alfvén waves in this region can be partially trapped at frequencies in the 0.1-1.0 Hz range. The same structure can trap fast-mode compressional waves in this frequency band. Since these waves can propagate across magnetic field lines, this structure constitutes a waveguide in which energy can propagate at speeds comparable to the Alfvén speed, typically on the order of 1000 km/s. Hall effects in the ionosphere couple these two wave modes, so that the introduction of a field-aligned current by means of a shearmode Alfvén wave can excite compressional waves that can propagate in the waveguide. In the limit of infinite ionospheric conductivity, these waves are isolated from the atmospheric fields; however, for finite conductivity, ionospheric and atmospheric waves are coupled. Transverse magnetic modes in the atmosphere can propagate at ULF frequencies and form global Schumann resonances with the fundamental at 8 Hz. It has been suggested that signals that propagate at the speed of light through this atmospheric waveguide can rapidly transmit signals from the polar region to lower latitudes during sudden storm commencements.

    DOI: 10.1029/169GM19

  • Poleward moving auroral arcs observed at the South Pole Station and the interpretation by field line resonances Reviewed

    Y. -M. Tanaka, Y. Ebihara, S. Saita, A. Yoshikawa, Y. Obana, A. T. Weatherwax

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   117 ( A9 )   2012.9

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    We investigate the characteristics of poleward moving auroral arcs (PMAAs) observed with the all-sky monochromatic imager at the South Pole Station (74.3 degrees CGLAT) in the interval 08:00-11:00 MLT on July 8, 2004. During this period, Pc 5 geomagnetic pulsations are also observed as well as quasi-stationary auroral patches (QSAPs), which keep their forms, luminosities, and locations for up to several hours. It is demonstrated that the PMAAs, Pc 5 pulsations in the north-south component, and oscillations in the drift of the QSAPs in the east-west direction have similar dominant periods and are well correlated with each other. The oscillatory ionospheric plasma drifts accompanying the PMAAs are extracted from the horizontal motion of the QSAPs and are found to propagate poleward with the PMAAs. The phase relations of the PMAAs and Pc 5 pulsations in the northward component with respect to the westward drift velocity of the QSAPs are close to anti-phase and in-phase, respectively. To examine whether these phenomena can be interpreted by field line resonances (FLRs), we perform a numerical simulation using a horizontally two-dimensional model that consists of the auroral acceleration region and the ionosphere with time-evolution conductivity. The results indicate that the observed data can be well explained by the FLR model with realistic physical parameters, except for the phase relation of the PMAAs with respect to the Pc 5 pulsations and the QSAPs.

    DOI: 10.1029/2012JA017899

  • Poleward moving auroral arcs observed at the South Pole Station and the interpretation by field line resonances Reviewed International journal

    Y. M. Tanaka, Y. Ebihara, S. Saita, @Akimasa Yoshikawa, Y. Obana, A. T. Weatherwax

    Journal of Geophysical Research   117 ( 9 )   2012.1

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    We investigate the characteristics of poleward moving auroral arcs (PMAAs) observed with the all-sky monochromatic imager at the South Pole Station (74.3°CGLAT) in the interval 08:00-11:00 MLT on July 8, 2004. During this period, Pc 5 geomagnetic pulsations are also observed as well as quasi-stationary auroral patches (QSAPs), which keep their forms, luminosities, and locations for up to several hours. It is demonstrated that the PMAAs, Pc 5 pulsations in the north-south component, and oscillations in the drift of the QSAPs in the east-west direction have similar dominant periods and are well correlated with each other. The oscillatory ionospheric plasma drifts accompanying the PMAAs are extracted from the horizontal motion of the QSAPs and are found to propagate poleward with the PMAAs. The phase relations of the PMAAs and Pc 5 pulsations in the northward component with respect to the westward drift velocity of the QSAPs are close to anti-phase and in-phase, respectively. To examine whether these phenomena can be interpreted by field line resonances (FLRs), we perform a numerical simulation using a horizontally two-dimensional model that consists of the auroral acceleration region and the ionosphere with time-evolution conductivity. The results indicate that the observed data can be well explained by the FLR model with realistic physical parameters, except for the phase relation of the PMAAs with respect to the Pc 5 pulsations and the QSAPs.

    DOI: 10.1029/2012JA017899

  • A study of latitudinal dependence of Pc 3-4 amplitudes at 96° magnetic meridian stations in Africa Reviewed

    Takla EM, Yumoto K, Cardinal MG, Abe S, Fujimoto A, Ikeda A, Tokunaga T, Yamazaki Y, Uo-zumi T, Mahrous A, Ghamry E, Mengistu G, Afullo T, Macamo JA, Joao L, Mweene H, Mwiinga N, Uiso C, Baki P, Kianji G, Badi K, Sutcliffe P, Palangio P. Terumasa Tokunaga, Daisuke Ikeda, Kazuyuki Nakamura, Tomoyuki Higuchi, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto, Akira Morioka, Kiyohumi Yumoto

    Sun and Geosphere   6 ( 2 )   65 - 70   2011.12

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    A study of latitudinal dependence of Pc 3-4 amplitudes at 96° magnetic meridian stations in Africa

  • Pi 2 waves simultaneously observed by Cluster and CPMN ground-based magnetometers near the plasmapause Reviewed International journal

    @Hideaki Kawano, S. Ohtani, @T. Uozumi, #T. Tokunaga, @Akimasa Yoshikawa, @K. Yumoto, E. A. Lucek, M. André

    Annales Geophysicae   29 ( 9 )   1663 - 1672   2011.10

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    We have analyzed an event on 14 February 2003 in which Cluster satellites and the CPMN ground magnetometer chain made simultaneous observations of a Pi 2 pulsation along the same meridian. Three of the four Cluster satellites were located outside the plasmasphere, while the other one was located within the plasmasphere. By combining the multipoint observations in space and the multipoint observations on the ground, we have obtained a detailed L-profile of the Pi 2 signatures, which has not been done in the past. In addition, we have used a method called Independent Component Analysis (ICA) to separate out other superposed waves with similar spectral components. The result shows that the wave phase of the Pi 2 was the same up to L &sim; 3.9 (corresponding to the plasmasphere), became earlier up to L &sim; 4.1 (corresponding to the plasmapause boundary layer), and showed a delaying tendency up to L &sim; 5.9 (corresponding to the plasmatrough). This systematic phase pattern, obtained for the first time by a combination of a ground magnetometer chain and multisatellites along a magnetic meridian with the aid of ICA, supports the interpretation that a Pi 2 signal propagated from a farther source and reached the plasmasphere.

    DOI: 10.5194/angeo-29-1663-2011

  • 1996~2007年にCPMNデータから導いた静穏な日地磁気場変動に関する経験モデル Reviewed

    YAMAZAKI Yosuke, YUMOTO Kiyohumi, UOZUMI Teiji, YOSHIKAWA Akimasa, KAKINAMI Yoshihiro, KIYOHUMI Yumoto

    地球電磁気・地球惑星圏学会総会及び講演会予稿集(CD-ROM)   116 ( A10 )   2011.10

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    An empirical model of the quiet daily geomagnetic field variation
    An empirical model of the quiet daily geomagnetic field variation has been constructed based on geomagnetic data obtained from 21 stations along the 210 Magnetic Meridian of the Circum-pan Pacific Magnetometer Network (CPMN) from 1996 to 2007. Using the least squares fitting method for geomagnetically quiet days (Kp <= 2+), the quiet daily geomagnetic field variation at each station was described as a function of solar activity SA, day of year DOY, lunar age LA, and local time LT. After interpolation in latitude, the model can describe solar-activity dependence and seasonal dependence of solar quiet daily variations (S) and lunar quiet daily variations (L). We performed a spherical harmonic analysis (SHA) on these S and L variations to examine average characteristics of the equivalent external current systems. We found three particularly noteworthy results. First, the total current intensity of the S current system is largely controlled by solar activity while its focus position is not significantly affected by solar activity. Second, we found that seasonal variations of the S current intensity exhibit north-south asymmetry; the current intensity of the northern vortex shows a prominent annual variation while the southern vortex shows a clear semi-annual variation as well as annual variation. Thirdly, we found that the total intensity of the L current system changes depending on solar activity and season; seasonal variations of the L current intensity show an enhancement during the December solstice, independent of the level of solar activity.

    DOI: 10.1029/2011JA016487

  • A self-consistent synthesis description of magnetosphere-ionosphere coupling and scale-dependent auroral process using shear Alfven wave Reviewed

    A. Yoshikawa, O. Amm, H. Vanhamaeki, R. Fujii

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   116 ( A8 )   2011.8

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    In order to correctly describe the dynamical behavior of the magnetosphere-ionosphere (MI) coupling system and the scale-dependent auroral process, we develop a synthesis formulation that combines the process of (1) the inverse Walen separation of MHD disturbance into parallel- and antiparallel-propagating shear Alfven wave to the ambient magnetic field, (2) the shear Alfven wave reflection process including (3) the scale-dependent electrostatic coupling process through the linearized Knight relation, (4) two-layer ionosphere model, and (5) dynamic conductance variations. A novel procedure that applies the inverse Walen relation to the incompressional MHD disturbances at the inner boundary of the MHD region enables to extract the component of the shear Alfven wave incident to the ionosphere. The extracted incident electric field supplies an electromotive force for the generation of the MI coupling system, and the reflected electric field is generated such that it totally satisfies the synthesis MI-coupling equation. A three-dimensional ionospheric current system is represented by a two-layer model in which the Pedersen and the Hall current are confined in the separated layers, which are connected by field-aligned currents driven by the linear current-voltage relation between two layers. Hence, our scheme possibly reproduces two types of the scale-dependent MI-decoupling process of the perpendicular potential structure: due to the parallel potential drop at the auroral acceleration region and the other due to the parallel potential differences inside the ionosphere. Our newly formulation may be well suited for description of scale-dependent auroral process and mesoscale ionospheric electrodynamics interlocked with the dynamical development of magnetospheric processes.

    DOI: 10.1029/2011JA016460

  • 変化点検出を応用した時系列データからの突発現象の前兆検出アルゴリズム

    徳永 旭将, 池田 大輔, 中村 和幸, 樋口 知之, 吉川 顕正, 魚住 禎司, 藤本 晶子, 森岡 昭, 湯元 清文

    情報処理学会論文誌数理モデル化と応用(TOM)   4 ( 3 )   14 - 34   2011.7

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    An Algorithm for Detecting Precursory Events from Time Series Data
    一般に,前兆現象は突発現象にそのものに比べて非常に目立ちにくく,その開始時刻は曖昧である.従来よく用いられてきた変化点検出法を適用した場合,このような微小で緩慢な変化は見逃されやすい.Tokunagaら(2010)では,Ideら(2005)の提案した特異スペクトル分析を応用した変化点検出法(SST)を,多次元データを用いたアルゴリズム(MSST)へと拡張することで,鋭敏に前兆現象の開始時刻を推定できることを示した.MSSTは,緩慢な変化も検出できる鋭敏な手法であるが,実データへの適用では誤検出が問題になる.本稿では,突発現象の大まかな開始時刻をあらかじめ検出し,さらに検出された時刻の前後で前兆現象の開始時刻と終了時刻を個別に探索することで,前兆現象を鋭敏に検出でき,かつMSST単体よりも誤検出を劇的に減少させることができることを示す.In general, precursory events are observed as minute and less-visible fluctuations preceding an onset of massive fluctuations of extraordinary phenomena. Hence, existing change-point detection methods most likely overlook precursory events. Tokunaga, et al. (2010) extended the method for detecting the change-points, Singular Spectrum Transformation (SST) proposed by Ide, et al. (2005), to the multivariable SST (MSST). Although MSST can detect minute changes, we have to reduce false positives because real world data includes non-stationary trends and measurement noise. In this paper, we propose the algorithm to detect precursory events in an off-line manner. Our algorithm consists of three kinds of change-point detection methods. We show that the number of false positive reduce drastically by combining three different types of change-point detection methods.

  • Onset time determination of precursory events in time series data by an extension of Singular Spectrum Transformation Reviewed

    #Terumasa Tokunaga,@ Daisuke Ikeda, Kazuyuki Nakamura, Tomoyuki Higuchi, @Akimasa Yoshikawa, @Teiji Uozumi, #Akiko Fujimoto, Akira Morioka, @Kiyohumi Yumoto

    International Journal of Circuits, Systems and Signal Processing   5 ( 1 )   46 - 60   2011.6

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    To predict an occurrence of extraordinary phenomena, such as earthquakes, failures of engineering systems and financial market crushes, it is important to identify precursory events in time series. However, existing methods are limited in their applicability for real world precursor detections. Recently, Ide and Inoue [1] have developed an SSA-based change-point detection method, called singular spectrum transformation (SST). SST is suitable for detecting various types of change-points, but real world precursor detections can be far more difficult than expected. In general, precursory events are observed as minute and less-visible fluctuations preceding an onset of massive fluctuations of extraordinary phenomena and therefore they are easily over-looked. To overcome this point, we extend the conventional SST to the multivariable SST. The originality of our strategy is in focusing on synchronism detections of precursory events in multiple sequences of univariate time series. We performed some experiments by using artificial data and showed the superiority of multivariable SST in detecting onset of precursory events. Furthermore, the superiority is also shown statistically in determining the onset of precursory events by using real world time series.

  • AKR modulation and global Pi2 oscillation Reviewed

    Teiji Uozumi, K. Yumoto, T. Tokunaga, S. I. Solovyev, B. M. Shevtsov, R. Marshall, K. Liou, S. Ohtani, S. Abe, A. Ikeda, K. Kitamura, A. Yoshikawa, H. Kawano, M. Itonaga

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   116 ( A6 )   2011.6

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    In this report we present a temporal relationship between ground Pi2 and auroral kilometric radiation (AKR). We analyzed six isolated substorm events, which were observed by the MAGDAS/CPMN ground magnetometer network and the plasma wave instrument onboard the Polar satellite. We found that the time derivative of the height-integrated AKR power and the ground Pi2 D component had the same periodicity and that the two were synchronized with each other. When the D component fluctuated with the same (opposite) polarity as the magnetic bay variation, the AKR power tended to increase (decrease) during the corresponding interval. An isolated substorm event (AE similar to 40 nT), which occurred around 10: 19 UT on 24 January1997, was selected for a detailed study. The behavior of the Pi2 event can be interpreted by the substorm current wedge (SCW) and Pi2 propagation models. It is confirmed that the midlatitude and high-latitude D component oscillations can be treated as a proxy of the SCW oscillations, whereas the H component oscillations exhibited some phase shifts by the propagation delay of the Pi2 waves. That is, the temporal relation between the time derivative of the AKR power and the ground Pi2 suggests that the height-integrated AKR power was modulated coherently with the SCW oscillations.

    DOI: 10.1029/2010JA016042

  • AKR modulation and global Pi2 oscillation Reviewed

    @Teiji Uozumi, @K. Yumoto, #T. Tokunaga, S. I. Solovyev, B. M. Shevtsov, R. Marshall, K. Liou, S. Ohtani, @S. Abe, #A. Ikeda, @K. Kitamura, @Akimasa Yoshikawa, @Hideaki Kawano, M. Itonaga

    Journal of Geophysical Research   116 ( 6 )   2011.1

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    In this report we present a temporal relationship between ground Pi2 and auroral kilometric radiation (AKR). We analyzed six isolated substorm events, which were observed by the MAGDAS/CPMN ground magnetometer network and the plasma wave instrument onboard the Polar satellite. We found that the time derivative of the height-integrated AKR power and the ground Pi2 D component had the same periodicity and that the two were synchronized with each other. When the D component fluctuated with the same (opposite) polarity as the magnetic bay variation, the AKR power tended to increase (decrease) during the corresponding interval. An isolated substorm event (AE ∼ 40 nT), which occurred around 10:19 UT on 24 January1997, was selected for a detailed study. The behavior of the Pi2 event can be interpreted by the substorm current wedge (SCW) and Pi2 propagation models. It is confirmed that the midlatitude and high-latitude D component oscillations can be treated as a proxy of the SCW oscillations, whereas the H component oscillations exhibited some phase shifts by the propagation delay of the Pi2 waves. That is, the temporal relation between the time derivative of the AKR power and the ground Pi2 suggests that the height-integrated AKR power was modulated coherently with the SCW oscillations.

    DOI: 10.1029/2010JA016042

  • Detecting precursory events in time series data by an extension of singular spectrum transformation

    #Terumasa Tokunaga, @Daisuke Ikeda, Kazuyuki Nakamura, Tomoyuki Higuchi, @Akimasa Yoshikawa, @eiji Uozumi, #Akiko Fujimoto, Akira Morioka, @Kiyofumi Yumoto

    10th WSEAS International Conference on Applied Computer Science, ACS'10 Selected Topics in Applied Computer Science - 10th WSEAS International Conference on Applied Computer Science, ACS'10   366 - 374   2010.12

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    To predict an occurrence of extraordinary phenomena, such as earthquakes, failures of engineering system and financial market crushes, it is important to identify precursory events in time series. However, existing methods are limited in their applicability for real world precursor detections. Recently, Ide and Inoue [1] have developed an SSA-based change-point detection method, called singular spectrum transformation (SST). In this paper, we extend the SST so that it is applicable for real world precursor detections, focusing on the wide applicability of the conventional SST. Although the SST is suitable for detecting various types of change-points, detecting precursors can be far more difficult than expected because, in general, real world time series contains measurement noise and non-stationary trends. Furthermore, precursory events are usually observed as minute and less-visible fluctuations preceding an onset of massive fluctuations of extraordinary phenomena and therefore they are easily over-looked. To overcome this, we extend the conventional SST to the multivariable SST, focusing on the synchronism detection of precursory events in multiple sequences of univariate time series. First, we would like to define the problem setting of real world precursory detections and consider its difficulties. Second, the multivariable SST is introduced. Third, we apply SST to geomagnetic time series data and show the multivariable SST is more suitable than the conventional SST for real world precursor detections. Finally, we show further experimental results using artificial data to evaluate the reliability of SST-based precursor detections.

  • A feasibility study of postoperative chemotherapy with S-1 and cisplatin (CDDP) for gastric carcinoma (CCOG0703)

    Yasuhiro Kodera, Akiharu Ishiyama, Takaki Yoshikawa, Takashi Kinoshita, Seiji Ito, Hiroyuki Yokoyama, Yoshinari Mochizuki, Hiroaki Ito, Akira Tsuburaya, Junichi Sakamoto, Akimasa Nakao

    Gastric Cancer   13 ( 3 )   197 - 203   2010.8

  • Phase Relation between Pi 2-associated Ionospheric Doppler Velocity and Magnetic Pulsation at Mid-Latitude MAGDAS Station Invited Reviewed International journal

    #Ikeda A., @K. Yumoto, @M. Shinohara, K. Nozaki, @A. Yoshikawa, A. Shinbori

    J. Geophys. Res.   115 ( A02215 )   2010.4

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    DOI: 10.1029/2009JA014397

  • Alfvenic‐coupling algorithm for global and dynamical magnetosphere‐ionosphere coupled system Reviewed

    Akimasa Yoshikawa, Hiroyuki Nakata, Aoi Nakamizo, Teiji Uozumi, Masahiro Itonaga, Shigeru Fujita, Kiyohumi Yumoto, Takashi Tanaka

    Journal of Geophysical Research: Space Physics   115 ( A4 )   2010.4

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    Alfvenic-coupling algorithm for global and dynamical magnetosphere-ionosphere coupled system
    This study proposes a new formula that describes a dynamical magnetosphere-ionosphere (MI) coupling system through the field-aligned current (FAC) closure and electrostatic potential connectivity. In the past, MI coupling processes were described as either "inductive'' or "static.'' The inductive coupling scheme is based on the reflection of MHD waves at the ionosphere, whereas in the static coupling scheme the electrostatic potential is determined through the FAC closure. In contrast, in our new formulation these two schemes are combined by the "Alfvenic-coupling'' algorithm. The concept of the Alfvenic coupling is as follows. When a distribution of ionospheric current is changed from the background condition through the mapping of magnetospheric disturbances and/or by the change of ionospheric conductivity, an ionospheric reflection electric filed is instantaneously generated to satisfy the current continuity condition. The electrostatic potential of this reflection field also feeds back to the magnetosphere and excites shear Alfvenic disturbances in the magnetosphere. Therefore, the current continuity condition has to include the FAC of Alfvenic disturbances. In this sense, the reflection potential is not only a modification of the ionospheric potential but also a source of inductive Alfvenic disturbances. Quantitative estimation of feedback components to the magnetosphere reveals that our new formulation is more suitable to global MI simulations than the static MI coupling, which has been the only scheme used in the past.

    DOI: 10.1029/2009JA014924

  • Phase relation between Pi2‐associated ionospheric Doppler velocity and magnetic pulsations observed at a midlatitude MAGDAS station Reviewed

    Akihiro Ikeda, Kiyohumi Yumoto, Teiji Uozumi, Manabu Shinohara, Kenro Nozaki, Akimasa Yoshikawa, V. V. Bychkov, B. M. Shevtsov

    Journal of Geophysical Research: Space Physics   115 ( A2 )   2010.2

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    Phase relation between Pi2-associated ionospheric Doppler velocity and magnetic pulsations observed at a midlatitude MAGDAS station
    We examined the correlation between nighttime Pi2 pulsations detected simultaneously by a frequency modulated continuous wave (FM-CW) (HF) radar and by a ground magnetometer, both located at a midlatitude (L = 2.05) Magnetic Data Acquisition System station. Eighty-three Pi2 events were observed during the 43 day period from 23 September 2006 to 4 November 2006. The variations of the ground magnetic H component and ionospheric Doppler velocity (V*) exhibited high coherence for 80&#37; of the 83 Pi2 events, for about a half of which the H and V* variations have the same dominant frequency. For such events, V* led H by 90 degrees in phase, in the midnight sector of 2230-0300 LT. The average Ey (east-west electric field) amplitude derived from V* is 0.27 mV/m. The 90 degrees phase delay was not found for the five events that were observed near dusk and dawn. The phase relation of H and V* for Pi2s in the midnight sector may be explained in terms of the radial standing structure of compressional waves, i.e., cavity mode oscillation.

    DOI: 10.1029/2009JA014397

  • Ionospheric observation using FM-CW radar array Reviewed

    A. Ikeda, A. Yoshikawa, M. G. Cardinal, K. Yumoto, M. Shinohara, K. Nozaki, B. M. Shevtsov, V. V. Bychkov, Q. M. Sugon, D. McNamara

    Advances in Geosciences: Volume 21: Solar Terrestrial (ST)   379 - 392   2010.1

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    In order to understand the electro-magnetic phenomenona in space, the Space Environment Research Center (SERC) of Kyushu University is deploying the MAGnetic Data Acquisition System of the Circum-pan Pacific Magnetometer Network (MAGDAS/CPMN). In this network, we also installed FM-CW (Frequency Modulated Continuous Wave) radars at Paratunka, Russia (PTK: Magnetic Latitude = 45.8°, Magnetic Longitude = 221.6°), Sasaguri, Japan (SAS: M. Lat. = 23.2°, M. Lon. = 199.6°), and Manila, Philippines (MNL: M. Lat. = 4.19°, M. Lon. = 192.4°) to detect the ionospheric electric field variations. The FM-CW radar is a kind of HF (High Frequency) radar that can measure the ionospheric Doppler velocity, from which we can calculate the ionospheric electric fields. In the present paper we will introduce our FM-CW radar array observations and its preliminary scientific results. The results are as follows: (1) At the time of SC, dusk-to-dawn and subsequent dawn-to-dusk electric field penetrate into the low-latitude ionosphere. (2) Pi 2-associated ionospheric electric field at L = 2.05 is a manifestation of the plasmaspheric cavity mode. (3) Ground Pc 5 pulsation seems to be driven by ionospheric electric field at low and equatorial region.

    DOI: 10.1142/9789812838209_0027

  • Magnetic field investigation of Mercury's magnetosphere and the inner heliosphere by MMO/MGF Reviewed

    Wolfgang Baumjohann, Ayako Matsuoka, Werner Magnes, Karl Heinz Glassmeier, Rumi Nakamura, Helfried Biernat, Magda Delva, Konrad Schwingenschuh, Tielong Zhang, Hans Ulrich Auster, Karl Heinz Fornacon, Ingo Richter, André Balogh, Peter Cargill, Chris Carr, Michele Dougherty, Timothy S. Horbury, Elizabeth A. Lucek, Fumio Tohyama, Takao Takahashi, Makoto Tanaka, Tsugunobu Nagai, Hideo Tsunakawa, Masaki Matsushima, @Hideaki Kawano, @Akimasa Yoshikawa, Hidetoshi Shibuya, Tomoko Nakagawa, Masahiro Hoshino, Yoshimasa Tanaka, Ryuho Kataoka, Brian J. Anderson, Christopher T. Russell, Uwe Motschmann, Manabu Shinohara

    Planetary and Space Science   58 ( 1-2 )   279 - 286   2010.1

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    The Mercury magnetospheric orbiter (MMO) of the Japanese-European BepiColombo mission carries a dual-sensor magnetometer, MMO/MGF. The sensors are of the classical fluxgate type mounted on a boom. For redundancy, each sensor carries its own electronics and is connected to a different data processing unit. MMO/MGF can sample the magnetic field at a rate of up to 128 Hz. The resulting comparatively high time resolution of the magnetic field measurements, i.e., down to 8 ms, will be necessary when studying the dynamics of and processes within the Hermean magnetosphere, since the Mariner 10 observations have shown that their typical time scales are much shorter than in the Earth's magnetosphere, by about a factor of 30. The high time resolution will also be very useful for studying the evolution of the still young solar wind plasma as well as interplanetary shocks at 0.3-0.46 AU. Of course, MMO/MGF is also well-prepared to assist the sister magnetometer aboard the Mercury planetary orbiter, MPO/MAG, in measuring Mercury's intrinsic magnetic field, in particular by helping to distinguish between temporal fluctuations and spatial variations.

    DOI: 10.1016/j.pss.2008.05.019

  • Equivalent current systems for the annual and semiannual S<inf>q</inf> variations observed along the 210°MM CPMN stations Reviewed

    Y. Yamazaki, K. Yumoto, T. Uozumi, A. Yoshikawa, M. G. Cardinal

    Journal of Geophysical Research: Space Physics   114 ( 12 )   2009.12

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    We analyzed ground magnetometer data for the 10 International Quiet Days during 1996-2007. The data were obtained from 19 stations along 210°magnetic meridian (MM) of the Circum-pan Pacific Magnetometer Network (CPMN) covering both the Northern Hemisphere and Southern Hemisphere. From the daily variations of the geomagnetic field, we deduced the latitude-local time (LAT-LT) diagram of the equivalent Sq current system, which can be regarded as the superposition of the following three current systems: Sqo, Sq 1, and Sq2. The Sq0, Sq1, and Sq2 current systems are equivalent current systems for the yearly average, annual variation, and semiannual variation of the Sq field, respectively. We have examined temporal and spatial features of these current systems. The principal features are as follows: (1) The total current intensities of the Sq1 and Sq2 current systems are about 35&#37; and 15&#37; of that of the Sq0 current system, respectively. (2) The Sq0 and Sq2 current systems have a dayside vortex in each hemisphere, while the Sq1 current system has a single vortex centered at the equatorial region in the morning sector (∼1000 LT). Copyright 2009 by the American Geophysical Union.

    DOI: 10.1029/2009JA014638

  • Equivalent current systems for the annual and semiannual Sq variations observed along the 210° MM CPMN stations Reviewed

    Yamazaki Y, Yumoto K, Uozumi T, Yoshikawa A, Cardinal MG

    Journal of Geophysical Research: Space Physics   114 ( A12 )   2009.12

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    Equivalent current systems for the annual and semiannual S-q variations observed along the 210 degrees MM CPMN stations
    We analyzed ground magnetometer data for the 10 International Quiet Days during 1996-2007. The data were obtained from 19 stations along 210 degrees magnetic meridian (MM) of the Circum-pan Pacific Magnetometer Network (CPMN) covering both the Northern Hemisphere and Southern Hemisphere. From the daily variations of the geomagnetic field, we deduced the latitude-local time (LAT-LT) diagram of the equivalent S-q current system, which can be regarded as the superposition of the following three current systems: Sq(0), Sq(1), and Sq(2). The Sq(0), Sq(1), and Sq(2) current systems are equivalent current systems for the yearly average, annual variation, and semiannual variation of the S-q field, respectively. We have examined temporal and spatial features of these current systems. The principal features are as follows: (1) The total current intensities of the Sq(1) and Sq(2) current systems are about 35&#37; and 15&#37; of that of the Sq(0) current system, respectively. (2) The Sq(0) and Sq(2) current systems have a dayside vortex in each hemisphere, while the Sq(1) current system has a single vortex centered at the equatorial region in the morning sector (similar to 1000 LT).

    DOI: 10.1029/2009JA014638

  • Equivalent current systems for the annual and semiannual S<inf>q</inf> variations observed along the 210°MM CPMN stations

    Y. Yamazaki, K. Yumoto, K. Yumoto, T. Uozumi, A. Yoshikawa, A. Yoshikawa, M. G. Cardinal

    Journal of Geophysical Research: Space Physics   114 ( 12 )   2009.12

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    Equivalent current systems for the annual and semiannual S-q variations observed along the 210 degrees MM CPMN stations
    We analyzed ground magnetometer data for the 10 International Quiet Days during 1996-2007. The data were obtained from 19 stations along 210 degrees magnetic meridian (MM) of the Circum-pan Pacific Magnetometer Network (CPMN) covering both the Northern Hemisphere and Southern Hemisphere. From the daily variations of the geomagnetic field, we deduced the latitude-local time (LAT-LT) diagram of the equivalent S-q current system, which can be regarded as the superposition of the following three current systems: Sq(0), Sq(1), and Sq(2). The Sq(0), Sq(1), and Sq(2) current systems are equivalent current systems for the yearly average, annual variation, and semiannual variation of the S-q field, respectively. We have examined temporal and spatial features of these current systems. The principal features are as follows: (1) The total current intensities of the Sq(1) and Sq(2) current systems are about 35&#37; and 15&#37; of that of the Sq(0) current system, respectively. (2) The Sq(0) and Sq(2) current systems have a dayside vortex in each hemisphere, while the Sq(1) current system has a single vortex centered at the equatorial region in the morning sector (similar to 1000 LT).

    DOI: 10.1029/2009JA014638

  • Propagation characteristics of Pi 2 pulsations observed at high- And low-latitude MAGDAS/CPMN stations: A statistical study Reviewed

    Teiji Uozumi, S. Abe, K. Kitamura, T. Tokunaga, A. Yoshikawa, H. Kawano, R. Marshall, R. J. Morris, B. M. Shevtsov, S. I. Solovyev, D. J. McNamara, K. Liou, S. Ohtani, M. Itonaga, K. Yumoto

    Journal of Geophysical Research: Space Physics   114 ( 11 )   2009.11

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    The objective of this study is to understand better the propagation of Pi 2 waves in the nighttime region. We examined Pi 2 oscillations that showed high correlation between high- and low-latitude Magnetic Data Acquisition System/Circum Pan-Pacific Magnetometer Network stations (correlation coefficient: |γ| ≥ 0.75). For each horizontal component (H and D) we examined the magnetic local time (MLT) dependence of the delay time of high-latitude Pi 2 oscillations that corresponds to the highest correlation with the low-latitude Pi 2 oscillation. We found the delay time of the high-latitude H showed remarkable MLT dependence, especially in the premidnight sector: we found that in the premidnight sector the high-latitude H oscillation tends to delay from the low-latitude oscillation (<100 s). On the other hand, the delay time of the high-latitude D oscillation was not significant (∼±10 s) in the entire nighttime sector. We propose a Pi 2 propagation model to explain the observed delay time of high-correlation highlatitude H. The model quantitatively explains the trend of the event distribution. We also examined the spatial distribution of high-correlation Pi 2 events relative to the center of auroral breakups. It was found that the high-correlation Pi 2 events tend to occur away from the center of auroral breakups by more than 1.5 MLT. The present result suggests that the high-correlation H component Pi 2 oscillations at high latitude are a manifestation of forced Alfvén waves excited by fast magnetosonic waves. Copyright 2009 by the American Geophysical Union.

    DOI: 10.1029/2009JA014163

  • Propagation characteristics of Pi 2 pulsations observed at high- and low-latitude MAGDAS/CPMN stations: A statistical study Reviewed

    Teiji Uozumi, S. Abe, K. Kitamura, T. Tokunaga, A. Yoshikawa, H. Kawano, R. Marshall, R. J. Morris, B. M. Shevtsov, S. I. Solovyev, D. J. McNamara, K. Liou, S. Ohtani, M. Itonaga, K. Yumoto

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   114 ( A11 )   2009.11

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    The objective of this study is to understand better the propagation of Pi 2 waves in the nighttime region. We examined Pi 2 oscillations that showed high correlation between high- and low-latitude Magnetic Data Acquisition System/Circum Pan-Pacific Magnetometer Network stations (correlation coefficient: vertical bar gamma vertical bar >= 0.75). For each horizontal component (H and D) we examined the magnetic local time (MLT) dependence of the delay time of high-latitude Pi 2 oscillations that corresponds to the highest correlation with the low-latitude Pi 2 oscillation. We found the delay time of the high-latitude H showed remarkable MLT dependence, especially in the premidnight sector: we found that in the premidnight sector the high-latitude H oscillation tends to delay from the low-latitude oscillation (<100 s). On the other hand, the delay time of the high-latitude D oscillation was not significant (similar to +/- 10 s) in the entire nighttime sector. We propose a Pi 2 propagation model to explain the observed delay time of high-correlation high-latitude H. The model quantitatively explains the trend of the event distribution. We also examined the spatial distribution of high-correlation Pi 2 events relative to the center of auroral breakups. It was found that the high-correlation Pi 2 events tend to occur away from the center of auroral breakups by more than 1.5 MLT. The present result suggests that the high-correlation H component Pi 2 oscillations at high latitude are a manifestation of forced Alfven waves excited by fast magnetosonic waves.

    DOI: 10.1029/2009JA014163

  • Characteristics of counter-S<inf>q</inf> SFE (SFE) at the dip equator CPMN stations A05306 Reviewed

    Y. Yamazaki, K. Yumoto, A. Yoshikawa, S. Watari, H. Utada

    Journal of Geophysical Research: Space Physics   114 ( 5 )   2009.5

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    The solar flare effect (SFE) at dip equatorial latitudes sometimes shows the counter-Sq variation around local noon. In this paper, we refer to this type of SFE as SFE*. Observations obtained by the Circum-pan Pacific Magnetometer Network (CPMN) reveal some previously unknown characteristics of SFE*. Some of these features are the following: (1) the counter-Sq SFE variation is observed in limited longitude (local time) and latitude sectors (i.e., LT ≈ 1030-1300, DipLat. ≲, 1.5°) (2) outside this limited region, the amplitude of SFE(Z/) and preflare S q(H) have a linear relationship (3) SFE* is observed during the significant depression of the horizontal magnetic field at dip equatorial latitudes, which indicates the presence of westward electric fields whose origin remains to be understood. Copyright 2009 by the American Geophysical Union.

    DOI: 10.1029/2009JA014124

  • Characteristics of counter-S-q SFE (SFE*) at the dip equator CPMN stations Reviewed

    Y. Yamazaki, K. Yumoto, A. Yoshikawa, S. Watari, H. Utada

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   114 ( A5 )   2009.5

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    The solar flare effect (SFE) at dip equatorial latitudes sometimes shows the counter-S-q variation around local noon. In this paper, we refer to this type of SFE as SFE*. Observations obtained by the Circum-pan Pacific Magnetometer Network (CPMN) reveal some previously unknown characteristics of SFE*. Some of these features are the following: (1) the counter-S-q SFE variation is observed in limited longitude (local time) and latitude sectors (i.e., LT approximate to 1030-1300, vertical bar DipLat.vertical bar less than or similar to 1.5 degrees), (2) outside this limited region, the amplitude of SFE(H) and preflare S-q(H) have a linear relationship, and (3) SFE* is observed during the significant depression of the horizontal magnetic field at dip equatorial latitudes, which indicates the presence of westward electric fields whose origin remains to be understood.

    DOI: 10.1029/2009JA014124

  • Characteristics of counter-S-q SFE (SFE*) at the dip equator CPMN stations

    Y. Yamazaki, K. Yumoto, A. Yoshikawa, S. Watari, H. Utada

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   114 ( 5 )   2009.5

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    The solar flare effect (SFE) at dip equatorial latitudes sometimes shows the counter-S-q variation around local noon. In this paper, we refer to this type of SFE as SFE*. Observations obtained by the Circum-pan Pacific Magnetometer Network (CPMN) reveal some previously unknown characteristics of SFE*. Some of these features are the following: (1) the counter-S-q SFE variation is observed in limited longitude (local time) and latitude sectors (i.e., LT approximate to 1030-1300, vertical bar DipLat.vertical bar less than or similar to 1.5 degrees), (2) outside this limited region, the amplitude of SFE(H) and preflare S-q(H) have a linear relationship, and (3) SFE* is observed during the significant depression of the horizontal magnetic field at dip equatorial latitudes, which indicates the presence of westward electric fields whose origin remains to be understood.

    DOI: 10.1029/2009JA014124

  • SC-associated Ionospheric Electric Fields at Low Latitude:FM-CW Radar Observation Reviewed

    #Ikeda A., @K. Yumoto,@ M. Shinohara, K. Nozaki, @A. Yoshikawa and A. Shinbor

    Mem. Fac. Sci., Kyushu Univ., Ser. D, Earth and Planet. Sci.   2009.3

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  • Towards understanding the electrodynamics of the 3-dimensional high-latitude ionosphere: Present and future Reviewed

    O. Amm, A. Aruliah, S. C. Buchert, R. Fujii, J. W. Gjerloev, A. Ieda, T. Matsuo, C. Stolle, H. Vanhamäki, A. Yoshikawa

    Annales Geophysicae   26 ( 12 )   3913 - 3932   2008.11

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    Traditionally, due to observational constraints, ionospheric modelling and data analysis techniques have been devised either in one dimension (e.g. along a single radar beam), or in two dimensions (e.g. over a network of magnetometers). With new upcoming missions like the Swarm ionospheric multi-satellite project, or the EISCAT 3-D project, the time has come to take into account variations in all three dimensions simultaneously, as they occur in the real ionosphere. The link between ionospheric electrodynamics and the neutral atmosphere circulation which has gained increasing interest in the recent years also intrinsically requires a truly 3-dimensional (3-D) description. In this paper, we identify five major science questions that need to be addressed by 3-D ionospheric modelling and data analysis. We briefly review what proceedings in the young field of 3-D ionospheric electrodynamics have been made in the past to address these selected question, and we outline how these issues can be addressed in the future with additional observations and/or improved data analysis and simulation techniques. Throughout the paper, we limit the discussion to high-latitude and mesoscale ionospheric electrodynamics, and to directly data-driven (not statistical) data analysis. © 2008 European Geosciences Union.

    DOI: 10.5194/angeo-26-3913-2008

  • Horizontal amplitude and phase structure of low-latitude Pc 3 pulsations around the dawn terminator A11308 Reviewed

    Y. M. Tanaka, K. Yumoto, A. Yoshikawa, M. Itonaga, M. Shinohara, S. Takasaki, B. J. Fraser

    Journal of Geophysical Research: Space Physics   112 ( 11 )   2007.11

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    The horizontal spatial structure of Pc 3 pulsations observed at low geomagnetic latitude (22-46°) around dawn is studied statistically using data acquired by the Circum-pan Pacific Magnetometer Network (CPMN). It is found that while the phase of the H component of low-latitude Pc 3 pulsations remains largely unchanged with the passing of dawn, the D component undergoes a phase shift of ca. 180°. This phase variation across dawn is related to the abrupt change in the major axis orientation of polarization ellipses observed in previous studies. Both the H and D components have higher amplitude after dawn than before dawn. This horizontal amplitude and phase structure is well explained by the response of a nonuniform ionosphere around dawn to incident Alfvén waves, where the secondary electric field caused by charge accumulation at the dawn terminator plays an important role in deformation of the current system. Enhancement of the DIH ratio is also observed just after dawn at very low latitudes (22°). As Alfvén waves are not excited efficiently at very low geomagnetic latitudes, including the magnetic equator, the observed horizontal structure in such regions may be due to a large-scale current system originating at higher latitudes. Copyright 2007 by the American Geophysical Union.

    DOI: 10.1029/2007JA012585

  • Horizontal amplitude and phase structure of low-latitude Pc 3 pulsations around the dawn terminator Reviewed

    Y. -M. Tanaka, K. Yumoto, A. Yoshikawa, M. Itonaga, M. Shinohara, S. Takasaki, B. J. Fraser

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   112 ( A11 )   2007.11

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    The horizontal spatial structure of Pc 3 pulsations observed at low geomagnetic latitude (22-46 degrees) around dawn is studied statistically using data acquired by the Circum-pan Pacific Magnetometer Network ( CPMN). It is found that while the phase of the H component of low-latitude Pc 3 pulsations remains largely unchanged with the passing of dawn, the D component undergoes a phase shift of ca. 180 degrees. This phase variation across dawn is related to the abrupt change in the major axis orientation of polarization ellipses observed in previous studies. Both the H and D components have higher amplitude after dawn than before dawn. This horizontal amplitude and phase structure is well explained by the response of a nonuniform ionosphere around dawn to incident Alfven waves, where the secondary electric field caused by charge accumulation at the dawn terminator plays an important role in deformation of the current system. Enhancement of the D/H ratio is also observed just after dawn at very low latitudes (22 degrees). As Alfven waves are not excited efficiently at very low geomagnetic latitudes, including the magnetic equator, the observed horizontal structure in such regions may be due to a large-scale current system originating at higher latitudes.

    DOI: 10.1029/2007JA012585

  • Horizontal amplitude and phase structure of low-latitude Pc 3 pulsations around the dawn terminator

    Y. -M. Tanaka, K. Yumoto, A. Yoshikawa, M. Itonaga, M. Shinohara, S. Takasaki, B. J. Fraser

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   112 ( A11 )   2007.11

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    The horizontal spatial structure of Pc 3 pulsations observed at low geomagnetic latitude (22-46 degrees) around dawn is studied statistically using data acquired by the Circum-pan Pacific Magnetometer Network ( CPMN). It is found that while the phase of the H component of low-latitude Pc 3 pulsations remains largely unchanged with the passing of dawn, the D component undergoes a phase shift of ca. 180 degrees. This phase variation across dawn is related to the abrupt change in the major axis orientation of polarization ellipses observed in previous studies. Both the H and D components have higher amplitude after dawn than before dawn. This horizontal amplitude and phase structure is well explained by the response of a nonuniform ionosphere around dawn to incident Alfven waves, where the secondary electric field caused by charge accumulation at the dawn terminator plays an important role in deformation of the current system. Enhancement of the D/H ratio is also observed just after dawn at very low latitudes (22 degrees). As Alfven waves are not excited efficiently at very low geomagnetic latitudes, including the magnetic equator, the observed horizontal structure in such regions may be due to a large-scale current system originating at higher latitudes.

    DOI: 10.1029/2007JA012585

  • Pi 2 source region in the magnetosphere deduced from CPMN data Reviewed

    Teiji Uozumi, H. Kawano, A. Yoshikawa, M. Itonaga, K. Yumoto

    Planetary and Space Science   55 ( 6 )   849 - 857   2007.4

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    In order to investigate the source region of Pi 2 and its propagation mechanism in the magnetosphere, we have developed a three-dimensional (3D) propagation model of MHD waves in the magnetosphere and compared it with observational results presented by Uozumi et al. [Propagation characteristics of Pi 2 magnetic pulsations observed at ground high latitudes. J. Geophys. Res. 109, A08203, doi:10.1029/2003JA009898]. We have assumed the propagation mechanism of Pi 2 as follows: fast mode waves are firstly generated at the Pi 2 source region, propagate from there in a 3D manner, and then excite shear Alfvén mode waves via mode conversion. Thus excited Alfvén mode waves then propagate to the Earth, and are observed as Pi 2 pulsations at ground stations. Based on the above propagation, we have assumed the propagation path of Pi 2 starting from a Pi 2 source region located on the magnetic equatorial plane to a ground station, and calculated the Alfvén transit time or time of flight (TOF) of MHD waves propagating in the magnetosphere. The model for the 3D spatial distribution of the Alfvén speed and the fast mode speed (assumed identical, under cold-plasma condition) is constructed based on realistic magnetic field and plasma density models of the magnetosphere. Time differences in model TOFs among our ground stations have been compared with the observed differences in the Pi 2 maximum-power times among the ground stations presented by Uozumi et al. [Propagation characteristics of Pi 2 magnetic pulsations observed at ground high latitudes. J. Geophys. Res. 109, A08203, doi:10.1029/2003JA009898]. As a result, it is suggested that the most probable source location of Pi 2 is 9 RE and 22.5 MLT on the equatorial plane in the magnetotail. This is the first study that deduced the Pi 2 source location in a quantitative manner. The consistency between the observational and the numerical estimation result supports our assumption shown in the above as regards the energy transfer mechanisms of Pi 2s globally observed in the high-latitude region. It is suggested that the generation of fast mode waves in the near-Earth region at the onsets of substorms is the essential process for the global Pi 2 occurrence. © 2006.

    DOI: 10.1016/j.pss.2006.03.016

  • ERG - A small-satellite mission to investigate the dynamics of the inner magnetosphere Reviewed

    K. Shiokawa, K. Seki, Y. Miyoshi, A. Ieda, T. Ono, M. Iizima, T. Nagatsuma, T. Obara, T. Takashima, K. Asamura, Y. Kasaba, A. Matsuoka, Y. Saito, H. Saito, M. Hirahara, Y. Tonegawa, F. Toyama, M. Tanaka, M. Nose, Y. Kasahara, @K. Yumoto,@ Hideaki Kawano, @Akimasa Yoshikawa, Y. Ebihara, A. Yukimatsu, N. Sato, S. Watanabe

    Advances in Space Research   38 ( 8 )   1861 - 1869   2006.12

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    The Earth's inner magnetosphere (inside 10 Re) is a region where particle energy increases to the relativistic energy range. This region is very important as a laboratory where high-energy particle acceleration can be directly measured in a dipolar field configuration, as well as for human activities in space including space weather prediction. Despite abundant in situ satellite measurements, this region has been "missing" because of several difficulties arising from the measurements, such as high-energy particle contamination of low-energy particle measurement, protection against the possible incidence of radiation belt particles on the satellite, and the difficulties of measuring three-dimensional particles over a broad energy range, from a few electron volts to more than 10 MeV. In this paper, we address important scientific topics and propose a possible configuration of small satellites termed Energization and Radiation in Geospace (ERG), which would provide new insights into the dynamics of the inner magnetosphere and strongly contribute to the International Living With a Star project.

    DOI: 10.1016/j.asr.2005.05.089

  • Ground-based observations of a significant decrease in the field line resonance frequency at L ~ 1.4 during a large magnetic storm Reviewed International journal

    Takasaki, S., H. Kawano, Y. Tanaka, A. Yoshikawa, M. Seto, M. Iijima, N. Sato and K. Yumoto

    Earth Planets Space   2006.10

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  • A significant mass density increase during a large magnetic storm in October 2003 obtained by ground-based ULF observations at L~1.4 Reviewed International journal

    #Satoko Takasaki, @Hideaki Kawano, #Yoshimasa Tanaka, @Akimasa Yoshikawa, Masahiro Seto, Masahide Iizima, #Yuki Obana, Natsuo Sato, @Kiyohumi Yumoto

    Earth, Planets and Space   58 ( 5 )   617 - 622   2006.1

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    During 28-31 October, 2003, a series of coronal mass ejections hit the magnetosphere and triggered two consecutive large storms. Three ground magnetometers at L=1.32-1.41 recorded field-line resonances (FLRs) during this interval. The FLR frequencies decreased from 0600 LT on 31 October 2003 during the main phase of the second storm until 12 LT when the recovery phase of this storm began. After the decrease, the FLR frequencies returned to its pre-storm value (at 0600 LT on 31 Oct.) in a few hours. The measured decrease in the FLR frequency suggests a relative increase in mass density along the field lines during the magnetic storm. On the other hand, the total electron content (TEC) data suggest that the ionospheric plasma number density during this storm was similar to that during quiet times. A possible explanation for the increase in mass density would be an outflow of the heavy ions (e.g., O+) from the ionosphere to the plasmasphere.

    DOI: 10.1186/BF03351959

  • North-south asymmetry of the amplitude of high-latitude Pc 3-5 pulsations: Observations at conjugate stations Reviewed

    Y Obana, A Yoshikawa, JV Olson, RJ Morris, BJ Fraser, K Yumoto

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   110 ( A10 )   2005.10

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    The north-south asymmetry of the amplitude of ULF pulsations in the Pc 3-5 band is studied using magnetic field data from the magnetically conjugate stations at L similar to 5.4: Kotzebue (KOT) in the northern hemisphere and Macquarie Island (MCQ) in the southern hemisphere. We obtained the following results for the northward (H) component of magnetic pulsations: (1) The north to south power ratio shows a maximum in the northern winter and a minimum in the northern summer. This "seasonal variation'' is stronger at higher frequencies (Pc 3 and Pc 4 frequencies). (2) The north to south power ratio for the Pc 4 and Pc 5 frequency band is basically greater than 1.0 for all seasons. This "positive offset'' is stronger at lower frequencies. The "seasonal variation'' implies that the magnetohydrodynamic (MHD) waves incident from the magnetosphere are more strongly shielded when the ionospheric conductivity is higher. The "positive offset'' may result from the difference of the background magnetic field intensity between KOT and MCQ.

    DOI: 10.1029/2003JA010242

  • Local time distribution of low and middle latitude ground magnetic disturbances at sawtooth injections of 18–19 April 2002 Reviewed

    Kentarou Kitamura, Hideaki Kawano, Shin‐ichi Ohtani, Akimasa Yoshikawa, Kiyohumi Yumoto

    Journal of Geophysical Research: Space Physics   110 ( A7 )   2005.7

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    Local time distribution of low and middle latitude ground magnetic disturbances at sawtooth injections of 18-19 April 2002
    [1] During a magnetic storm of 18 April 2002, quasi-periodic variations of the low-energy electron flux were observed by the LANL satellites at geosynchronous orbit; this phenomenon has been called the "sawtooth event." During this event, on the ground, magnetic bays and Pi 2 pulsations took place corresponding to each enhancement of the particle flux, and they had features typical to usual substorms. However, unlike typical substorms, the ACE satellite observed no apparent northward turnings of the IMF corresponding to the sawtooth event. In this study, we used ground magnetic data from middle- and low-latitude stations which are distributed widely in the longitudinal direction, selected from the CPMN (Circum-Pan Pacific Magnetometer Network) and INTERMAGNET stations and compared the magnetic variations during the sawtooth event with that of the typical substorm (Lester et al., 1984). We found that the local time distribution of the polarization axis of the Pi 2 pulsations show a good agreement with that for a typical substorm, except that the local time width of the expected current wedge was 12 hours. On the other hand, the H component is predominant in the amplitude of the magnetic bay on the ground; the distribution of the H component also suggests a 12-hour-wide current wedge, which did not develop much in time. From these features, it is suggested that a current wedge was formed during this sawtooth event, and it generated the Pi 2 pulsations on the ground. However, the local time width of the current wedges is much wider than typical substorms, and its uniqueness causes the ground features different from typical substorm-associated magnetic variations on the ground. Copyright 2005 by the American Geophysical Union.

    DOI: 10.1029/2004JA010734

  • Local time distribution of low and middle latitude ground magnetic disturbances at sawtooth injections of 18-19 April 2002

    K Kitamura, H Kawano, S Ohtani, A Yoshikawa, K Yumoto

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   110 ( A7 )   2005.7

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    [1] During a magnetic storm of 18 April 2002, quasi-periodic variations of the low-energy electron flux were observed by the LANL satellites at geosynchronous orbit; this phenomenon has been called the "sawtooth event.'' During this event, on the ground, magnetic bays and Pi 2 pulsations took place corresponding to each enhancement of the particle flux, and they had features typical to usual substorms. However, unlike typical substorms, the ACE satellite observed no apparent northward turnings of the IMF corresponding to the sawtooth event. In this study, we used ground magnetic data from middle- and low-latitude stations which are distributed widely in the longitudinal direction, selected from the CPMN (Circum-Pan Pacific Magnetometer Network) and INTERMAGNET stations and compared the magnetic variations during the sawtooth event with that of the typical substorm (Lester et al., 1984). We found that the local time distribution of the polarization axis of the Pi 2 pulsations show a good agreement with that for a typical substorm, except that the local time width of the expected current wedge was 12 hours. On the other hand, the H component is predominant in the amplitude of the magnetic bay on the ground; the distribution of the H component also suggests a 12-hour-wide current wedge, which did not develop much in time. From these features, it is suggested that a current wedge was formed during this sawtooth event, and it generated the Pi 2 pulsations on the ground. However, the local time width of the current wedges is much wider than typical substorms, and its uniqueness causes the ground features different from typical substorm-associated magnetic variations on the ground.

    DOI: 10.1029/2004JA010734

  • Propagation characteristics of Pi 2 magnetic pulsations observed at ground high latitudes Reviewed

    T Uozumi, K Yumoto, H Kawano, A Yoshikawa, S Ohtani, JV Olson, SI Akasofu, SI Solovyev, EF Vershinin, K Liou, CI Meng

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   109 ( A8 )   2004.8

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    In order to investigate the characteristics of Pi 2 propagation observed in the high-latitude region, ground magnetometer data obtained at high-latitude CPMN stations were analyzed. The power of magnetic perturbation, (DeltaH)(2) + (DeltaD)(2), were calculated for Pi 2 events observed at four stations from 11 February through 20 April 1996 and for Pi 2s observed at two stations from 1 January through 27 March 1997. The times when the power of Pi 2s reached the maximum and the maximum amplitudes were compared among stations. The results are as follows. Pi 2s observed at Kotel'nyy (KTN: MLAT = 69.94degrees, MLON = 201.02degrees) reached the maximum amplitude earlier than those at lower-latitude station Tixie (TIK: MLAT = 65.67degrees, MLON = 196.88degrees), though the amplitudes were smaller at KTN than at TIK on average. The time lag from KTN to TIK has two peaks in its distribution; the primary and the secondary peaks are located around 10 s and 35 s, respectively. The mean value of the whole distribution of the time lag from KTN to TIK is about 20 s. Ultra Violet Image (UVI) data obtained by the Polar satellite was available during the second period; the UVI data indicate that it was when the auroral oval was located equatorward to KTN that the Pi 2 amplitude tended to reach the maximum earlier at KTN than at TIK. This observational result is important because Pi 2 was observed earlier in the polar cap region rather than in the auroral region. That is to say, Pi 2 was observed earlier in the polar cap region, which is not directly connected with the source region of Pi 2 via the magnetic field line. Longitudinal characteristics of Pi 2 propagation were derived by using data from longitudinally separated stations TIK, Chokurdakh (CHD: MLAT = 64.67degrees, MLON = 212.12degrees) and Kotzebue (KOT: MLAT = 64.52degrees, MLON = 249.72degrees). The result indicates the existence of the longitudinal center of Pi 2 propagation. The average magnetic local time of the center is estimated to have been similar to22.5 MLT; eastward (westward) of the center, Pi 2 exhibited an eastward ( westward) propagation. The temporal and spatial developments of the Pi 2 propagation along the auroral zone were derived in an empirical manner. That is, the MLT ( set to zero at the propagation center) dependence of the maximum amplitude time and the maximum amplitude itself of Pi 2 were derived in an empirical manner. As a result it is concluded that in the premidnight sector (i.e., around 22.5 MLT), KTN is the most probable location that observes the maximum amplitude of Pi 2 earliest among the CPMN stations located along 210degrees magnetic meridian. Our results show that the low-latitude Pi 2, which has often been used as a time indicator of substorm onset, is often delayed from the Pi 2 observed in the premidnight polar cap region. The present results imply that the consideration of high-latitude Pi 2s in addition to low-latitude Pi 2s can provide a new insight into the substorm onset timing. Thus it is necessary to consider the global features, especially Pi 2s observed in higher-latitude region, for studying substorm onset timing issues.

    DOI: 10.1029/2003JA009898

  • Propagation characteristics of Pi 2 magnetic pulsations observed at ground high latitudes Reviewed

    Teiji Uozumi, K. Yumoto, H. Kawano, A. Yoshikawa, S. Ohtani, J. V. Olson, S. I. Akasofu, S. I. Solovyev, E. F. Vershinin, K. Liou, C. I. Meng

    Journal of Geophysical Research: Space Physics   109 ( A8 )   2004.8

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    [1] In order to investigate the characteristics of Pi 2 propagation observed in the high-latitude region, ground magnetometer data obtained at high-latitude CPMN stations were analyzed. The power of magnetic perturbation, (ΔH)2 + (ΔD)2, were calculated for Pi 2 events observed at four stations from 11 February through 20 April 1996 and for Pi 2s observed at two stations from 1 January through 27 March 1997. The times when the power of Pi 2s reached the maximum and the maximum amplitudes were compared among stations. The results are as follows. Pi 2s observed at Kotel'nyy (KTN: MLAT = 69.94°, MLON = 201.02°) reached the maximum amplitude earlier than those at lower-latitude station Tixie (TIK: MLAT = 65.67°, MLON = 196.88°), though the amplitudes were smaller at KTN than at TIK on average. The time lag from KTN to TIK has two peaks in its distribution; the primary and the secondary peaks are located around 10 s and 35 s, respectively. The mean value of the whole distribution of the time lag from KTN to TIK is about 20 s. Ultra Violet Image (UVI) data obtained by the Polar satellite was available during the second period; the UVI data indicate that it was when the auroral oval was located equatorward to KTN that the Pi 2 amplitude tended to reach the maximum earlier at KTN than at TIK. This observational result is important because Pi 2 was observed earlier in the polar cap region rather than in the auroral region. That is to say, Pi 2 was observed earlier in the polar cap region, which is not directly connected with the source region of Pi 2 via the magnetic field line. Longitudinal characteristics of Pi 2 propagation were derived by using data from longitudinally separated stations TIK, Chokurdakh (CHD: MLAT = 64.67°, MLON = 212.12°) and Kotzebue (KOT: MLAT = 64.52°, MLON = 249.72°). The result indicates the existence of the longitudinal center of Pi 2 propagation. The average magnetic local time of the center is estimated to have been ∼22.5 MLT; eastward (westward) of the center, Pi 2 exhibited an eastward (westward) propagation. The temporal and spatial developments of the Pi 2 propagation along the auroral zone were derived in an empirical manner. That is, the MLT (set to zero at the propagation center) dependence of the maximum amplitude time and the maximum amplitude itself of Pi 2 were derived in an empirical manner. As a result it is concluded that in the premidnight sector (i.e., around 22.5 MLT), KTN is the most probable location that observes the maximum amplitude of Pi 2 earliest among the CPMN stations located along 210° magnetic meridian. Our results show that the low-latitude Pi 2, which has often been used as a time indicator of substorm onset, is often delayed from the Pi 2 observed in the premidnight polar cap region. The present results imply that the consideration of high-latitude Pi 2s in addition to low-latitude Pi 2s can provide a new insight into the substorm onset timing. Thus it is necessary to consider the global features, especially Pi 2s observed in higher-latitude region, for studying substorm onset timing issues. Copyright 2004 by the American Geophysical Union.

    DOI: 10.1029/2003JA009898

  • Longitudinal structure of Pc3 pulsations on the ground near the magnetic equator Reviewed

    Y. M. Tanaka, K. Yumoto, A. Yoshikawa, M. Shinohara, H. Kawano, T. I. Kitamura

    Journal of Geophysical Research: Space Physics   109 ( A3 )   A03201   2004.3

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    It has been generally accepted that there are two models for the propagation mechanism of Pc3 pulsations observed on the ground near the magnetic equator, as follows: (1) Compressional waves, propagating along the equatorial plane of the magnetosphere across the ambient magnetic field lines, arrive at the equatorial ionosphere and couple with the magnetic perturbations on the ground through the ionosphere (compressional wave model); (2) Alfvén waves or compressional waves, propagating into the high-latitude ionosphere, generate large-scale ionospheric current oscillations there, and then they leak to the low latitude and cause Pc3 pulsations near the magnetic equator (ionospheric current model). In order to clarify which of these models is more suitable for Pc3 pulsations on the ground near the magnetic equator, the longitudinal structures of their coherence, amplitude, and phase were statistically studied by using three longitudinally separated subequatorial stations, CRI (Φ = 3.01°, A = 273.44°), GUA (Φ = 5.60°, A = 215.50°), and MUT (Φ = 6.24°, A = 192.17°). We found a nearly inphase structure in the 0730-1700 LT sector and a nearly 180° phase shift across 0730 LT for high-coherence Pc3 events in the H component. The longitudinal phase structure can be explained by the ionospheric current model; in this case, the 180° phase shift across 0730 LT means a meridional current along the dawn terminator supplied from the source at higher latitudes. The compressional wave model cannot explain the 180° phase shift across 0730 LT if the ionosphere is assumed as an infinitely thin sheet; however, the compressional wave model still remains as a candidate if we treat the ionosphere as that having a finite thickness. The data at hand do not let us conclude which of the two models is more appropriate; still, the longitudinal phase structure, shown in this paper, is a new finding that has never been reported and is important for understanding how Pc3 pulsations propagate from the magnetosphere to the equatorial ionosphere. Copyright 2004 by the American Geophysical Union.

    DOI: 10.1029/2003JA009903

  • Longitudinal structure of Pc3 pulsations on the ground near the magnetic equator Reviewed

    YM Tanaka, K Yumoto, A Yoshikawa, M Shinohara, H Kawano, TI Kitamura

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   109 ( A3 )   2004.3

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    [1] It has been generally accepted that there are two models for the propagation mechanism of Pc3 pulsations observed on the ground near the magnetic equator, as follows: ( 1) Compressional waves, propagating along the equatorial plane of the magnetosphere across the ambient magnetic field lines, arrive at the equatorial ionosphere and couple with the magnetic perturbations on the ground through the ionosphere ( compressional wave model); ( 2) Alfven waves or compressional waves, propagating into the high-latitude ionosphere, generate large-scale ionospheric current oscillations there, and then they leak to the low latitude and cause Pc3 pulsations near the magnetic equator ( ionospheric current model). In order to clarify which of these models is more suitable for Pc3 pulsations on the ground near the magnetic equator, the longitudinal structures of their coherence, amplitude, and phase were statistically studied by using three longitudinally separated subequatorial stations, CRI (Phi = 3.01degrees, Lambda = 273.44degrees), GUA (Phi = 5.60degrees, Lambda = 215.50degrees), and MUT (Phi = 6.24degrees, Lambda = 192.17degrees). We found a nearly inphase structure in the 0730 - 1700 LT sector and a nearly 180degrees phase shift across 0730 LT for high-coherence Pc3 events in the H component. The longitudinal phase structure can be explained by the ionospheric current model; in this case, the 180degrees phase shift across 0730 LT means a meridional current along the dawn terminator supplied from the source at higher latitudes. The compressional wave model cannot explain the 180degrees phase shift across 0730 LT if the ionosphere is assumed as an infinitely thin sheet; however, the compressional wave model still remains as a candidate if we treat the ionosphere as that having a finite thickness. The data at hand do not let us conclude which of the two models is more appropriate; still, the longitudinal phase structure, shown in this paper, is a new finding that has never been reported and is important for understanding how Pc3 pulsations propagate from the magnetosphere to the equatorial ionosphere.

    DOI: 10.1029/2003JA009903

  • Enhancements of the plasmaspheric density in its low-L part during magnetic storms Reviewed International journal

    #Takasaki, S., Y., @H. Kawano, #Y. Tanaka, @A. Yoshikawa, M. Seto, M. Iizima, and @K. Yumoto

    Proceeding of The fifth Workshop on Applications of Radio Science (WARS) obart Australia, on Feb. 18-20, 2004   2004.2

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  • Excitation of a Hall‐current generator by field‐aligned current closure, via an ionospheric, divergent Hall‐current, during the transient phase of magnetosphere–ionosphere coupling Reviewed

    Akimasa Yoshikawa

    Journal of Geophysical Research: Space Physics   107 ( A12 )   2002.12

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    Excitation of a Hall-current generator by field-aligned current closure, via an ionospheric, divergent Hall-current, during the transient phase of magnetosphere-ionosphere coupling
    To clarify the process by which an ionospheric current system is formed by field-aligned current (FAC) closure in the ionosphere, an inclusive formulation of magnetosphere-ionosphere (MI) coupling is undertaken. The "Hall-current generator", which is excited during the transient phase of MI coupling, plays a crucial role in the formation of the ionospheric rotational-current system. It extracts energy from the FAC system through the divergent Hajl-current and pumps it into the rotational Hall-current. The energy of the rotational current accumulates as an evanescent poloidal magnetic field, associated with the ionospheric surface wave. This accumulated energy is also fed back to the FAC system through the change in energy flow of the Hall-current generator. It is found that there is a typical timescale for the rotational-current system to accumulate or extract the poloidal magnetic energy of ionospheric surface waves. This depends on the inductance of the rotational-current system and the effective conductivity of the ionospheric rotational current. This characteristic timescale becomes the cause of an ionospheric inductive effect, such as a time delay or phase lag between the source electromagnetic field of the FAC and the corresponding poloidal magnetic field on the ground. The latter causes an inductive shielding effect on the amplitude of the geomagnetic disturbance. Numerical simulation has been able to explain the details of the physical process that occurs when the incident FAC is developing and decaying, and how the energy and current are redistributed into the other elements during the transient MI-coupling process Copyright 2002 by the American Geophysical Union.

    DOI: 10.1029/2001JA009170

  • Excitation of a Hall-current generator by field-aligned current closure, via an ionospheric, divergent Hall-current, during the transient phase of magnetosphere-ionosphere coupling

    A Yoshikawa

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   107 ( A12 )   2002.12

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    To clarify the process by which an ionospheric current system is formed by field-aligned current (FAC) closure in the ionosphere, an inclusive formulation of magnetosphere-ionosphere (MI) coupling is undertaken. The "Hall-current generator'', which is excited during the transient phase of MI coupling, plays a crucial role in the formation of the ionospheric rotational-current system. It extracts energy from the FAC system through the divergent Hall-current and pumps it into the rotational Hall-current. The energy of the rotational current accumulates as an evanescent poloidal magnetic field, associated with the ionospheric surface wave. This accumulated energy is also fed back to the FAC system through the change in energy flow of the Hall-current generator. It is found that there is a typical timescale for the rotational-current system to accumulate or extract the poloidal magnetic energy of ionospheric surface waves. This depends on the inductance of the rotational-current system and the effective conductivity of the ionospheric rotational current. This characteristic timescale becomes the cause of an ionospheric inductive effect, such as a time delay or phase lag between the source electromagnetic field of the FAC and the corresponding poloidal magnetic field on the ground. The latter causes an inductive shielding effect on the amplitude of the geomagnetic disturbance. Numerical simulation has been able to explain the details of the physical process that occurs when the incident FAC is developing and decaying, and how the energy and current are redistributed into the other elements during the transient MI-coupling process.

    DOI: 10.1029/2001JA009170

  • Diagrammatic method to describe the self-inductive response of the magnetosphere-ionosphere-atmosphere-Earth electromagnetically coupled system as a quasi-particle excitation Reviewed

    A Yoshikawa, K Yumoto, M Shinohara, M Itonaga

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   107 ( A5 )   2002.5

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    [1] A diagrammatic method to intuitively describe the inductive response of wave fields in the magnetosphere-ionosphere-atmosphere-Earth (MIAE) electromagnetically coupled system is developed. The coupling process of magnetohydrodynamic (MHD) waves and atmospheric electromagnetic waves, which interact with an anisotropically conducting thin sheet ionosphere, can be understood in terms of a process of redistribution of the induced current of wave modes. On the basis of the current conservation law and Faraday's law of electromagnetic induction, a redistribution process of the source-induced current of wave modes to the secondary wave is simply illustrated. The purpose of this paper is to propose a methodology to describe the inductive response of a complex electromagnetically coupled system that is divided by a conducting boundary layer. As an example, we derive the reflection coefficient and the mode conversion ratio of MHD waves at an anisotropic, inductive ionosphere by using the concept of induced current redistribution. We also demonstrate that the redistribution process of wave modes under the law of conservation of induced current also satisfies an energy conservation law in the MIAE system. However, the true merit of this method is its applicability to the highly inhomogeneous region, in which many types of waves exist and interact through the arbitrary boundary layers.

    DOI: 10.1029/2000JA000405

  • Diagrammatic method to describe the self-inductive response of the magnetosphere-ionosphere-atmosphere-Earth electromagnetically coupled system as a quasi-particle excitation Reviewed

    Akimsa Yoshikawa, Kiyohumi Yumoto, Manabu Shinohara, Masahiro Itonaga

    Journal of Geophysical Research: Space Physics   107 ( A5 )   2002.5

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    [i] A diagrammatic method to intuitively describe the inductive response of wave fields in the magnetosphere-ionosphere-atmosphere-Earth (MIAE) electromagnetically coupled system is developed. The coupling process of magnetohydrodynamic (MHD) waves and atmospheric electromagnetic waves, which interact with an anisotropically conducting thin sheet ionosphere, can be understood in terms of a process of redistribution of the induced current of wave modes. On the basis of the current conservation law and Faraday's law of electromagnetic induction, a redistribution process of the source-induced current of wave modes to the secondary wave is simply illustrated. The purpose of this paper is to propose a methodology to describe the inductive response of a complex electromagnetically coupled system that is divided by a conducting boundary layer. As an example, we derive the reflection coefficient and the mode conversion ratio of MHD waves at an anisotropic, inductive ionosphere by using the concept of induced current redistribution. We also demonstrate that the redistribution process of wave modes under the law of conservation of induced current also satisfies an energy conservation law in the MIAE system. However, the true merit of this method is its applicability to the highly inhomogeneous region, in which many types of waves exist and interact through thearbitrary boundary layers. Copyright 2002 by the American Geophysical Union.

    DOI: 10.1029/2000JA000405

  • Hall‐induced inductive shielding effect on geomagnetic pulsations Reviewed

    Akimasa Yoshikawa, Yuki Obana, Manabu Shinohara, Masahiro Itonaga, Kiyohumi Yumoto

    Geophysical Research Letters   29 ( 8 )   107-1 - 107-4   2002.4

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    Hall-induced inductive shielding effect on geomagnetic pulsations
    A new formula describing the inductive response of the magnetosphere-ionosphere-atmosphere-Earth electromagnetic coupled system to the time development of the field-aligned current (FAC) source-field is developed. Using this new formula, the Hall-induced inductive shielding effect (ISE) on geomagnetic pulsation is investigated. The ISE is caused by the reduction of the amplitude of total rotational current because of the generation of "inductive" rotational current by the inductive part of ionospheric divergent electric field, which originates the existence of divergent Hall current. It will be shown that the ISE is more efficient for high-frequency pulsations, large horizontal scale phenomena and high-conducting ionospheric conditions. Quantitative analysis strongly suggests that the ionospheric conductivity in the dayside hemisphere can easily reach and sometimes exceed the turning point of geomagnetic pulsations of which frequencies are in the Pc 3 ∼ 4 pulsations range.

    DOI: 10.1029/2001GL013610

  • Hall-induced inductive shielding effect on geomagnetic pulsations Reviewed

    Akimasa Yoshikawa, Yuki Obana, Manabu Shinohara, Masahiro Itonaga, Kiyohumi Yumoto

    Geophysical Research Letters   29 ( 8 )   107 - 1-107-4   2002.4

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    A new formula describing the inductive response of the magnetosphere-ionosphere-atmosphere-Earth electromagnetic coupled system to the time development of the field-aligned current (FAC) source-field is developed. Using this new formula, the Hall-induced inductive shielding effect (ISE) on geomagnetic pulsation is investigated. The ISE is caused by the reduction of the amplitude of total rotational current because of the generation of "inductive" rotational current by the inductive part of ionospheric divergent electric field, which originates the existence of divergent Hall current. It will be shown that the ISE is more efficient for high-frequency pulsations, large horizontal scale phenomena and high-conducting ionospheric conditions. Quantitative analysis strongly suggests that the ionospheric conductivity in the dayside hemisphere can easily reach and sometimes exceed the turning point of geomagnetic pulsations of which frequencies are in the Pc 3 ∼ 4 pulsations range.

  • How does the ionospheric rotational Hall current absorb the increasing energy from the field‐aligned current system? Reviewed

    Akimasa Yoshikawa

    Geophysical Research Letters   29 ( 7 )   37 - 1   2002.4

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    How does the ionospheric rotational Hall current absorb the increasing energy from the field-aligned current system?
    It has been well recognized that field-aligned current (FAC) systems lose their energy in the ionosphere through the Joule dissipation that is caused by their closure via the ionospheric Pedersen current, and that the ionospheric Hall current cannot contribute the total energy dissipation. However, it is also true that the rotational Hall current is excited by the incident FAC, and it radiates a Poynting vector that grows a poloidal-type magnetic field. Even if the Hall effect cannot do work on an external system, what does its contribution to the accumulation of poloidal magnetic energy really mean? In this paper, it is clarified that the divergent Hall current, excited during the transient phase of magnetosphere-ionosphere coupling, closes via the FAC and produces a Hall current generator, which pumps up the energy of the FAC system to increase the ionospheric rotational Hall current (together with its associated poloidal magnetic field).

    DOI: 10.1029/2001GL014125

  • A numerical simulation of the Pi2 pulsations associated with the substorm current wedge Reviewed

    S Fujita, H Nakata, M Itonaga, A Yoshikawa, T Mizuta

    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS   107 ( A3 )   2002.3

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    [1] The present paper deals with the transient behavior of MHD perturbations in the inner magnetosphere induced by an impulsive localized eastward current (source current) as a model of Pi2 pulsations in the magnetosphere. The magnetospheric model consists of a dipole magnetic field, plasmasphere, ionosphere with Pedersen conductivity, and a free outer boundary. The source current is an impulsive magnetospheric current at the onset of the substorm current wedge and is distributed around the equatorial plane of L = 10 with +/-2 hour longitudinal extent around midnight. The numerical results allow us to track variation in the expected Pi2 pulsation signals in both local time and L. The poloidal-mode wave exhibits plasmasphere virtual resonance, resulting in large amplitudes around midnight, weakening toward dayside. The toroidal-mode wave is excited as a field line resonance immediately after the wave front of the poloidal-mode wave crosses regions where the radial gradient of V-A is steep. The toroidal-mode wave has largest amplitude at the local time of the east/west edge of the source current. The duration of this wave is similar to5 min. In the middle plasmasphere where the radial gradient of the V-A is smaller, the poloidal-mode wave tends to predominate over the toroidal-mode wave. These numerical results are consistent with satellite observations, in so far as the day-night asymmetry of Pi2 pulsations and the observation of transient toroidal waves.

    DOI: 10.1029/2001JA900137

  • A numerical simulation of the Pi2 pulsations associated with the substorm current wedge Reviewed

    S. Fujita, H. Nakata, M. Itonaga, A. Yoshikawa, T. Mizuta

    Journal of Geophysical Research: Space Physics   107 ( A3 )   2002.3

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    The present paper deals with the transient behavior of MHD perturbations in the inner magnetosphere induced by an impulsive localized eastward current (source current) as a model of Pi2 pulsations in the magnetosphere. The magnetospheric model consists of a dipole magnetic field, plasmasphere, ionosphere with Pedersen conductivity, and a free outer boundary. The source current is an impulsive magnetospheric current at the onset of the substorm current wedge and is distributed around the equatorial plane of L = 10 with ±2 hour longitudinal extent around midnight. The numerical results allow us to track variation in the expected Pi2 pulsation signals in both local time and L. The poloidal-mode wave exhibits plasmasphere virtual resonance, resulting in large amplitudes around midnight, weakening toward dayside. The toroidal-mode wave is excited as a field line resonance immediately after the wave front of the poloidal-mode wave crosses regions ? where the radial gradient of VA is steep. The toroidal-mode wave has largest amplitude at the local time of the east/west edge of the source current. The duration of this wave is ̃5 min. In the middle plasmasphere where the radial gradient of the VA is smaller, the poloidal-mode wave tends to predominate over the toroidal-mode wave. These numerical results are consistent with satellite observations, in so far as the day-night asymmetry of Pi2 pulsations and the observation of transient toroidal waves. Copyright 2002 by the American Geophysical Union.

    DOI: 10.1029/2001JA900137

  • Propagation property of transient MHD impulses in the magnetosphere - Ionosphere system: The 2D model of the Pi2 pulsation

    S. Fujita, T. Mizuta, M. Itonaga, A. Yoshikawa, H. Nakata

    Geophysical Research Letters   28 ( 11 )   2161 - 2164   2001.6

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    Propagation property of the 2D-coupled MHD wave induced from an impulsive current is studied by using a magnetospheric model having the dipole magnetic field, tile ionosphere with Pedersen conductivity, and a free outer boundary. This study is the first step toward realistic modeling of Pi2 pulsation generated by the current wedge model. Numerical calculation reveals that the ionosphere controls not only damping of the field-line resonance oscillation but also its frequency. The field-line resonance oscillation exhibits the fundamental mode structure along the field line in the plasmasphere. In high latitudes, there are waves bouncing between the ionospheres. This suggests that the waveform in the middle- and low-latitudes is different from that in high-latitudes.

    DOI: 10.1029/2000GL000108

  • Transient MHD impulses in the magnetosphere-ionosphere system: The 2D model of the Pi2 pulsations Reviewed International journal

    Fujita S., T. Mizuta, @M. Itonaga, H. Nakata and @A. Yoshikawa

    Geophysical Research Letters   2001.1

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  • A wave equation describing the generation of field-aligned current in the magnetosphere

    Masahiro Itonaga, Akimasa Yoshikawa, Shigeru Fujita, Shigeru Fujita

    Earth, Planets and Space   52 ( 7 )   503 - 507   2000.8

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    A wave equation describing the generation of field-aligned current (FAC) in the magnetosphere is derived. The equation has four source terms. The first and second terms represent the effects of inhomogeneous Alfven speed (VA) and curvilinear magnetic field line, respectively. The perpendicular perturbation inertial current produces the perturbation FAC via these effects. Around the magnetic equator in the region of dipolar magnetic field where VA is inversely proportional to the power of the radial distance from the Earth's center, the first and second terms have magnitudes of the same order and their signs are identical. The first term dominates over the second one around the region where the gradient of VA is sharp and vice versa around the position where the stretched field line intersects the magnetic equator. The third and fourth terms are related to the diamagnetic current. When the unperturbed magnetic pressure has an inhomogeneous distribution, the perpendicular diamagnetic current due to the perturbation of the plasma pressure yields the perturbation FAC (third term). When the perpendicular diamagnetic current flows in the unperturbed state, the perturbations of the magnetic and plasma pressures also bring about the perturbation FAC (fourth term). In the case of β ~ 1, the third and fourth terms have magnitudes of the same order. If the disturbance bears a diamagnetic property, this would be especially the case. However, if the disturbance propagates perpendicularly to the ambient magnetic field, the perturbation FAC would be little generated by the fourth term. © 2000, The Seismological Society of Japan, Society of Geomagnetism and Earth, Planetary and Space Sciences, The Volcanological Society of Japan, The Geodetic Society of Japan, The Japanese Society for Planetary Sciences. All rights reserved.

    DOI: 10.1186/BF03351654

  • Characteristics of energy transfer of Pi 2 magnetic pulsations: Latitudinal dependence Reviewed

    T. Uozumi, K. Yumoto, H. Kawano, A. Yoshikawa, J. V. Olson, S. I. Solovyev, E. F. Vershinin

    Geophysical Research Letters   27 ( 11 )   1619 - 1622   2000.6

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    To investigate the generation and propagation mechanisms of Pi 2 magnetic pulsations, we have analyzed magnetic field data from the 210° magnetic meridian (MM) stations. We used 50 Pi 2 events that were simultaneously observed at seven stations along the 210° MM during January 1995, and focused our analysis on associated magnetic energy, ((ΔH)2+(ΔD)2)/μ<inf>0</inf>. The times when the amplitude of the magnetic energy attained the maximum (T(max)) were compared among these stations. We found that T(max) has a latitudinal dependence, especially at higher latitudes, which has not been previously reported. At Kotel'nyy (L=8.50) on the poleward side of the auroral region, T(max) occurred an average of 21 seconds earlier than T(max) at Guam (L=1.01), and often as much as one minute earlier. The existence of latitudinal variation has implications for interpretation of issues related to timing of substorm onset; it is necessary to consider the global features of Pi 2 events in the study of auroral and magnetospheric substorms.

    DOI: 10.1029/1999GL010767

  • The nature of reflection and mode conversion of MHD waves in the inductive ionosphere: Multistep mode conversion between divergent and rotational electric fields Reviewed

    A. Yoshikawa, M. Itonaga

    Journal of Geophysical Research: Space Physics   105 ( A5 )   10565 - 10584   2000.5

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    The nature of reflection and mode conversion of MHD waves at the high-latitudinal inductive ionosphere is analyzed, based on the current conservation law of wave modes. The term "inductive ionosphere" refers to the nonzero rotational electric field or nonzero compressional magnetic field in the reflection process of shear Alfvén waves on the ionosphere. The finite rotational electric field causes mutual induction between the divergent and rotational current systems at the ionosphere. The one-step Hall effect for the divergent electric field of the shear Alfvén wave produces a rotational Hall current and excites the ionospheric surface compressional wave. The Hall effect for the rotational electric field of an ionospheric surface compressional wave produces a divergent Hall current (two-step Hall effect), which feeds back the compressional magnetic energy to the reflected field-aligned current. We find that the renormalization of the ionospheric rotational electric field to the reflection process of the shear Alfvén wave causes some peculiarities in the distribution of ionospheric currents and mode-converted wave magnetic fields. Such peculiarities become particularly obvious in the high-conducting ionosphere. For example, in the ionospheric current distributions, a considerable component of the ionospheric divergent current is accounted for by the divergent Hall current. The rotational Hall and Pedersen currents cancel each other out and lead to zero total ionospheric rotational current. The amplitude of the poloidal magnetic field transmitted from the toroidal magnetic field of the incident shear Alfvén wave shows a nonlinear dependence on ΣH/ΣP. It also shows a new type of effective ionospheric shielding effect in the ΣP/ΣA parameter space for a fixed ΣH/ΣP condition. We assert that the inductive response of the ionosphere should become an indispensable concept for reflection, mode conversion, transmission, and generation of various phenomena relating to the field-aligned current system. Copyright 2000 by the American Geophysical Union.

    DOI: 10.1029/1999ja000159

  • Ground magnetic perturbations associated with the standing toroidal mode oscillations in the magnetosphere ? ionosphere system Reviewed International journal

    Nakata, H., S. Fujita, @A.Yoshikawa M. Itonaga and K. Yumoto

    Earth Planets Space   52 ( 9 )   601 - 613   2000.1

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  • Ground magnetic perturbations associated with the standing toroidal mode oscillations in the magnetosphere-ionosphere system

    Hiroyuki Nakata, Hiroyuki Nakata, Shigeru Fujita, Shigeru Fujita, Akimasa Yoshikawa, Masahiro Itonaga, Kiyohumi Yumoto

    Earth, Planets and Space   52 ( 9 )   601 - 613   2000.1

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    Ground magnetic perturbations associated with the standing toroidal mode oscillations in the magnetosphere-ionosphere system
    The behavior of toroidal mode oscillations of standing Alfvén waves (refer to as standing Alfvén oscillations) in the coupled magnetosphere-ionosphere system is investigated using a trapezoid-shape magnetosphere model. It is found that the magnetic perturbation is transmitted across the ionosphere differently in the two cases where the ionospheric electric field perturbation is static (Pedersen conductivity > Hall conductivity) and where it is inductive (Pedersen conductivity < Hall conductivity). It is noted that the ionospheric Hall current for the inductive condition shields the magnetic field perturbation. The north-south asymmetry of the conjugate ground magnetic perturbations is calculated by using a trapezoid model with the ionospheric and magnetospheric parameters based on the IGRF and IRI. It is revealed that the ionospheric electric field is almost static for the fundamental mode oscillation, whereas inductive for the higher harmonic ones. It is also found that the north-south asymmetry of the ground magnetic perturbations depends not only on the L-value but also on magnetic longitude; this is because the ionosphere and magnetic field conditions are not uniform as a function of longitude.

    DOI: 10.1186/BF03351669

  • Eigenmode analysis of field line oscillations interacting with the ionosphere‐atmosphere‐solid earth electromagnetic coupled system Reviewed

    Akimasa Yoshikawa, Masahiro Itonaga, Shigeru Fujita, Hiroyuki Nakata, Kiyohumi Yumoto

    Journal of Geophysical Research: Space Physics   104 ( A12 )   28437 - 28457   1999.12

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    Eigenmode analysis of field line oscillations interacting with the ionosphere-atmosphere-solid earth electromagnetic coupled system
    In order to understand the effect of ionosphere on the localized toroidal magnetic shell oscillation (field line oscillation), we have constructed a rectangular box model for the magnetosphere-ionosphere-solid earth system including the anisotropically conducting ionosphere and performed the eigenmode analysis of the magnetohydrodynamic (MHD) waves in the model. We have found that the eigenmodes of field line oscillation are effectively controlled by the height-integrated Pedersen and Hall conductivities, meaning that the field-aligned current (FAC) in the magnetosphere is closed to both the Pedersen current and the Hall current. The divergent Hall current, that is, the Hall current, which closes the FAC, is a new found current that is driven by the Hall effect of the ionospheric inductive (rotational) electric field. The divergent Hall current brings into sharp relief by considering the ionosphere to be inductive, and it inevitably requires the electromagnetic coupling between the magnetosphere, ionosphere, atmosphere, and solid earth. The nature of the ionospheric current associated with the standing shear Alfven mode is also analyzed in detail by using the concept of wave reflection and mode conversion at the inductive ionosphere. In particular, we emphasize that the magnetic flux sustained by the rotational Hall current, that is, accompanied by the radiation of fast magnetosonic wave to the magnetosphere and atmospheric poloidal magnetic wave to the atmosphere, should be taken into account for magnetosphere-ionosphere coupling of FAC.

    DOI: 10.1029/1999ja900287, 10.1186/bf03351669_references_DOI_QZjTXhdUbFP8cCtoeB591eezRJP, 10.1029/2011ja016460_references_DOI_QZjTXhdUbFP8cCtoeB591eezRJP, 10.1186/bf03351736_references_DOI_QZjTXhdUbFP8cCtoeB591eezRJP, 10.1186/bf03352541_references_DOI_QZjTXhdU

  • Transient response of the non-uniform equatorial ionosphere to compressional MHD waves Reviewed

    M. Itonaga, A. Yoshikawa, K. Yumoto

    Journal of Atmospheric and Solar-Terrestrial Physics   60 ( 2 )   253 - 261   1998.1

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    By assuming a realistic distribution of the height-integrated Cowling conductivity along the noon meridian, the transient response of the non-uniform equatorial ionosphere to plane compressional MHD waves is examined numerically. The direct incidence of an SC-type disturbance (or DL-field) on the ionosphere produces no preliminary reverse impulse (PRI) changes around the dayside equator, supporting the view that the equatorial PRI is caused by an extension of the ionospheric current responsible for the high-latitude PRI. The rise of the ground DL-field at the dip equator lags behind those in the off-equatorial region. This is a new finding which has not yet been reported observationally. When a magnetic pulsation is incident on the dayside ionosphere, the phase of the ground magnetic perturbation at the dip equator also lags behind those in the off-equatorial region. The phase lag at the dip equator obtained numerically agrees approximately with those observed for daytime Pi2 pulsations. However, the amplitude of the ground magnetic perturbation obtained numerically is depressed at the dip equator. Such a depression is contrary to the observational fact that the pulsation amplitude is enhanced at the dayside equator. Since there exists a sharp increase of the ionospheric zonal current at the dayside equator, the Pi2 pulsations around the dayside equator may also be due to the ionospheric current of polar origin. © 1998 Elsevier Science Lid. All rights reserved.

    DOI: 10.1016/S1364-6826(97)00110-7

  • Wave characteristics of geomagnetic pulsations across the dip equator Reviewed

    M. Shinohara, K. Yumoto, N. Hosen, Akimasa Yoshikawa, H. Tachihara, O. Saka, T. I. Kitamura

    Journal of Geophysical Research: Space Physics   103 ( A6 )   11745 - 11754   1998.1

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    In order to clarify the wave characteristics of Pi2 and Pc 4-5 magnetic pulsations around the dip equator, we analyzed magnetic data from the latitudinally dense magnetometer array in Brazil. We found that the phase difference between Pi2 pulsations observed at globally separated low-latitude stations is small, whereas Pi2 pulsations observed within the dayside dip equator region of ±2° latitude show phase lags of about 30° ∼ 50° behind those in the off-dip equator region. Pc 4-5 magnetic pulsations at the dip equator also show the same phase character. Pi2 amplitudes are enhanced in the equatorial region, where the phase lags of pulsations must be associated with the enhancement of ionospheric conductivity. The equatorial phase lags can be explained by invoking the induction effect of the equatorial enhanced ionospheric current above the good conductor Earth.

  • Wave characteristics of daytime and nighttime Pi 2 pulsations at the equatorial and low latitudes Reviewed International journal

    @M. Shinohara, @K. Yumoto, @Akimasa Yoshikawa, @O. Saka, S. I. Solovyev, E. F. Vershinin, N. B. Trivedi, J. M. Da Costa

    Geophysical Research Letters   24 ( 18 )   2279 - 2282   1997.1

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    Peculiarities of daytime and nighttime Pi 2 pulsations at the dip equator are examined by using multipoint measurements from the 210° magnetic meridian (MM) magnetometer network. We found that during daytime the amplitude of Pi 2 pulsations at the dip equator is enhanced, and the phase lags ∼ 34° behind those at low-latitude (magnetic latitude Φ = 19.5-46.2°) stations. On the other hand, during nighttime the amplitude of Pi 2 pulsations at the dip equator is depressed, and the phase lags ∼ 18° behind those at the lower latitudes. Because the zonal ionospheric conductivity at the dip equator is much higher than that at the off-dip equator region, Pi 2 signals are expected to be distorted more effectively at the dip equator. The observations imply that the daytime and nighttime Pi 2 pulsations in the equatorial and low-latitude regions can be explained by invoking an instantaneous penetration of electric field variations from the nightside polar ionosphere to the dayside equatorial ionosphere, and a direct incidence of compressional oscillations from the nightside inner magnetosphere, respectively.

    DOI: 10.1029/97GL02146

  • One-dimensional transient response of the inner magnetosphere at the magnetic equator, 1. Transfer function and poles Reviewed

    M. Itonaga, Akimasa Yoshikawa, K. Yumoto

    Earth, Planets and Space   49 ( 1 )   21 - 48   1997

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    One-dimensional transient response of the inner magnetosphere at the magnetic equator is investigated using two models of altitude distribution of the Alfvén speed VA. The present paper concentrates on the transfer function of the system under consideration and its poles, which govern the transient response of the system. The poles, which are mathematical counterparts of the cavity resonances, appear owing to the inhomogeneity of VA and their locations depend on the altitude distribution of VA as well as the position of external source (or outer boundary of the inner magnetosphere). Even if there exists no strong Alfvén velocity gradient at the outer boundary, an observable cavity-mode oscillation in the Pi2 range can be excited because of the existence of a strong gradient of the plasmapause within the inner magnetosphere. However, the existence of a strong gradient at the outer boundary brings about a long-lived nature of the cavity-mode oscillation as well as calls some new poles into existence. While the surface of the solid earth forms the inner boundary at which the almost perfect reflection of wave takes place, the ionosphere is of secondary importance as a reflector of wave. The existence of the solid earth plays an essential role in the observability of the compressional oscillation arising from the cavity resonance all over the inner magnetosphere. The real part of each pole has a negative value, meaning that the cavity-mode oscillation decays with a damping factor of absolute value of the real part of the pole. Such a damping is primarily due to the leakage of energy through the outer boundary of the inner magnetosphere.

  • One-dimensional transient response of the inner magnetosphere at the magnetic equator, 2. Analysis of waveforms Reviewed

    M. Itonaga, Akimasa Yoshikawa, K. Yumoto

    Earth, Planets and Space   49 ( 1 )   49 - 68   1997

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    Under a model of altitude distribution of the Alfvén speed VA, one-dimensional transient response of the inner magnetosphere at the magnetic equator to earthward propagating impulse- and step-like MHD disturbances is considered. The waveforms of transient compressional oscillations due to these disturbances at some L shells are directly simulated by a numerical inversion of the Laplace transform with orthonormal Laguerre functions. The present paper concentrates on the analysis of waveforms. Then, it is verified that the compressional oscillations are due to the poles of the system under consideration. The oscillation arising from the cavity resonance all over the inner magnetosphere is most dominant. However, its amplitude becomes smaller as the characteristic time scale T of an incident disturbance grows large, and it is negligibly small for T greater than several times of eigenperiod of the resonance. On the other hand, when T is relatively small (e.g., T ≲ 10 s), the oscillations due to the cavity resonances trapped around the trough in VA are outstanding. It is also found that the relative phase between the cavity-mode oscillations all over the inner magnetosphere at the earth's surface and another L shell increases monotonically with L when the inner magnetosphere has no strong gradient or a strong positive gradient of VA at its outer boundary. However, the relative phase is nearly zero and nearly 180° inside and outside a specific L shell, respectively, when the inner magnetosphere has a strong negative gradient at its outer boundary. The one-dimensional cavity-mode type resonance of the inner magnetosphere is certainly a cause of equatorial Pi2 pulsations. However, some constituents of the Pi2's may be not cavity-mode oscillations but quasi-steady-state oscillations forced by some damped sinusoidal waves incident on the outer boundary of the inner magnetosphere.

  • Reflection of shear Alfvén waves at the ionosphere and the divergent Hall current

    A. Yoshikawa, A. Yoshikawa, M. Itonaga, M. Itonaga

    Geophysical Research Letters   23 ( 1 )   101 - 104   1996.1

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    Reflection of shear Alfvén waves at the ionosphere and the divergent Hall current
    A general expression for the reflection and mode conversion of MHD waves at the ionosphere is derived. On the basis of the expression, the effect of ionospheric divergent Hall current (Hall part of the induction current associated with the inductive electric field of fast magnetosonic wave) on localized toroidal oscillation is examined. When the horizontal scale of localized oscillation is of the order of several times of the height of ionosphere, the inductive electric field can play a significant role in the reflection of shear Alfvén waves with longer periods (e.f., - 100 s) in the high-latitude region, especially, in the auroral zone. Then, the contribution of the divergent Hall current to the field-aligned one can be no longer neglected and so the eigenfrequency of localized toroidal oscillation is effectively controlled by the height-integrated Hall conductivity in the ionosphere.

    DOI: 10.1029/95GL03580

  • Reflection of shear Alfven waves at the ionosphere and the divergent Hall current Reviewed

    A Yoshikawa, M Itonaga

    GEOPHYSICAL RESEARCH LETTERS   23 ( 1 )   101 - 104   1996.1

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    A general expression for the reflection and mode conversion of MHD waves at the ionosphere is derived. On the basis of the expression, the effect of ionospheric divergent Hall current (Hall part of the induction current associated with the inductive electric field of fast magnetosonic wave) on localized toroidal oscillation is examined. When the horizontal scale of localized oscillation is of the order of several times of the height of ionosphere, the inductive electric field can play a significant role in the reflection of shear Alfven waves with longer periods (e.g., similar to 100 s) in the high-latitude region, especially, in the auroral zone. Then, the contribution of the divergent Hall current to the field-aligned one can be no longer neglected and so the eigenfrequency of localized toroidal oscillation is effectively controlled by the height-integrated Hall conductivity in the ionosphere.

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Books

  • Earth's ionosphere Theory and phenomenology of cowling channels

    Akimasa Yoshikawa, Ryoichi Fujii(Role:Joint author)

    wiley  2018.4 

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    The Cowling channel is a generic name of a current system forming inside a high conductivity band in which a secondary polarization electric field modifies the current flow. The polarization field is excited when a divergent part of Hall current driven by the primary electric field is prevented from flowing out to the magnetosphere as the field-aligned current. The purpose of this chapter is to review the recent development of the Cowling channel model. Recent work provides an extension of the theoretical description of the classical Cowling channel with respect to the following aspects: (1) taking into account the 3D nature of the ionosphere by introducing two current layers at different altitudes, and (2) considering finite length of the Cowling channel by introducing a conductance boundary not only at the meridional borders of the Cowling channel, but also at its zonal boundaries. Using this improved model, we discuss current closure and the energy principle for evolution of the Cowling channel. Energy flow inside the Cowling channel and impact of the polarization effect on Joule dissipation in the more general M-I coupling scheme are also provided. We also clarify how shear Alfvén waves interact to the Cowling channel and their application to the global magnetosphere- ionosphere coupling simulations.

    DOI: 10.1002/9781119324522.ch25

  • Earth’s Ionosphere: Theory and Phenomenology of Cowling Channels, in Electric Currents in Geospace and Beyond

    Yoshikawa A. and R. Fujii(Role:Joint author)

    John Wiley & Sons, Inc, Hoboken, N.J.  2018.4 

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    The Cowling channel is a generic name of a current system forming inside a high conductivity band, in which a secondary polarization electric field modifies the current flow. The polarization field is excited when a divergent part of Hall current driven by the primary electric field is prevented from flowing out to the magnetosphere as the field-aligned current (FAC). The Cowling effect is now well known as enhancement of current flow in the direction of the primary electric field by the secondary Hall current [Chapman, 1956]. The Cowling effect was first investigated by Cowling [1932] in connection with the solar atmosphere. The generation mechanism [Cowling and Boreger, 1948] was adopted to account for equatorial electrojet [Hirono, 1950, Untied, 1967] and auroral electrojet [Boström, 1964]. The Cowling effect has been investigated theoretically and observationally [e.g., Baujohann, 1983; Yasuhara et al., 1985; Haerendel, 2008, Amm et al., [2008]; Amm and Fujii, 2008; Marghitu et al., 2011]. Figure 1 shows traditional picture of two-dimensional Cowling channel model elongated along east-west direction [e.g., Baumjohann, 1983], in which ionospheric Hall and Pedersen conductivity are height-integrated. The primary westward electric field (E1) drives northward Hall current and westward Pedersen current. The southward secondary field (E2) is generated so that the Pedersen current closes the primary Hall current between the conductivity gradients. The secondary Hall current flows in the same direction as the primary Pedersen current and forms the electrojet system. Generally, it is difficult to specify polarization effects in the ionosphere from ground-based data alone. These data only allow to infer the resultant total electrodynamic fields, but cannot track back the chain of cause and consequence that led to the physical situation which then causes these observed total fields. Thus, using ground-based data alone in most cases we can only state whether an observed situation is consistent or not with the expectations from an “active” polarization effect. To quantify the Cowling effect, we need to know the relative strength of the polarization electric field to total electric field and to what extent it cancels (closes) the primary Hall current. This problem is complementary to the question: How much curl-free Hall current flows out to the magnetosphere as FAC? In order to reply to this problem provided by Amm et al., [2008], modeling of Cowling channel has been further developed. To describe the Cowling channel, Amm et al., [2011] and Fujii et al., [2011] introduce a parameter called the Cowling efficiency. It is defined as a ratio how much of Hall current is confined inside the ionosphere by the secondary Pedersen current excited by the polarization electric field. Definition of Cowling efficiency is practically important. It provides a general way to calculate quantitatively the polarization electric field, if the Cowling efficiency, the conductance, and either primary or the total electric fields are known [Amm et al., 2013]. It has been suggested that to identify the Cowling efficiency for specific phenomenon, one needs to know the impedance of the magnetospheric circuit, which completes the current circuit in the M-I system via FAC [e.g., Fujii et al., 2011]. However, it is questionable to assign a magnetospheric impedance for steady state because the M-I system is always changing dynamically. The M-I coupling process via shear Alfven waves has been used to investigate the nonstationary FAC closure by ionospheric conducting current [e.g., Scholer, 1970]. Assuming specific electric field configurations of an incident wave, Glaβmeier [1983] and Itonaga and Kitamura [1988] have shown that a secondary polarization field due to gradients of Hall conductance can appear in the reflected wave. Actually, the Alfven wave approach can be used to describe not only local and dynamical phenomena but also more generally global quasi-static M-I coupling processes [Yoshikawa et al., 2010]. Therefore it is very important to understand the how the shear Alfven wave interacts with the Cowling channel. Yoshikawa et al., [2011a] give a general theory about M-I coupling, independent of specific geometries or specific situations. This theory, based on the Alfven waves used in a way of a basis function for the M-I coupling process, is later applied in Yoshikawa et al., [2013a] and Yoshikawa et al., [2013b] specifically to a Cowling channel situation, but can be applied for any general case. Most of Cowling channel models introduced so far rely on a thin-sheet ionosphere [e.g., Baujohann, 1983]. However, in a realistic ionospheric E-layer, a vertical distribution of the Pedersen conductivity and Hall conductivity has maximum peak around 125 km altitude and around 110 km altitude, respectively [e.g., Richmond and Thayer, 2000]. In order properly consider the ionospheric current closure, one also takes into account the ionospheric thickness [Amm et al., 2008]. One step in this direction is to assume that the Pedersen and Hall current flow thin layers at different altitudes [Fujii et al., 2011; Amm et al., 2011; Yoshikawa et al., 2011]. The classical picture illustrated in Figure 1 describes divergence-free approximation of auroral electrojet. However, a longitudinal boarder of Cowling channel is also important for considering finite aurora arc formation and Harang reversal region [Harang, 1947; Heppner, 1972; Marghitu et al., 2011], where the auroral electrojet is diverging. Amm et al., [2008] give a review of the work available in the literature until 2008 regarding following aspects of ionospheric electrodynamics and Magnetosphere-Ionosphere (M-I) coupling: -Polarization effect in the ionosphere (often referred to as “Cowling effect)” -Inductive effect in the ionosphere -The effect of the three-dimensional (3D) nature of the ionosphere for ionospheric electrodynamics -The consequences of the above mentioned aspects to M-I coupling. Marghitu, [2012] provides an excellent review for auroral arc electrodynamics, by considering the 1D thin uniform arc, the 2D thick uniform arc, and the non-uniform arc. The various arc features are assembled together in a tentative 3D arc model. The purpose of this chapter is to review the recent development of Cowling channel model after Amm et al., [2008] and Marghitu, [2012]. Recent work provide an extension of theoretical description of the classical Cowling channel with respect to the following aspects: 1) Taking into account the 3D nature of ionosphere by introducing two current layers at different altitudes, and 2) considering finite length of the Cowling channel by introducing a conductance boundary not only at the meridional borders of Cowling channel, but also at its zonal boundaries. Using this improved model, schematically illustrated in Figure 2 with Cowling efficiency description, we discuss current closure and their energy principle for evolution of Cowling channel. Energy flow inside the Cowling channel and impact of polarization effect on Joule dissipation in more general M-I coupling scheme are also provided. In addition, we also clarify how shear Alfven wave interacts to the Cowling channel and their application to the global magnetosphere-ionosphere coupling simulations.

    DOI: 10.1002/9781119324522.ch25

  • Resonant Cavities and Waveguides in the Ionosphere and Atmosphere, Magnetospheric ULF Waves: Synthesis and New Directions

    Lysak, R. L. and A. Yoshikawa(Role:Joint author)

    AGU, Washington, D. C.  2006.12 

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Presentations

  • 宇宙プラズマシミュレーションのための量子アルゴリズム

    #樋口颯人, J. W. Pedersen, @吉川顕正

    九州大学 量子ネイティブ育成 研究シンポジウム  2024.1 

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    Event date: 2024.1

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学 稲盛財団記念館 稲盛ホール   Country:Japan  

  • 宇宙プラズマシミュレーションのための量子アルゴリズム

    樋口颯人, J. W. Pedersen, 吉川顕正

    九州大学 量子ネイティブ育成 研究シンポジウム  2024.1 

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    Event date: 2024.1

    Language:Japanese  

    Venue:九州大学 稲盛財団記念館 稲盛ホール   Country:Japan  

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  • 量子特異値変換を使ったVlasov-Maxwell系の量子計算アルゴリズムの再構築

    #樋口颯人, J. W. Pedersen, 黄海仲星, 吉川耕司, @吉川顕正

    STEシミュレーション研究会・KDKシンポジウム合同研究会  2023.12 

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    Event date: 2023.12

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:神戸大学瀧川記念学術交流会館   Country:Japan  

  • 量子特異値変換を使ったVlasov-Maxwell系の量子計算アルゴリズムの再構築

    樋口颯人, J. W. Pedersen, 黄海仲星, 吉川耕司, 吉川顕正

    STEシミュレーション研究会・KDKシンポジウム合同研究会  2023.12 

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    Event date: 2023.12

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    Venue:神戸大学瀧川記念学術交流会館   Country:Japan  

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  • Quasi-6-Day Wave Variation on the Inter-Hemispheric Field-Aligned Currents (IHFACs) Invited International conference

    #Takayama Kumi, @Yoshikawa Akimasa, @Miyoshi Yasunobu

    American Geophysical Union Fall Meeting 2023  2023.12 

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    Event date: 2023.12

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    Venue:San Francisco   Country:United States  

  • Quantum Calculation for Kinetic Multi-scale Auroral Mechanism: A Novel Approach to Numerical Analysis from Kinetic Alfvén Wave Scales to MHD Scales Invited International conference

    #Higuchi, H, J. W. Pedersen and @A. Yoshikawa

    American Geophysical Union Fall Meeting 2023  2023.12 

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    Event date: 2023.12

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    Venue:San Francisco   Country:United States  

    プラズマのマルチスケール結合が本質となるオーロラ物理学について、量子アルゴリズムの適用可能性と、そのロードマップについて議論を行う。

  • Development of Affine Connection for Describing Spatiotemporal Evolving 3D Magnetic Vector Fields and its Applications Invited International conference

    @Akimasa Yoshikawa

    American Geophysical Union Fall Meeting 2023  2023.12 

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    Venue:San Francisco   Country:United States  

  • Investigating the mechanism of electric field penetration during isolated substorms using a ground-based multi-point magnetic and electric field network Invited International conference

    #Hayashi, M., @A. Yoshikawa, A. Fujimoto, S. Ohtani

    American Geophysical Union Fall Meeting 2023  2023.12 

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    Venue:San Francisco   Country:United States  

  • Development of Affine Connection for Describing Spatiotemporal Evolving 3D Magnetic Vector Fields and its Applications Invited International conference

    Akimasa Yoshikawa

    American Geophysical Union Fall Meeting 2023  2023.12 

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    Venue:San Francisco   Country:United States  

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  • Quantum Calculation for Kinetic Multi-scale Auroral Mechanism: A Novel Approach to Numerical Analysis from Kinetic Alfvén Wave Scales to MHD Scales Invited International conference

    Higuchi, H, J. W. Pedersen and A. Yoshikawa

    American Geophysical Union Fall Meeting 2023  2023.12 

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    Event date: 2023.12

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    Venue:San Francisco   Country:United States  

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  • A Novel Application of Nonlinear PDEs Quantum Algorithms: Toward Large-Scale Space Plasma Simulations International conference

    #Higuchi, H, J. W. Pedersen and @A. Yoshikawa

    10th International Workshop of Quantum Simulation and Quantum Walks  2023.11 

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    Event date: 2023.11

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    Venue:つくば国際会議場   Country:Japan  

  • A Novel Application of Nonlinear PDEs Quantum Algorithms: Toward Large-Scale Space Plasma Simulations International conference

    Higuchi, H, J. W. Pedersen and A. Yoshikawa

    10th International Workshop of Quantum Simulation and Quantum Walks  2023.11 

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    Event date: 2023.11

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    Venue:つくば国際会議場   Country:Japan  

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  • 主成分分析を用いた地上磁場からの半球間沿磁力線電流(IHFACs)成分の抽出, 太陽地球系物理学分野のデータ解析手法、ツールの理解と応用 Invited

    #高山久美, @吉川顕正, @三好勉信

    IUGONET合同研究集会、太陽地球系物理学分野のデータ解析手法、ツールの理解と応用  2023.11 

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    Event date: 2023.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学生存圏研究所   Country:Japan  

  • Quantum Calculation of Classical Kinetic Equations: A Novel Approach for Numerical Analysis of 6D Boltzmann-Maxwell Equations in Collisionless Plasmas Using Quantum Computing

    #樋口颯人, J. W. Pedersen, @吉川顕正

    場の理論の新しい計算方法2023 量子計算とテンソルネットワークに関するスクール  2023.10 

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    Event date: 2023.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:大阪大学豊中キャンパス 南部ホール   Country:Japan  

  • Quantum Calculation of Classical Kinetic Equations: A Novel Approach for Numerical Analysis of 6D Boltzmann-Maxwell Equations in Collisionless Plasmas Using Quantum Computing

    樋口颯人, J. W. Pedersen, 吉川顕正

    場の理論の新しい計算方法2023 量子計算とテンソルネットワークに関するスクール  2023.10 

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    Event date: 2023.10

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    Venue:大阪大学豊中キャンパス 南部ホール   Country:Japan  

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  • Large-scale research project in Japan, "Study of coupling processes in the Solar-Terrestrial system” Invited International conference

    @A. Yoshikawa, M. Yamamoto, Y. Ogawa, K. Shiokawa, K. Iwai, H. Hashiguchi, T. Yokoyama, S. Nozawa, Y. Ohtsuka, A. Shinbori, Y. Tanaka, @S. Abe

    AOSWA 2023  2023.10 

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    Event date: 2023.10

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    Venue:Bangi   Country:Malaysia  

  • Analysis of substorms using ground-based magnetic and electric field network: results and challenges for space weather forecasting International conference

    #Hayashi, M., @A. Yoshikawa, A. Fujimoto, S. Ohtani

    AOSWA 2023  2023.10 

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    Venue:Bangi   Country:Malaysia  

  • Mid-latitude Ground Magnetic and Electric Field Responses Associated with SCW Development during Substorms International conference

    #Hayashi, M., @A. Yoshikawa, A. Fujimoto, S. Ohtani

    IconSpace 2023  2023.10 

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    Venue:Penang   Country:Malaysia  

  • Schumann resonance parameters at Kuju and global lightning activity

    Akihiro Ikeda, @Teiji Uozumi, @Akimasa Yoshikawa, Akiko Fujimoto, @Shuji Abe

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • 大型研究プロジェクト「太陽地球系結合過程の研究基盤形成」

    山本衛, 小川泰信, 塩川和夫, @吉川顕正, 岩井一正

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • 630-nm大気光増光の3地点同時観測に基づくサブストームに伴う中緯度への電場侵入の複数例解析

    森田早紀, 塩川和夫, 大塚雄一, 西谷望, 新堀淳樹, 惣宇利卓弥, 藤本晶子, @吉川顕正, 西岡未知, PERWITASARISEPTI, 山本衛

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • 特異的減少傾向を持つ赤道ジェット電流の発生特性について

    #池末暉, 吉川顕正, @藤本晶子

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東北大学青葉山キャンパス   Country:Japan  

  • 半球間沿磁力線電流(IHFAC)に現れる準6日波の変動

    #高山久美, @吉川顕正, @三好 勉信

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • プラズマバブル発生に関するCEJの影響

    #加藤彰紘, @吉川顕正, 藤本晶子

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • ペナルティ付き動体検出に基づいた時系列イオノグラム画像における電離圏エコー抽出モデルの開発

    廣重優, 藤本晶子, 池田昭大, @阿部修司, @吉川顕正

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • ELF電磁波観測によるスプライトがグローバルサーキットに与える影響に関する研究

    #古谷享一, @吉川顕正, 池田昭大

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • Scattered perpendicular flow speed in the dayside reconnection regions due to change in the IMF Bz direction

    #Tsubasa Hashimoto, @Akimasa Yoshikawa, @Takashi Tanaka

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • Evolution of M-I convection depending on the Alfven conductance as simulated by global MHD model with Alfvenic coupling

    Aoi Nakamizo, @Akimasa Yoshikawa, Hiroyuki Nakata, Keiichiro Fukazawa,@Takashi Tanaka

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東北大学青葉山キャンパス   Country:Japan  

  • Development of Affine connections to describe 3D evolving magnetic vector fields and its application to space physics

    @Akimasa Yoshikawa

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • Severe erosion of the plasmasphere caused by the ring current particle injection into the deep inner magnetosphere

    @Yuki Obana, @Akimasa Yoshikawa, Naomi Maruyama, 他17名

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • サブストームに伴うPi2及びPc4脈動の発生特性について

    #橋本明史, @吉川顕正, @魚住禎司

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • 3次元衝突性HallMHDシミュレーションを用いたオーロラ加速領域における電磁場構造の解析

    #川上航典, @吉川顕正, 深沢圭一郎

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東北大学青葉山キャンパス   Country:Japan  

  • Multi-spacecraft observations of widespread solar proton transport in the heliosphere

    Takahiro Obara, @Akimasa Yoshikawa

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • 量子コンピュータシミュレータQiskitを用いた無衝突プラズマ6次元BoltzmannMaxwell系のセルフコンシステントな量子計算アルゴリズムの開発

    #樋口颯人,ピダーセン珠杏,@吉川顕正

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Venue:東北大学青葉山キャンパス   Country:Japan  

  • The Impact of the Geomagnetic Storm Event of February 2022 on the Inner Radiation Belt by Test Particle Simulations

    @Kirolosse Girgis1, @Tohru Hada, @Shuichi Matsukiyo, @Akimasa Yoshikawa, Abraham Chian

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東北大学青葉山キャンパス   Country:Japan  

  • 孤立型サブストーム時のCW構造の発達に応じた、中低緯度電場応答の研究

    #林萌英, @吉川顕正

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東北大学青葉山キャンパス   Country:Japan  

  • Geomagnetic Field Observation Project by YOTSUBA-KULOVER Satellite with COTS Magnetometer

    Kentarou Kitamura, Hirokazu Masui, @Shuji Abe ,T@eiji Uozumi, Mariko Teramoto, Akiko Fujimoto, Kei Sano, @Akimasa Yoshikawa, Mengu Cho

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東北大学青葉山キャンパス   Country:Japan  

  • 文字列照合等を用いた赤道ジェット電流地磁気変動の特性抽出とその応用

    #西口稜真, @吉川顕正, 藤本晶子

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東北大学青葉山キャンパス   Country:Japan  

  • 孤立型サブストーム時のCW構造の発達に応じた、中低緯度電場応答の研究

    林萌英, 吉川顕正

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

    Language:Japanese  

    Venue:東北大学青葉山キャンパス   Country:Japan  

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  • Geomagnetic Field Observation Project by YOTSUBA-KULOVER Satellite with COTS Magnetometer

    Kentarou Kitamura, Hirokazu Masui, Shuji Abe, Teiji Uozumi, Mariko Teramoto, Akiko Fujimoto, Kei Sano, Akimasa Yoshikawa, Mengu Cho

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

    Language:Japanese  

    Venue:東北大学青葉山キャンパス   Country:Japan  

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  • 3次元衝突性HallMHDシミュレーションを用いたオーロラ加速領域における電磁場構造の解析

    川上航典, 吉川顕正, 深沢圭一郎

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

    Language:Japanese  

    Venue:東北大学青葉山キャンパス   Country:Japan  

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  • 量子コンピュータシミュレータQiskitを用いた無衝突プラズマ6次元BoltzmannMaxwell系のセルフコンシステントな量子計算アルゴリズムの開発

    樋口颯人, ピダーセン珠杏, 吉川顕正

    地球電磁気・地球惑星圏学会第154 回総会・講演会  2023.9 

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    Event date: 2023.9

    Language:Japanese  

    Venue:東北大学青葉山キャンパス   Country:Japan  

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  • Quantum numerical computation of the classical kinetic equation by quantum computer: new method for the Boltzmann equation in 6D collisionless plasma International conference

    #Higuchi, H, J. W. Pedersen and @A. Yoshikawa

    Union Radio-Scientifique Internationale GASS 2023  2023.8 

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    Event date: 2023.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:SAPPORO   Country:Japan  

  • Quantum numerical computation of the classical kinetic equation by quantum computer: new method for the Boltzmann equation in 6D collisionless plasma International conference

    Higuchi, H, J. W. Pedersen and A. Yoshikawa

    Union Radio-Scientifique Internationale GASS 2023  2023.8 

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    Event date: 2023.8

    Language:English  

    Venue:SAPPORO   Country:Japan  

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  • Clarification of Atmospheric Tidal Modes Appearing in Ionospheric Currents by Independent Component Analysis Invited International conference

    #Takayama Kumi, @Yoshikawa Akimasa, @Miyoshi Yasunobu

    AOGS 2023 20th Annual Meeting  2023.8 

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    Event date: 2023.7 - 2023.8

    Language:English   Presentation type:Oral presentation (general)  

    Country:Singapore  

  • Statistical Study of Mid- and Low-latitude Electric Field Response Corresponding to the CW Structure That Develops During Substorms Invited International conference

    #Hayashi, M., @A. Yoshikawa, A. Fujimoto, S. Ohtani

    AOGS 2023 20th Annual Meeting  2023.8 

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    Event date: 2023.7 - 2023.8

    Language:English   Presentation type:Oral presentation (general)  

    Country:Singapore  

  • On the electron acceleration process as a carrier of field-aligned current and its energy conversion process in the Alfvén wavefront International conference

    @Akimasa Yoshikawa

    AGU Chapman Conference on Advances in Understanding Alfvén Waves in the Sun and the Heliosphere  2023.5 

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    Event date: 2023.5 - 2023.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Berlin   Country:Germany  

  • Ionospheric role in the development of the M-I coupled convection system: generation of Alfvénic disturbances from the ionospheric convection field deformed by conductance non-uniformity Invited International conference

    Aoi Nakamizo, @Akimasa Yoshikawa, Hiroyuki Nakata, Keiichiro Fukazawa

    AGU Chapman Conference on Advances in Understanding Alfvén Waves in the Sun and the Heliosphere  2023.5 

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    Event date: 2023.5 - 2023.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Berlin   Country:Germany  

  • Latest activities of i-SPES & Kyutech FM-CW project International conference

    藤本晶子, @阿部修司, @吉川顕正, 池田昭大, 廣重優, 中村 駿仁

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 量子コンピュータによる6次元無衝突プラズマの古典運動論的方程式の量子数値計算 International conference

    #樋口颯人, Pedersen Juan, @吉川 顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 独立成分分析を用いた大気潮汐によって励起される磁場変動の抽出 International conference

    #高山久美, @吉川顕正, @三好勉信

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • あらせ観測に基づいた二つの中規模磁気嵐におけるリングカレントイオンと電子フラックスの比較研究 International conference

    @尾花由紀, @吉川顕正, 丸山奈緒美, 他17名

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Extraction of ionospheric echoes for time series Ionograms International conference

    廣重優, 藤本晶子, @阿部修司, 池田昭大, @吉川顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • サブストーム時に発達するCW構造に応じた、中低緯度電場応答の統計的研究 International conference

    #林萌英, @吉川顕正, 藤本晶子, 大谷 晋一

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Characteristics of the IHFAC derived from the Complementary Geomagnetic Field Observations by the Satellite and Ground Stations International conference

    北村健太郎, 藤本晶子, 寺本万里子, @吉川顕正, @阿部修司

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 日本の地上観測点に基づくサブストームに伴う630-nm大気光増光の複数例解析 International conference

    森田早紀, 塩川和夫, 大塚雄一, 新堀淳樹, 惣宇利卓弥, 藤本晶子, @吉川顕正, 西岡未知, Perwitasari Septi

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Ionospheric role in the development of the M-I convection system: generation of Alfvénic disturbances from the ionospheric convection field deformed by conductance non-uniformity International conference

    中溝葵, @吉川顕正, 中田裕之, 深沢圭一郎, @田中高史

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Development of Affine Connection for Describing Spatiotemporal Evolving 3D Magnetic Vector Fields and its applications International conference

    @吉川顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 大型研究プロジェクト「太陽地球系結合過程の研究基盤形成」 International conference

    山本衛, 小川泰信, 塩川和夫, @吉川顕正, 岩井一正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • The Causality of Electromagnetic Channel Formation in the Ionosphere from Polar to Equatorial Regions International conference

    @吉川顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Recent activities of i-SPES and MAGDAS project International conference

    @阿部修司, 藤本晶子, 池田昭大,@魚住禎司, @吉川顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 日本の地上観測点に基づくサブストームに伴う630-nm大気光増光の複数例解析 International conference

    森田早紀, 塩川和夫, 大塚雄一, 新堀淳樹, 惣宇利卓弥, 藤本晶子, 吉川顕正, 西岡未知, Perwitasari Septi

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • サブストーム時に発達するCW構造に応じた、中低緯度電場応答の統計的研究 International conference

    林萌英, 吉川顕正, 藤本晶子, 大谷 晋一

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • あらせ観測に基づいた二つの中規模磁気嵐におけるリングカレントイオンと電子フラックスの比較研究 International conference

    尾花由紀, 吉川顕正, 丸山奈緒美, 他17名

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • The Causality of Electromagnetic Channel Formation in the Ionosphere from Polar to Equatorial Regions International conference

    吉川顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • Recent activities of i-SPES and MAGDAS project International conference

    阿部修司, 藤本晶子, 池田昭大, 魚住禎司, 吉川顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • Latest activities of i-SPES & Kyutech FM-CW project International conference

    藤本晶子, 阿部修司, 吉川顕正, 池田昭大, 廣重優, 中村 駿仁

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • Ionospheric role in the development of the M-I convection system: generation of Alfvénic disturbances from the ionospheric convection field deformed by conductance non-uniformity International conference

    中溝葵, 吉川顕正, 中田裕之, 深沢圭一郎, 田中高史

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • Extraction of ionospheric echoes for time series Ionograms International conference

    廣重優, 藤本晶子, 阿部修司, 池田昭大, 吉川顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • Development of Affine Connection for Describing Spatiotemporal Evolving 3D Magnetic Vector Fields and its applications International conference

    吉川顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • Characteristics of the IHFAC derived from the Complementary Geomagnetic Field Observations by the Satellite and Ground Stations International conference

    北村健太郎, 藤本晶子, 寺本万里子, 吉川顕正, 阿部修司

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • 量子コンピュータによる6次元無衝突プラズマの古典運動論的方程式の量子数値計算 International conference

    樋口颯人, Pedersen Juan, 吉川 顕正

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • 独立成分分析を用いた大気潮汐によって励起される磁場変動の抽出 International conference

    高山久美, 吉川顕正, 三好勉信

    日本地球惑星科学連合2023年大会  2023.5 

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    Event date: 2023.5

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • Statistical study of mid- and low-latitude electric field response corresponding to the CW structure that develops during substorms

    #林萌英・@吉川顕正・藤本 晶子・S.Ohtani

    2022 年度国立極地研究所・名古屋大学宇宙地球環境研究所研究集会・ SuperDARN 研究集会  2023.3 

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    Event date: 2023.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所、東京都立川市   Country:Japan  

  • 量子コンピュータによる古典運動論的方程式の量子数値計算:6 次元無衝突プラズマの Boltzmann-Maxwell 方程式の新計算手法

    #樋口颯人, J. W. Pedersen, @吉川顕正

    STE シミュレーション研究会・KDK シンポジウム合同研究会  2023.3 

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    Event date: 2023.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Country:Japan  

  • 量子コンピュータによる古典運動論的方程式の量子数値計算:6 次元無衝突プラズマの Boltzmann-Maxwell 方程式の新計算手法

    樋口颯人, J. W. Pedersen, 吉川顕正

    STE シミュレーション研究会・KDK シンポジウム合同研究会  2023.3 

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    Event date: 2023.3

    Language:Japanese  

    Country:Japan  

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  • Statistical study of mid- and low-latitude electric field response corresponding to the CW structure that develops during substorms

    林萌英・吉川顕正・藤本 晶子・S.Ohtani

    2022 年度国立極地研究所・名古屋大学宇宙地球環境研究所研究集会・ SuperDARN 研究集会  2023.3 

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    Event date: 2023.3

    Language:Japanese  

    Venue:国立極地研究所、東京都立川市   Country:Japan  

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  • Research on the electromagnetic response of mid and low latitudinal region to the spatio-temporal development of CW during substorms International conference

    #M. Hayashi, @A.Yoshikawa, A.Fujimoto, S.Ohtani

    AGU Fall Meeting 2022  2022.12 

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    Event date: 2022.12 - 2023.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Chicago   Country:United States  

  • Clarification of Atmospheric Tidal Modes Appearing in Ionospheric Currents by Principal Component Analysis International conference

    #Takayama Kumi, @Yoshikawa Akimasa, and @Miyoshi Yasunobu

    AGU Fall Meeting 2022  2022.12 

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    Event date: 2022.12 - 2023.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Chicago   Country:United States  

  • Clarification of Atmospheric Tidal Modes Appearing in Ionospheric Currents by Principal Component Analysis International conference

    Takayama Kumi, Yoshikawa Akimasa, and Miyoshi Yasunobu

    AGU Fall Meeting 2022  2022.12 

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    Event date: 2022.12 - 2023.12

    Language:English  

    Venue:Chicago   Country:United States  

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  • Research on the electromagnetic response of mid and low latitudinal region to the spatio-temporal development of CW during substorms International conference

    M. Hayashi, A.Yoshikawa, A.Fujimoto, S.Ohtani

    AGU Fall Meeting 2022  2022.12 

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    Event date: 2022.12 - 2023.12

    Language:English  

    Venue:Chicago   Country:United States  

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  • Current Status and Challenges in M-I Coupling Research Invited International conference

    @A.Yoshikawa

    Prof.Kamide Memorial Symposium  2022.11 

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    Event date: 2022.11 - 2023.11

    Language:English   Presentation type:Oral presentation (general)  

    Venue:名古屋大学野依学術記念館   Country:Japan  

  • Current Status and Challenges in M-I Coupling Research Invited International conference

    A.Yoshikawa

    Prof.Kamide Memorial Symposium  2022.11 

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    Event date: 2022.11 - 2023.11

    Language:English  

    Venue:名古屋大学野依学術記念館   Country:Japan  

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  • Development of Quantum Algorithm for Clarifying Auroral Electron Acceleration Mechanism by Collisional Boltzmann-Maxwell Equation

    #樋口 颯人, @吉川 顕正

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:相模原市立産業会館   Country:Japan  

  • 時空発展する3次元磁場ベクトル場記述のためのアフィン接続

    @吉川 顕正

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:English   Presentation type:Oral presentation (general)  

    Venue:2022年11月3〜4日,相模原市立産業会館   Country:Japan  

  • 主成分分析による磁場水平ベクトルの解明

    #高山 久美, @吉川 顕正

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:English   Presentation type:Oral presentation (general)  

    Venue:2022年11月3〜4日,相模原市立産業会館   Country:Japan  

  • Evolution of electrostatic potential in magnetosphere-ionospheric system as simulated by global MHD model with Alfvenic-coupling

    Aoi Nakamizo, Akimasa @Yoshikawa, Hiroyuki Nakata, Keiichiro Fukazawa,@Takashi Tanaka

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:2022年11月3〜4日,相模原市立産業会館   Country:Japan  

  • 高緯度帯でのAlfven波を介したM-I結合系の記述;分極、誘導効果、伝導度発展による複合効果の探査

    #森澤 将, @吉川 顕正

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:2022年11月3〜4日,相模原市立産業会館   Country:Japan  

  • How is stacked northward IMF removed from the dayside magnetosheath region due to the southward IMF reversal?

    #橋本 翼, @吉川 顕正, @田中 高史

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:2022年11月3〜4日,相模原市立産業会館   Country:Japan  

  • 太陽-地球方向を向いた惑星間空間磁場に対する地球磁気圏の応答研究

    #城戸 蓮太郎, @吉川 顕正, @魚住 禎司,

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:2022年11月3〜4日,相模原市立産業会館   Country:Japan  

  • IGRFモデルおよび準3次元ポテンシャルソルバーを用いたM-I結合系におけるEEJ変動の構造解析

    #伊集院拓也,@吉川顕正,@三好 勉信, 品川 裕之, 藤原 均, 陣 英克, 中溝 葵, 垰 千尋, 塩川 和夫

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:2022年11月3〜4日,相模原市立産業会館   Country:Japan  

  • サブストーム時のCW発達に伴う中緯度領域/地上磁場・電場観応答の考察

    #林 萌英, @吉川 顕正, 藤本 晶子

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:2022年11月3〜4日,相模原市立産業会館   Country:Japan  

  • Eastward Magnetic Variations in the Equatorial Latitude Associated with the IHFAC Observed on the Ground and LEO

    北村 健太郎, 藤本 晶子, 寺本 万里子, @吉川 顕正, @阿部 修司

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:2022年11月3〜7日,相模原市立産業会館   Country:Japan  

  • How do the geomagnetic storms affect the LEO proton flux distribution during Solar Energetic Particle events?

    @Kirolosse Girgis, @Tohru Hada, @Akimasa Yoshikawa, @Shuichi Matsukiyo, Joseph Lemaire, Viviane Pierrard, Samwel Susan

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:相模原市立産業会館   Country:Japan  

  • FMCWイオノグラム画像E/Es層エコー検出に関する一般物体検出モデルの高有効性

    廣重 優, 藤本 晶子, @阿部 修司, 池田 昭大, @吉川 顕正

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:相模原市立産業会館   Country:Japan  

  • Schumann resonance parameters at Kuju during intense solar activity

    池田 昭大,@ 魚住 禎司, @吉川 顕正, 藤本 晶子, @阿部 修司

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:相模原市立産業会館   Country:Japan  

  • 高緯度帯でのAlfven波を介したM-I結合系の記述;分極、誘導効果、伝導度発展による複合効果の探査

    森澤 将, 吉川 顕正

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese  

    Venue:2022年11月3〜4日,相模原市立産業会館   Country:Japan  

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  • How do the geomagnetic storms affect the LEO proton flux distribution during Solar Energetic Particle events?

    Kirolosse Girgis, Tohru Hada, Akimasa Yoshikawa, Shuichi Matsukiyo, Joseph Lemaire, Viviane Pierrard, Samwel Susan

    地球電磁気・地球惑星圏学会第152 回総会・講演会  2022.11 

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    Event date: 2022.11

    Language:Japanese  

    Venue:相模原市立産業会館   Country:Japan  

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  • Quantum Algorithm for Clarifying Auroral Acceleration Mechanism by Collisional Boltzmann-Maxwell Equation

    #樋口 颯人, @吉川 顕正

    宇宙地球惑星科学若手会夏の学校 2022  2022.9 

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    Event date: 2022.9

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:休暇村志賀島、福岡市   Country:Japan  

  • Quantum Algorithm for Clarifying Auroral Acceleration Mechanism by Collisional Boltzmann-Maxwell Equation

    樋口 颯人, 吉川 顕正

    宇宙地球惑星科学若手会夏の学校 2022  2022.9 

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    Event date: 2022.9

    Language:Japanese  

    Venue:休暇村志賀島、福岡市   Country:Japan  

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  • Principal Component Analysis for Extracting Variations due to Sq Current and Atmospheric Tides from Magnetic Field Data International conference

    #Takayama Kumi, @Yoshikawa Akimasa

    American Geophysics Union Fall Meeting 2021  2021.12 

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    Event date: 2021.12 - 2022.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:United States  

  • Electron acceleration mechanism in "ionospheric polarized Poleward Boundary Intensification": A new validation with 3-dimensional fluid electron acceleration simulators International conference

    #Higuchi, H, and @A. Yoshikawa

    American Geophysics Union Fall Meeting 2021  2021.12 

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    Event date: 2021.12 - 2022.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:United States  

  • Research on the Poler to Mid-latitude Ionospheric Response During Substorm based on mid-latitude electric field and global magnetic field observations International conference

    #M. Hayashi, @A.Yoshikawa, A.Fujimoto, S.Ohtani

    American Geophysics Union Fall Meeting 2021  2021.12 

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    Event date: 2021.12 - 2022.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:United States  

  • Electron acceleration mechanism in "ionospheric polarized Poleward Boundary Intensification": A new validation with 3-dimensional fluid electron acceleration simulators International conference

    Higuchi, H, and A. Yoshikawa

    American Geophysics Union Fall Meeting 2021  2021.12 

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    Event date: 2021.12 - 2022.12

    Language:English  

    Venue:オンライン   Country:United States  

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  • Research on the Poler to Mid-latitude Ionospheric Response During Substorm based on mid-latitude electric field and global magnetic field observations International conference

    M. Hayashi, A.Yoshikawa, A.Fujimoto, S.Ohtani

    American Geophysics Union Fall Meeting 2021  2021.12 

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    Event date: 2021.12 - 2022.12

    Language:English  

    Venue:オンライン   Country:United States  

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  • Principal Component Analysis for Extracting Variations due to Sq Current and Atmospheric Tides from Magnetic Field Data International conference

    Takayama Kumi, Yoshikawa Akimasa

    American Geophysics Union Fall Meeting 2021  2021.12 

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    Event date: 2021.12 - 2022.12

    Language:English  

    Venue:オンライン   Country:United States  

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  • 主成分分析による地上磁場データの成分分離

    #高山 久美, @吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 夜側オーロラオーバルの極側境界で発生するオーロラ増光現象における電離圏分極の数値解析

    #森澤 将, @吉川 顕正, 大谷 晋一

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 磁場・電界観測に基づく極域・中緯度電離圏の応答の解明

    #林 萌英, @吉川 顕正, 藤本 晶子, Ohtani Shinichi

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Feasibility Study of Space Weather Observation by CubeSat in LEO

    Kentarou Kitamura, Mengu Cho, @Akimasa Yoshikawa, @Teiji Uozumi, @Shuji Abe, Mariko Teramoto, Akiko Fujimoto

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Characteristics of dusk-side IHFAC polarity during storm and quiet time

    Akiko Fujimoto, @Akimasa Yoshikawa, Manjula Ranasinghe, Chandana Jayaratne

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Progress of the SDR-based dual-band scintillation detector development and its application for space weather study

    @Shuji Abe, Akiko Fujimoto, @Akimasa Yoshikawa

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Seasonal and long-term variations in the Schumann Resonance observed at Kuju Japan

    Akihiro Ikeda,@Teiji Uozumi, @Akimasa Yoshikawa, Akiko Fujimoto, @Shuji Abe

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Progress of the SDR-based dual-band scintillation detector development and its application for space weather study

    @Shuji Abe, Akiko Fujimoto, @Akimasa Yoshikawa

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Development of an autonomous FM-CW ionospheric observation system based on reinforcement learning

    Toru Mikuriya,Akiko Fujimoto,@Shuji Abe,Akihiro Ikeda,@Akimasa Yoshikawa

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 磁気赤道域における特異的な太陽フレア効果(SFE*)の発生要因の探究

    #安永 朗宏, 藤本 晶子, @吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 電離圏分極型PBIにおける電子加速メカニズム:3次元流体的電子加速シミュレータから得られる新機構

    #樋口 颯人, @吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • A study on the geometrical evolution of magnetic fields

    @Akimasa Yoshikawa

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 3次元全球電離圏静電ポテンシャルソルバーの開発

    #伊集院 拓也, @吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 磁気圏多点衛星観測時代に向けたデータ解析手法の開発

    #中村 典, @吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Implementation of Alfvenic Coupling in Global MHD Magnetosphere Simulation

    Aoi Nakamizo, @Akimasa Yoshikawa, Hiroyuki Nakata, Keiichiro Fukazawa,Takashi Tanaka,

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 夜側オーロラオーバルの極側境界で発生するオーロラ増光現象における電離圏分極の数値解析

    森澤 将, 吉川 顕正, 大谷 晋一

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese  

    Venue:オンライン   Country:Japan  

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  • 磁場・電界観測に基づく極域・中緯度電離圏の応答の解明

    林 萌英, 吉川 顕正, 藤本 晶子, Ohtani Shinichi

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese  

    Venue:オンライン   Country:Japan  

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  • 主成分分析による地上磁場データの成分分離

    高山 久美, 吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese  

    Venue:オンライン   Country:Japan  

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  • Characteristics of dusk-side IHFAC polarity during storm and quiet time

    Akiko Fujimoto, Akimasa Yoshikawa, Manjula Ranasinghe, Chandana Jayaratne

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese  

    Venue:オンライン   Country:Japan  

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  • A study on the geometrical evolution of magnetic fields

    Akimasa Yoshikawa

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese  

    Venue:オンライン   Country:Japan  

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  • 3次元全球電離圏静電ポテンシャルソルバーの開発

    伊集院 拓也, 吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese  

    Venue:オンライン   Country:Japan  

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  • 電離圏分極型PBIにおける電子加速メカニズム:3次元流体的電子加速シミュレータから得られる新機構

    樋口 颯人, 吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese  

    Venue:オンライン   Country:Japan  

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  • 磁気赤道域における特異的な太陽フレア効果(SFE*)の発生要因の探究

    安永 朗宏, 藤本 晶子, 吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese  

    Venue:オンライン   Country:Japan  

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  • 磁気圏多点衛星観測時代に向けたデータ解析手法の開発

    中村 典, 吉川 顕正

    地球電磁気・地球惑星圏学会(SGEPSS) 第150 回総会・講演会  2021.11 

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    Event date: 2021.10 - 2022.11

    Language:Japanese  

    Venue:オンライン   Country:Japan  

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  • Research for formation of global current system during substorm through observation of ionospheric response at mid-latitudinal region International conference

    #M.Hayashi, @A.Yoshikawa, A.Fujimoto, S.Ohtani,

    AOGS Annual Virtual Meeting 2021  2021.8 

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    Event date: 2021.8 - 2022.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Singapore  

  • Research on the unique Solar Flare Effect (SFE*) at the dip equator around local noon International conference

    #Yasunaga Akihiro、@Akimasa Yoshikawa, and Fujimoto Akiko

    AOGS Annual Virtual Meeting 2021  2021.8 

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    Event date: 2021.8 - 2022.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Singapore  

  • Quasi-6-Day Wave Effect on Electric Conductivity, Electric field, and Current with GAIA model International conference

    #Takayama Kumi, @Yoshikawa Akimasa, and @Miyoshi Yasunobu

    AOGS Annual Virtual Meeting 2021  2021.8 

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    Event date: 2021.8 - 2022.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Singapore  

  • Quasi-6-Day Wave Effect on Electric Conductivity, Electric field, and Current with GAIA model International conference

    Takayama Kumi, Yoshikawa Akimasa, and Miyoshi Yasunobu

    AOGS Annual Virtual Meeting 2021  2021.8 

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    Event date: 2021.8 - 2022.8

    Language:English  

    Venue:オンライン   Country:Singapore  

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  • Research on the unique Solar Flare Effect (SFE*) at the dip equator around local noon International conference

    Yasunaga Akihiro, Akimasa Yoshikawa, and Fujimoto Akiko

    AOGS Annual Virtual Meeting 2021  2021.8 

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    Event date: 2021.8 - 2022.8

    Language:English  

    Venue:オンライン   Country:Singapore  

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  • Research for formation of global current system during substorm through observation of ionospheric response at mid-latitudinal region International conference

    M.Hayashi, A.Yoshikawa, A.Fujimoto, S.Ohtani

    AOGS Annual Virtual Meeting 2021  2021.8 

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    Event date: 2021.8 - 2022.8

    Language:English  

    Venue:オンライン   Country:Singapore  

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  • Comparison of general object detection models for Ionogram sporadic E layer echoes detection International conference

    廣重 優,藤本 晶子,@阿部 修司,池田 昭大,@吉川 顕正

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Disruption of accumulated northward IMF lines in the dayside magnetosheath due to discontinuous southward turning of IMF International conference

    #橋本 翼,@吉川 顕正,#田中 高史

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 夜側オーロラオーバルの極側境界で発生するオーロラ増光現象における電離圏分極の数値解析 International conference

    #森澤 将,@吉川 顕正,大谷 晋一

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Modeling of Magnetosphere-Ionosphere-Atmosphere System to Elucidate the Coupling Process in the Space-Earth Transition Region International conference

    @吉川 顕正

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • On the electron acceleration process as a carrier of field-aligned current and its energy conversion process in the Alfvén wavefront International conference

    @吉川 顕正

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 太陽地球系結合過程の研究基盤形成 International conference

    山本衛, 小川泰信, 塩川和夫, @吉川顕正

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Evolution of electrostatic potential in magnetosphere-ionosphere system as simulated by global MHD model with Alfvénic-coupling International conference

    中溝 葵, @吉川 顕正, 中田 裕之, 深沢 圭一郎

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 朝側Pc3脈動の特徴と発生原因について International conference

    小原 隆博,@吉川 顕正,@魚住 禎司,@阿部 修司

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 衝突性3流体モデルから導かれる磁気圏-電離圏結合系の物理描像 International conference

    #樋口 颯人,@吉川 顕正

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Comparison of Magnetic Variations Associated with the IHFAC Observed on the Ground and in the LEO International conference

    北村 健太郎,藤本 晶子,@吉川 顕正,@阿部 修司,

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Control of switching two observation modes on FM-CW ionospheric observation system based on reinforcement learning International conference

    藤本 晶子,御厨 徹,@阿部 修司,池田 昭大,@吉川 顕正

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Recent activities and future plans of MAGDAS project under new organization International conference

    @阿部 修司, 藤本 晶子, @魚住禎司,@吉川 顕正

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Evolution of electrostatic potential in magnetosphere-ionosphere system as simulated by global MHD model with Alfvénic-coupling International conference

    中溝 葵, 吉川 顕正, 中田 裕之, 深沢 圭一郎

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • On the electron acceleration process as a carrier of field-aligned current and its energy conversion process in the Alfvén wavefront International conference

    吉川 顕正

    日本地球惑星科学連合2022年大会  2022.6 

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    Event date: 2021.6 - 2022.6

    Language:English  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

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  • Investigation of the mid-latitude ionospheric response during substorm based on magnetic and electric field observations International conference

    #M.Hayashi, @A.Yoshikawa, A.Fujimoto , S. Ohtani

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Study of coupling processes in the solar-terrestrial system International conference

    山本 衛、橋口 浩之、横山 竜宏、宮岡 宏、小川 泰信、塩川 和夫、野澤 悟徳、@吉川 顕正、津田 敏隆

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Generation mechanisms of plasma density irregularity from equatorial to midlatitude ionosphere during a geomagnetic storm on 21 and 22 December 2014 International conference

    惣宇利 卓弥、新堀 淳樹、大塚 雄一、津川 卓也、西岡 未知、@吉川 顕正

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • D-region ionospheric effects for 2016 eruptions of Mt. Aso using LF transmitter signals International conference

    大矢 浩代、折戸 雄飛、土屋 史紀、山本 真行、中田 裕之、@吉川 顕正

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Multiple equatorial ionospheric observation project based on FMCW radar combining MAGDAS/SDR-based scintillation detector International conference

    藤本 晶子、@阿部 修司、御厨 徹、池田 昭大、@吉川 顕正

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Development of a novel method for extracting the geometrical properties of the magnetic vector fields towards the era of multi-point satellite observations International conference

    @吉川 顕正、#橋本 翼、中溝 葵、大谷 晋一

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 太陽地球系物理学科学委員会(SCOSTEP)の活動と展望:学術会議を通した国際活動の推進 International conference

    塩川 和夫, 三好 由純, @吉川 顕正、中村 卓司

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Seasonal dependence of dusk-side equatorial IHFACs polarity during solar cycle 23-24 International conference

    ラナシンハ マンジュラ, 藤本 晶子, @吉川 顕正, ジャヤラトナ チャンダ

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Development of a new M-I coupling algorithm in global MHD magnetosphere simulation: Alfvénic-Coupling International conference

    中溝 葵, @吉川 顕正, 中田 裕之, 深沢 圭一郎, 田中 高史

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Modeling of magnetosphere-ionosphere-atmosphere system for investigation of coupling process in the space-terrestrial transition region International conference

    @Akimasa Yoshikawa

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Numerical Proton Flux Response in South Atlantic Anomaly during Geomagnetic Storm International conference

    @Kirolosse Mina Girgis, @Tohru Hada, @Shuichi Matsukiyo, @Akimasa Yoshikawa,

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 夜側オーロラオーバルの極側境界で起こるオーロラ増光現象の発生過程における電離圏分極の数値解析 International conference

    #森澤将、@吉川顕正、大谷晋一

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • IGRFモデルを用いた3次元全球電離圏静電ポテンシャルソルバーの開発 International conference

    #伊集院拓也、@吉川顕正

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Study on the Solar Flare Effect (SFE*) of equatorial electrojet around local noon International conference

    #Yasunaga Akihiro、Fujimoto Akiko、@Yoshikawa Akimasa

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Seasonal Dependence of the Quasi-6-Day Oscillation in Sq-EEJ Current System International conference

    #Takayama Kumi, @Yoshikawa Akimasa, and @Miyoshi Yasunobu

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • Exploring the Electron Acceleration Mechanism in the Poleward Boundary Intensification International conference

    #Higuchi, H. and @A. Yoshikawa,

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Japan  

  • 夜側オーロラオーバルの極側境界で起こるオーロラ増光現象の発生過程における電離圏分極の数値解析 International conference

    森澤将, 吉川顕正, 大谷晋一

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • 太陽地球系物理学科学委員会(SCOSTEP)の活動と展望:学術会議を通した国際活動の推進 International conference

    塩川 和夫, 三好 由純, 吉川 顕正, 中村 卓司

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • Development of a new M-I coupling algorithm in global MHD magnetosphere simulation: Alfvénic-Coupling International conference

    中溝 葵, 吉川 顕正, 中田 裕之, 深沢 圭一郎, 田中 高史

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

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    Venue:オンライン   Country:Japan  

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  • Study on the Solar Flare Effect (SFE*) of equatorial electrojet around local noon International conference

    Yasunaga Akihiro, Fujimoto Akiko, Yoshikawa Akimasa

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

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    Venue:オンライン   Country:Japan  

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  • Study of coupling processes in the solar-terrestrial system International conference

    山本 衛, 橋口 浩之, 横山 竜宏, 宮岡 宏, 小川 泰信, 塩川 和夫, 野澤 悟徳, 吉川 顕正, 津田 敏隆

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • Seasonal Dependence of the Quasi-6-Day Oscillation in Sq-EEJ Current System International conference

    Takayama Kumi, Yoshikawa Akimasa, and Miyoshi Yasunobu

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • Seasonal dependence of dusk-side equatorial IHFACs polarity during solar cycle 23-24 International conference

    ラナシンハ マンジュラ, 藤本 晶子, 吉川 顕正, ジャヤラトナ チャンダ

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • Numerical Proton Flux Response in South Atlantic Anomaly during Geomagnetic Storm International conference

    Kirolosse Mina Girgis, Tohru Hada, Shuichi Matsukiyo, Akimasa Yoshikawa

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • Multiple equatorial ionospheric observation project based on FMCW radar combining MAGDAS/SDR-based scintillation detector International conference

    藤本 晶子, 阿部 修司, 御厨 徹, 池田 昭大, 吉川 顕正

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • Modeling of magnetosphere-ionosphere-atmosphere system for investigation of coupling process in the space-terrestrial transition region International conference

    Akimasa Yoshikawa

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

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    Venue:オンライン   Country:Japan  

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  • Investigation of the mid-latitude ionospheric response during substorm based on magnetic and electric field observations International conference

    M.Hayashi, A.Yoshikawa, A.Fujimoto, S. Ohtani

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • IGRFモデルを用いた3次元全球電離圏静電ポテンシャルソルバーの開発 International conference

    伊集院拓也, 吉川顕正

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • Generation mechanisms of plasma density irregularity from equatorial to midlatitude ionosphere during a geomagnetic storm on 21 and 22 December 2014 International conference

    惣宇利 卓弥, 新堀 淳樹, 大塚 雄一, 津川 卓也, 西岡 未知, 吉川 顕正

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • Exploring the Electron Acceleration Mechanism in the Poleward Boundary Intensification International conference

    Higuchi, H. and A. Yoshikawa

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • Development of a novel method for extracting the geometrical properties of the magnetic vector fields towards the era of multi-point satellite observations International conference

    吉川 顕正, 橋本 翼, 中溝 葵, 大谷 晋一

    Japan GeoScience Meeting 2021  2021.6 

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    Event date: 2021.5 - 2022.6

    Language:English  

    Venue:オンライン   Country:Japan  

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  • 磁気圏電離圏結合の展開とその基礎論 Invited

    @吉川顕正

    EISCAT研究集会  2021.3 

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    Event date: 2021.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Country:Other  

  • MAGDASシステムの10Hzデータを用いた、Pc2脈動の全球的分布特性の解明

    #樺澤 大生, @吉川 顕正, @魚住 禎司, 藤本 晶子, @阿部 修司, 塩川 和夫, Connors Martin

    地球電磁気・地球惑星圏学会 第148回 総会・講演会(2020年 秋学会)  2020.11 

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    Event date: 2020.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Other  

  • 大気波動によるSq-EEJ電流系の準6日振動現象の解明

    #高山 久美, @三好 勉信, @吉川 顕正

    地球電磁気・地球惑星圏学会 第148回 総会・講演会(2020年 秋学会)  2020.11 

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    Event date: 2020.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Other  

  • サブストームオンセットにおける中緯度電離圏全球応答の精査

    #林 萌英, @吉川 顕正, 藤本 晶子, Ohtani Shinichi

    地球電磁気・地球惑星圏学会 第148回 総会・講演会(2020年 秋学会)  2020.11 

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    Event date: 2020.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Country:Other  

  • Sq・EEJ電流系における6日振動現象に着目した大気圏ー電離圏の上下結合の研究 International conference

    #高山 久美, @三好 勉信, @吉川 顕正

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Event date: 2020.7

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    Venue:オンライン   Country:Other  

  • Alfvénic disturbances generated by the ionospheric polarization and the convection reversal in the magnetosphere International conference

    中溝 葵, 吉川 顕正, 大谷 晋一, 田中 高史

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Venue:オンライン   Country:Other  

  • Causality for formation of electromagnetic channel from Polar to Equatorial Ionosphere International conference

    吉川 顕正, 中溝 葵, 大谷 晋一

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Other  

  • Investigation of global electromagnetic coupling from polar to equatorial ionosphere International conference

    吉川 顕正, 河野 英昭, 阿部 修司, 魚住 禎司, 藤本 晶子, 池田 昭大, 樺澤 大生, 黒木 智, 林 萌英, 高山 久美, 中溝 葵, Ohtani Shinichi

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Event date: 2020.7

    Language:English   Presentation type:Oral presentation (general)  

    Country:Other  

  • 磁気圏電離圏全球結合系解明に向けたイオノグラムの自動読み取り International conference

    #林 萌英, @吉川 顕正, 藤本 晶子, 大谷 晋一

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Other  

  • MAGDAS9システムの10Hzデータによる、Pc2脈動の全球的発生分布特性解明 International conference

    #樺澤 大生, 吉@川 顕正, @魚住 禎司, 藤本 晶子, @阿部 修司

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Other  

  • Study on auroral 3D structure in the northen Europe International conference

    Yoshimasa Tanaka, Yasunobu Ogawa, Akira Kadokura, Takanori Nishiyama, Akimasa Yoshikawa, Bjorn Gustavsson, Kirsti Kauristie, Carl-fredrik, Enell, Urban Brandstrom, Tima Sergienko, Alexander Kozlovsky, Tero Raita, Vanhamaki Heikki

    Sixth International Symposium on Arctic Research (ISAR-6), Online  2020.3 

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    Event date: 2020.3

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco   Country:Japan  

  • 大分県久住町で観測されたシューマン共鳴の特性

    池田昭大, @魚住禎司, @吉川顕正, 藤本晶子, @阿部修司

    日本大気電気学会第98回研究発表会  2020.1 

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    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:静岡市   Country:Japan  

  • Diurnal and seasonal variations in the Schumann Resonance observed at Kuju Japan International conference

    Ikeda A., T. Uozumi, A. Yoshikawa, A. Fujimoto, and S. Abe

    AGU fall meeting  2019.12 

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    Event date: 2019.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco   Country:Japan  

  • プラネタリー波が電離圏変動に及ぼす影響

    三好 勉信, 山崎 洋介, 陣 英克, 藤田 茂, 吉川 顕正, 阿部 修司

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • Comparison of FM-CW Ionosonde and MAGDAS observations with S4 index in Peru

    Akiko Fujimoto, Shuji Abe, Akihiro Ikeda, Akimasa Yoshikawa

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • MAGDAS9システムの10Hzデータを用いた,Pc2脈動の全球的な発生特性解明

    #樺澤 大生, @吉川 顕正, @魚住 禎司, 藤本 晶子,@阿部 修司

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • Daily and seasonal variations of Schumann Resonance

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • One-to-one correspondence between the vertical evolution of AKR and global high-correlation Pi 2

    Teiji Uozumi, Akimasa Yoshikawa, Shinichi Ohtani, Atsushi Kumamoto, Fuminori Tsuchiya, Yoshiya Kasahara

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • サブストームに伴う磁気擾乱の子午面内伝播

    今城 峻, 能勢 正仁, 相田 真里, 東尾 奈々, 松本 晴久, 古賀 清一, 吉川 顕正

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • サブストームオンセット後のPc4脈動とオーロラストリーマーの動態解明に向けて,

    #波多江 真紀, @吉川 顕正, @魚住 禎司

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • Revisiting dynamical process of Birkeland current generation

    Akimasa Yoshikawa

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • Ionospheric Polarization: Deformation of Ionospheric Convection and Effects on Magnetosphere

    Aoi Nakamizo, Akimasa Yoshikawa, Shinichi Ohtani and Takashi Tanaka

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • 3D analysis of discrete arcs based on auroral computed tomography

    Yoshimasa Tanaka, Yasunobu Ogawa, Akira Kadokura, Takanori Nishiyama and Akimasa Yoshikawa

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • Deformation of ionospheric potential pattern by ionospheric Hall polarization International conference

    Aoi Nakamizo and Akimasa Yoshikawa

    SuperDARN Workshop 2019, Fuji  2019.6 

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    Event date: 2019.6

    Language:English   Presentation type:Symposium, workshop panel (public)  

    Venue:Fujiyoshida   Country:Japan  

    The present study shows that the ionospheric Hall polarization can deform the high-latitude ionospheric convection field, which is widely considered to be a manifestation of the convection field in the magnetosphere.
    We perform the Hall polarization field separation with a potential solver by changing the conductance distribution step- by-step from a uniform one to a more realistic one.
    We adopt dawn-dusk and north-south symmetric distributions of conductance and region 1 (R1) field-aligned current (FAC).
    The pair of the primary field of the R1 system and each gradient of Hall conductance generates the Hall polarization field and consequently causes potential deformations as follows.
    (a) The equatorward gradient causes clockwise rotation.
    (b) The gradient across the terminator, together with the effect of the equatorward gradient, causes the dawn-dusk asymmetry.
    (c) The high conductance band in the auroral region causes kink-type deformations.
    In particular, a nested structure at the equatorward edge of the band in the midnight sector well resembles the Harang Reversal.
    Result (a) can explain the clockwise bias inexplicable by the IMF-By effect alone, the combination of (a) and (b) can explain the clearness and unclearness in the round or crescent shapes of the dawn-dusk cells depending on the IMF-By polarity, and (c) suggests that the ionosphere may not need the upward-FAC for the formation of the Harang Reversal.
    We suggest that the final structure of the ionospheric potential is established by the combined effects of both the magnetospheric requirements (external causes) and ionospheric polarization (internal effect).

  • MAGDAS project: Research for global and local electromagnetic coupling from polar to equatorial ionosphere Invited International conference

    Akimasa Yoshikawa

    SuperDARN Workshop 2019, Fuji  2019.6 

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    Event date: 2019.6

    Language:English   Presentation type:Symposium, workshop panel (public)  

    Venue:Fujiyoshida   Country:Japan  

    International Center for Space Weather Science and Education (ICSWSE) of Kyushu University is a research institute that conducts academic research and education in space weather and related fields. We have constructed an observation network known as the "MAGDAS/CPMN (MAGnetic Data AcquisitionSystem/Circum-pan Pacific Magnetometer Network)" in international collaboration with more than 60 organizations, including those in developing countries. Currently, over 80 magnetometers and 4 FM-CW (Frequency Modulated Continuous Wave) radars have been installed all over the world. To understand the active role of ionospheric dynamics on the global and local Magnetosphere-Ionosphere coupling from polar to equatorial ionosphere, we conduct integrated studies of theory, numerical simulation, in-situ magnetosphere observation, and global ionosphere observation by MAGDAS. Especially, the ionospheric Hall effect strongly controls the spatiotemporal evolution of the M-I coupling system. Generation of polarization electric field at conductance gradient regions causes rotation, shear, and acceleration/deceleration of ionospheric convection in both local and global manners. The ionospheric polarization field activates upward shear Alfven wave that could cause ionospheric driven magnetospheric dynamics and induce a new type of M-I coupled current system. Generation of induction electric field at the wavefront of ionospheric disturbances enables the electric field of electrostatic potential type to propagate horizontally as a result of coupling between magnetosonic mode and shear Alfven mode induced by multistep Hall effect in a time domain, at the ionospheric E-layer. Such a combined effect of ionospheric Hall polarization and induction on the ionospheric dynamics is a key element for understanding the formation process of the global current system from polar to equatorial ionosphere. In this talk, we will discuss how to identify elementary components of Hall-polarization and induction effect (generalized Cowling effect) from coupled phenomena, and the possibility of collaborative studies between SuperDARN and MAGDAS project to further understand active role of ionospheric dynamics.

  • Revisiting the energy conversion process of Birkeland current

    Akimasa Yoshikawa

    日本地球惑星科学連合2019年大会  2019.5 

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    Event date: 2019.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張メッセ   Country:Japan  

  • 太陽地球系結合過程の研究基盤形成 Invited

    山本 衛, 橋口 浩之, 横山 竜宏, 宮岡 宏, 小川 泰信, 塩川 和夫, 野澤 悟徳, 吉川 顕正, 津田 敏隆

    日本地球惑星科学連合2019年大会  2019.5 

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    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張メッセ   Country:Japan  

  • Development of MAGDAS project: Search for global electromagnetic coupling from polar to equatorial ionosphere

    吉川 顕正, 樺澤 大生, 魚住 禎司, 藤本 晶子, 阿部 修司

    日本地球惑星科学連合2019年大会  2019.5 

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    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張メッセ   Country:Japan  

  • MAGDAS9システムの10Hzデータによる,Pc1-2脈動の全球分布特性解明

    #樺澤 大生, @吉川 顕正, @魚住 禎司, 藤本 晶子, @阿部 修司

    日本地球惑星科学連合2019年大会  2019.5 

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    Event date: 2019.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張メッセ   Country:Japan  

  • Latest installation of FM-CW radar in Peru

    藤本 晶子, 池田 昭大, 吉川顕正

    日本地球惑星科学連合2019年大会  2019.5 

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    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張メッセ   Country:Japan  

  • Research of Geomagnetism for Earth and Space Environmen Invited International conference

    Akimasa YOSHIKAWA

    Theme Seminar of the Scientific lecture at the annual Theme Seminar of the Sri Lanka Association for the Advancement of Science (“Space Science and Technology Applications for Sustainable Development” )  2018.12 

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    Event date: 2018.12

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:コロンボ   Country:Sri Lanka  

  • Revisiting the dynamic process of field-aligned current generation

    Akimasa Yoshikawa, Teiji Uozumi, Aoi Nakamizo, Shinichi Ohtani

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • Characteristics of temporal variation of AKR and Pi 2 observed by ARASE and MAGDAS/CPMN: Initial results

    Teiji Uozumi, Akimasa Yoshikawa, Shinichi Ohtani, Atsushi Kumamoto, Fuminori Tsuchiya, Yoshiya Kasahara

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • Variation of Schumann Resonance during the intense solar activity from October to November, 2003

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • Propagation of Pi2 pulsation from nightside to dayside: Observations and modeling of global current system

    Shun Imajo, Akimasa Yoshikawa, Teiji Uozumi, Shinichi Ohtani, Aoi Nakamizo, Peter Chi

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • EEJ、CEJ とプラズマバブルの関係

    #秋山 鷹史, @吉川 顕正, 藤本 晶子, 魚住 禎司

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • 磁気擾乱時における中低緯度領域電磁誘導応答の研究

    #中原 美音, @吉川 顕正, @魚住 禎司, 藤本 晶子

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • サブストームオンセット後に励起されるPc4脈動とオーロラストリーマの動態解明に向けて

    #波多江 真紀, @吉川 顕正, @魚住 禎司

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • Geomagnetism and Life Invited International conference

    Akimasa YOSHIKAWA

    Geomagnetic Focus Group Discussion 2018  2018.9 

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    Event date: 2018.9

    Language:English   Presentation type:Oral presentation (general)  

    Venue:BMKG, Jakarta   Country:Indonesia  

  • Space Weather Data in IR 4.0 (Industry Revolution 4.0) era and the success story on MAGDAS project Invited International conference

    Akimasa YOSHIKAWA

    International Conference on Space Weather and Satellite Application (ICeSSAT2018)  2018.8 

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    Event date: 2018.8

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Shah, Alam, Selangor   Country:Malaysia  

  • Electromagnetic Induction Responses to Geomagnetic Disturbances at Low-And-Mid-Latitudes International conference

    Mio Nakahara, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto

    International Conference on Space Weather and Satellite Application (ICeSSAT2018)  2018.8 

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    Event date: 2018.8

    Language:English  

    Venue:Shah, Alam, Selangor   Country:Malaysia  

  • Characteristic of the Disturbed Days Ionospheric Current System in the 180-Degree Magnetic Meridian International conference

    Siti Nurbaiti Ibrahim, Mohamad Huzaimy Jusoh, Ahmad Asari Sulaiman, Akimasa Yoshikawa

    International Conference on Space Weather and Satellite Application (ICeSSAT2018)  2018.8 

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    Event date: 2018.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Shah, Alam, Selangor   Country:Malaysia  

  • Relationship Between Plasma Bubble and Ionospheric Current Equatorial Electrojet and Equatorial Counter Electrojet International conference

    Takafumi Akiyama and Akimasa Yoshikawa, Akiko Fujimoto, Teiji Uozumi

    International Conference on Space Weather and Satellite Application (ICeSSAT2018)  2018.8 

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    Event date: 2018.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Shah, Alam, Selangor   Country:Malaysia  

  • On Generalization of Birkeland Current System in the Tree-Dimensional Magnetosphere-Ionosphere Coupling Invited International conference

    Akimasa Yoshikawa

    AOGS2018 15th Annual Meeting  2018.6 

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    Event date: 2018.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Waikiki, Hawai   Country:United States  

  • Response of Schumann Resonance to Solar and Geomagnetic Activities International conference

    Akihiro IKEDA, Teiji UOZUMI, Akimasa YOSHIKAWA, Akiko FUJIMOTO, Shuji ABE, Hiromasa NOZAWA, Manabu SHINOHARA

    AOGS2018 15th Annual Meeting  2018.6 

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    Event date: 2018.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Waikiki, Hawai   Country:United States  

  • Local Time Characteristic of Low-Latitude Geomagnetic Field Response to Intense Solar Flares International conference

    Akiko FUJIMOTO, Akimasa YOSHIKAWA, Toshiya NISHIGUCHI

    AOGS2018 15th Annual Meeting  2018.6 

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    Event date: 2018.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Waikiki, Hawai   Country:United States  

  • Decomposition of the Wave Elements of the Global High-Correlation Pi 2 International conference

    Teiji UOZUMI, Akimasa YOSHIKAWA, Shin OHTANI, Dmitry BAISHEV, Alexey MOISEEV, Boris SHEVTSOV

    AOGS2018 15th Annual Meeting  2018.6 

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    Event date: 2018.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Waikiki, Hawai   Country:United States  

  • Study of anomalous behaviors of geomagnetic diurnal variations prior to earthquake

    #白 旻基, @吉川 顕正

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • 3D current system of eastward expanding auroral surges

    田中 良昌, 小川 泰信, 門倉 昭, Gustavsson Bjorn, Partamies Noora, Kauristie Kirsti, Whiter Daniel, Enell Carl-fredrik, Brandstrom Urban, Sergienko Tima, Kozlovsky Alexander, Vanhamaki Heikki, 吉川 顕正, 宮岡 宏

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • Study of the Jovian magnetosphere-ionosphere coupling using an ionospheric potential solver: Contributions of H+ and meteoric ions to ionospheric conductivity

    寺田 綱一朗, 垰 千尋, 寺田 直樹, 笠羽 康正, 北 元, 中溝 葵, 吉川 顕正, 大谷 晋一, 土屋 史紀, 鍵谷 将人, 坂野井 健, 村上 豪, 吉岡 和夫, 木村 智樹, 山崎 敦, 吉川 一朗

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • Global distribution of ULF waves during magnetic storms: Comparison of Arase and ground observations and BATSRUS+CRCM modeling

    高橋 直子, 関 華奈子, 寺本 万里子, Mei-Ching Fok, 松岡 彩子, 東尾 奈々, 塩川 和夫, Dmitry Baishev, 吉川 顕正

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • 太陽地球系結合過程の研究基盤形成

    山本 衛, 橋口 浩之, 宮岡 宏, 小川 泰信, 塩川 和夫, 野澤 悟徳, 吉川 顕正, 津田 敏隆

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • Variation of Schumann resonance at Kuju station during solar flares

    池田 昭大, 魚住 禎司, 吉川 顕正, 藤本 晶子, 野澤 宏大

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • Recent activities of MAGDAS project

    阿部 修司, 吉川 顕正, 魚住 禎司, 藤本 晶子

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • Research project for investigation of active role of ionospheric dynamics on the magnetosphere-ionosphere coupled system

    吉川 顕正, 大谷 晋一, 中溝 葵, 今城 峻

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • Effects of Ionospheric Hall Polarization on Magnetospheric Configurations and Dynamics in Global MHD Simulation

    中溝 葵, 吉川 顕正, 田中 高史

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • FM-CW radar project: goals and a new installation in Peru

    藤本 晶子, 池田 昭大, 吉川 顕正

    日本地球惑星科学連合2018大会  2018.5 

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    Event date: 2018.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ   Country:Japan  

  • Generalized Description of Three- Dimensional Magnetosphere-Ionosphere Coupling by Shear Alfvén Waves International conference

    Yoshikawa A., A. Nakamizo, and S. Ohtani

    2016 Fall AGU Meeting  2016.12 

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    Event date: 2017.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco (California)   Country:United States  

  • Development of EEJ Model Based on Dense Ground-based Magnetometer Array International conference

    Matsushita, H., A. Yoshikawa, T. Uozumi, A. Fujimoto, S. Abe, J. K. Ishitsuka, O. Veliz, D. Rosales, E. Safor and V. Beteta

    2016 Fall AGU Meeting  2016.12 

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    Event date: 2017.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco (California)   Country:United States  

  • Possibility of Ionospheric Cause of FACs and Convection Field in the Magnetosphere-Ionosphere System: The Harang Reversal, Premidnight Upward-FAC, and the Ionospheric Hall Polarization Field International conference

    A. Nakamizo and A. Yoshikawa

    2016 Fall AGU Meeting  2016.12 

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    Event date: 2017.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco (California)   Country:United States  

  • Field-aligned Currents Induced by Electrostatic Polarization at the Ionosphere: Application to the Poleward Boundary Intensification (PBI) of Auroral Emission International conference

    Ohtani, S., and A. Yoshikawa

    2016 Fall AGU Meeting  2016.12 

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    Event date: 2017.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco (California)   Country:United States  

  • Effects of Ionospheric Hall Polarization on Magnetospheric Configurations and Dynamics in Global MHD Simulation Invited International conference

    A Nakamizo, A Yoshikawa, T Tanaka

    AGU Fall Meeting  2017.12 

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    Event date: 2017.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:New Orleans, USA   Country:United States  

  • Magnetosphere-Ionosphere Coupling Invited International conference

    @Yoshikawa A.

    The SCOSTEP/ISWI International School on Space Science  2016.11 

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    Event date: 2017.11 - 2017.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Sangli, Maharashtra   Country:India  

  • PBI 数値シミュレーション~オーロラオーバルとオーロラストリーマーの相互作用 について~

    青柳 優介, 吉川 顕正

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Seasonal dependence of semidiurnal equatorial magnetic variations

    Akiko Fujimoto, Akimasa Yoshikawa, Teiji Uozumi, Shuji Abe, Hiroki Matsushita

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Comparison of ULF waves measured by the ERG satellite and MAGDAS network

    Akiko Fujimoto, Ayako Matsuoka, Akimasa Yoshikawa, Mariko Teramoto, Reiko Nomura, Yoshimasa Tanaka, Manabu Shinohara

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • CEJ発生日のプラズマバブルイベント

    秋山 鷹史, 吉川 顕正, 藤本 晶子, 魚住 禎司

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • 磁気擾乱時における中低緯度領域電磁誘導応答の研究

    中原 美音, 吉川 顕正, 魚住 禎司, 藤本 晶子, 松下 拓輝

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • 各地方時におけるSFEの発生特性について

    西口 俊弥, 吉川 顕正, 藤本 晶子, 松下 拓輝

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Formation and Development of Poleward Boundary Intensifications of Auroral Emission

    Shinichi Ohtani, Tetsuo Motoba, Akimasa Yoshikawa

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Effects of Ionospheric Hall Polarization Field on Magnetosphere in Global MHD Simulation

    Aoi Nakamizo, Akimasa Yoshikawa, Takashi Tanaka

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Application of a magnetospheric-ionospheric current model for dayside and terminator Pi2 pulsation

    Shun Imajo, Akimasa Yoshikawa, Teiji Uozumi, Shinichi Ohtani, Aoi Nakamizo, Peter Chi

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • New interpretation PBI

    Akimasa Yoshikawa, Shinichi Ohtani

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Monitoring of Space and Earth electromagnetic environment by MAGDAS project: Collaboration with IKIR Invited International conference

    Yoshikawa A.

    International Conference on Solar-Terrestrial Relations and Physics of Earthquake Precursors  2017.9 

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    Event date: 2017.9

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Paratunka, Kamchatka   Country:Russian Federation  

  • Characteristics of Schumann Resonance Parameters at Kuju Station Invited International conference

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe, Hiromasa Nozawa, Manabu Shinohara

    International Conference on Solar-Terrestrial Relations and Physics of Earthquake Precursors  2017.9 

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    Event date: 2017.9

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Paratunka, Kamchatka   Country:Russian Federation  

  • What is Space Weather? Invited International conference

    Yoshikawa A.

    Universidad Nacional Agraria de la Selva (UNAS) Invited Seminar  2017.8 

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    Event date: 2017.8

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Tingo Maria   Country:Peru  

  • (B,V) Paradigm of Magnetosphere-Ionosphere Coupling Invited International conference

    Yoshikawa A.

    URSI Asia-Pacific Radio Science Conference (URSI AP-RASC 2016)  2016.8 

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    Event date: 2017.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Soul, Korea   Country:Korea, Republic of  

    これまでの磁気圏電離圏結合研究では、磁気圏側はMHDダイナミクス(B-Vパラダイム)で、電離圏側は静電的な電離層電流層近似(J-Eパラダイム)で扱われ、その両者は静電的な境界条件をつうじた結合問題として扱われてきた。本研究では電離圏ダイナミクスをイオン-中性大気の衝突効果により必然的に生じるHall電場を電離圏から磁気圏までシームレスに導入する理論的枠組を整理し、磁気圏電離圏結合系を一つの系のダイナミクスの下に記述する(B,V)パラダイムを提案する。これにより、これまで電気回路的な理解しかされてこなかった電離圏特有の現象をプラズマダイナミクスの文脈の下に記述することが可能となる。

  • Magnetosphere-Ionosphere coupling by shear Alfven wave Invited International conference

    Impact of Space Weather on Earth COSPAR Capacity Building Workshop

    August 15 – 26, 2016  2016.8 

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    Event date: 2017.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Paratunka, Kamchatka   Country:Russian Federation  

  • Geomagnetic observation to support space weather study Invited International conference

    Yoshikawa A.

    AMGASA Public Talk  2017.8 

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    Event date: 2017.8

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:National University of Malaysia, Kuala Lumpur   Country:Malaysia  

    汎世界的な地磁気多点観測網によりあぶり出される様々な宇宙天気現象、宇宙ー気象ー地象結合現象について紹介し、その適用サイエンスの幅広さと様々な地球物理現象のモニタリングの可能性について、わかりやすく講演する。

  • Study of Coupling Processes in the Solar-Terrestrial System Invited International conference

    Yoshikawa A.

    2nd National School on EARTH and ELECTROMAGNETISM  2017.8 

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    Event date: 2017.8

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Mara Technical University, Johor Bahru   Country:Malaysia  

  • Space Weather Indexes Produced by ICSWSE/MAGDAS Project International conference

    Yoshikawa A., Fujimoto, A., T. Uozumi, S. Abe, H. Matsushita, and, S. Abe

    Asia Oceania Geoscience Society 13th Annual Meeting  2016.7 

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    Event date: 2017.7 - 2017.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Beijing   Country:China  

  • Three components analysis of ground magnetometer network data for developing GIC index,13th Annual Meeting Asia Oceania Geoscience Society International conference

    Abe. S, H. Matsushita, Y. Nawata, A. Yoshikawa

    Asia Oceania Geoscience Society 13th Annual Meeting  2016.7 

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    Event date: 2017.7 - 2017.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Beijing   Country:China  

  • Long-term EE-index Variation for Monitoring Equatorial Electrojet Based on ICSWSE Magnetometer Network International conference

    Fujimoto, A., T. Uozumi, S. Abe, H. Matsushita, and A. Yoshikawa

    Asia Oceania Geoscience Society 13th Annual Meeting  2016.7 

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    Event date: 2017.7 - 2017.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Beijing   Country:China  

  • Development Of New Eej Index By Dense Magnetometer Array In Peru, presented at Asia Oceania Geoscience Society 13th Annual Meeting International conference

    Matsushita, H., A. Yoshikawa, T. Uozumi, A. Fujimoto, S. Abe, J. K. Ishitsuka, O. Veliz, D. ROSALES, E. SAFOR, V. BETETA, and G. CÁRDENAS

    Asia Oceania Geoscience Society 13th Annual Meeting  2016.7 

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    Event date: 2017.7 - 2017.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Beijing   Country:China  

  • How much curl-free Hall current flows out to the magnetosphere as field-aligned current from Cowling channel? International conference

    Yoshikawa A.

    Chamman Conference on Current in Geospace and Beyond  2016.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Dubrovnik   Country:Croatia  

  • Recent Development of ICWSE/MAGDAS project for Study of Coupling Processes in the Solar-Terrestrial System International conference

    Yoshikawa A.

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Latitudinal and Longitudinal Profile of EEJ current during different phases of Solar Cycle International conference

    Nurul Shazana Abdul Hamid, Wan Nur Izzaty Ismail, Mardina Abdullah, Akimasa Yoshikawa

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • The Sq-current and the Ionospheric Profile Parameters during Solar Minimum International conference

    Nurul Shazana Abdul Hamid, Saeed Abioye Bello, Mardina Abdullah, Akimasa Yoshikawa

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Study of the Coupled Solar-Earth System with Large Atmospheric Radars, Ground-based Observation Network and Satellite Data: Project Overview International conference

    津田 敏隆, 山本 衛, 橋口 浩之, 宮岡 宏, 小川 泰信, 塩川 和夫, 野澤 悟徳, 吉川 顕正

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • スペースデブリ環境推移モデルにおける大気密度モデルの改良と宇宙天気活動の影響評価 International conference

    阿部 修司, 花田 俊也, 吉川 顕正, 平井 隆之, 河本 聡美

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • 磁気擾乱時における中低緯度領域電磁誘導応答の研究 International conference

    中原 美音, 松下 拓輝, 吉川 顕正, 魚住 禎司, 藤本 晶子, 阿部 修司

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • On the relationships between EEJ distribution and plasma bubble occurrences International conference

    秋山 鷹史, 吉川 顕正, 松下 拓輝, 藤本 晶子, 魚住 禎司

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Application of Global Three-Dimensional Current Model for Dayside and Terminator Pi2 Pulsations International conference

    今城 峻, 吉川 顕正, 魚住 禎司, 大谷 晋一, 中溝 葵

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Study on Effects of Ionospheric Polarization Field and Inner Boundary Conditions on Magnetospheric Dynamics and Substorm Processes in Global MHD Simulation International conference

    中溝 葵, 吉川 顕正, 田中 高史

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • MAGDASプロジェクトEE-indexの磁気赤道域現象への適用事例 International conference

    藤本 晶子, 吉川 顕正, 魚住 禎司, 阿部 修司, 松下 拓輝

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Magnetosphere-Ionosphere coupling process produced by Ampere force forcing from the magnetosphere International conference

    Yoshikawa A.

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Co-seismic magnetic signatures of Moro Gulf Quake of 2010-07-23 using MAGDAS data

    Quirino Sugon Jr., Christine Chan, Felix Muga II, Clint Bennett, Randell Teodoro, Sergio Su, Daniel McNamara, Dexter Lo, Roland Otadoy, Grace Rolusta, Akiko Fujimoto, Teiji Uozumi, and Akimasa Yoshikawa

    地域ネットワークによる宇宙天気の観測・教育活動に関する研究集会  2017.3 

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    Event date: 2017.3

    Language:English   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡県福岡市   Country:Japan  

  • 振動電流系、定在性および伝播性MHD波動としてのPi2振動の共存: 事例解析

    今城峻, 吉川顕正, 魚住禎司, 西村幸敏, Vassilis Angelopoulos, Eric Donovan

    電磁圏物理学シンポジウム  2017.3 

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    Event date: 2017.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡県福岡市   Country:Japan  

  • EE-indexに基づく赤道地磁気活動の概況報告(2016年9月~2017年2月)

    藤本晶子, 魚住禎司, 阿部修司, 松下拓輝, 吉川顕正

    平成28年度・第2回STE現象報告会  2017.3 

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    Event date: 2017.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡県福岡市   Country:Japan  

  • EE-indexの磁気赤道域現象への適用事例と課題

    藤本晶子, 吉川顕正, 魚住禎司, 阿部修司, 松下拓輝, MAGDASプロジェクト

    平成28年度・第2回STE現象報告会  2017.3 

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    Event date: 2017.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡県福岡市   Country:Japan  

  • MAGDAS/CPMNプロジェクトの現状と課題

    Yoshikawa A.

    九州大学西新プラザ、福岡県福岡市  2017.3 

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    Event date: 2017.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • MAGDAS/CPMNプロジェクトの現状と課題

    Yoshikawa A.

    シンポジウム「太陽地球系科学に於ける地上観測の現状と課題」  2017.3 

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    Event date: 2017.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡県福岡市   Country:Japan  

  • Coordinated observation of Pi2 pulsations by global magnetometer array, all sky imager and satellites in the plasmasphere

    Shun Imajo, Yukitoshi Nishimura, Akimasa Yoshikawa, Teiji Uozumi, Shinichi Ohtani, Aoi Nakamizo, Vassilis Angelopoulos, Stephen Mende

    NIPR Symposium on Polar Science  2016.11 

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    Event date: 2016.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所   Country:Japan  

  • EE-indexに基づく赤道地磁気活動の概況報告(2016年4月~2016年11月)

    藤本晶子, 魚住禎司, 阿部修司, 松下拓輝, and 吉川顕正

    平成28年度・第1回STE現象報告会  2016.11 

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    Event date: 2016.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学宇宙地球環境研究所、名古屋   Country:Japan  

  • Generalization of Ionospheric Polarization and Magnetospheric Field- Resonance

    吉川顕正

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • Solar terminator effects on middle- to low-latitude Pi2 pulsations

    Imajo, S., A. Yoshikawa, T. Uozumi, S. Ohtani, A. Nakamizo, S.Demberel, and B. M. Shevtsov

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • Auroral features of Pi2 pulsation associated with poleward boundary intensification

    今城峻, 西村幸敏, 吉川顕正, 魚住禎司, Ohtani Shinichi, 中溝葵, Vassilis Agelopoulos, Stephen Mende

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • Lunar tide variation of Equatorial Electrojet based on the long-term EE-index

    Fujimoto, A., T. Uozumi, S. Abe, H. Matsushita, and A. Yoshikawa

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • 磁気圏MHDグローバルモデルにおける磁気圏電離圏解法部分の概要・ 再考・改良計画 International conference

    中溝葵, 吉川顕正, 中田裕之

    第13回 宇宙環境シンポジウム  2016.11 

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    Event date: 2016.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京都小金井市   Country:Japan  

  • 磁気圏電離圏結合 Invited

    吉川顕正

    平成28年度「磁気圏・電離圏シンポジウム」、電離圏・磁気圏探査衛星検討リサーチグループ第1回会合」  2016.10 

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    Event date: 2016.10 - 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:宇宙科学研究所, 神奈川県相模原市   Country:Japan  

  • 磁気圏電離圏結合ダイナミクスの無撞着な記述:境界条件を超えて Invited International conference

    吉川顕正

    「磁気圏複合系研究会・プラズマシート極域電離圏投影問題研究会」  2016.9 

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    Event date: 2016.9 - 2017.9

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所、東京都立川市   Country:Japan  

  • Alfven波による一般化された3次元磁気圏電離圏結合 Invited International conference

    吉川顕正

    名大ISEE/極地研/NICT/京大RISH 共同主催「中間圏・熱圏・電離圏 (MTI) 研究集会」/(第321回生存圏シンポジウム)  2016.8 

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    Event date: 2016.8 - 2017.8

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:情報通信研究機構, 東京都小金井市   Country:Japan  

  • Recent development of MAGDAS project: Strategy for international alliance of geomagnetic field network observation International conference

    Yoshikawa A., Shuji Abe, Teiji Uozumi, Akiko Fujimoto, Hiroki Matsushita, Hideaki Kawano

    日本地球惑星科学連合2016大会  2016.5 

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    Event date: 2016.5 - 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • The Harang Reversal Generated by Ionospheric Polarization Field by Hall Current Divergence International conference

    Nakamizo, A. and A. Yoshikawa

    日本地球惑星科学連合2016大会  2016.5 

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    Event date: 2016.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Three components analysis of ground magnetometer network data for understanding GIC excited by space weather disturbances International conference

    Abe. S, H. Matsushita, Y. Nawata, A. Yoshikawa

    日本地球惑星科学連合2016大会  2016.5 

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    Event date: 2016.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • What if the evolution of auroral forms does not reflect magnetospheric processes? International conference

    Ohtani, S., and A. Yoshikawa

    日本地球惑星科学連合2016大会  2016.5 

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    Event date: 2016.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • 湯元教授の九大での貢献について-観測と教育を中心に- Invited

    吉川顕正

    電磁圏物理学シンポジウム  2016.3 

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    Event date: 2016.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡市   Country:Japan  

  • 中低緯度Pi2地磁気脈動に対する朝夕昼夜境界の効果 Invited

    今城 峻, 吉川 顕正, 魚住 禎司, Shinichi Ohtani, 中溝葵

    電磁圏物理学シンポジウム  2016.3 

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    Event date: 2016.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡市   Country:Japan  

  • ペルー新地磁気観測ネットワークから見た、2015年12月19日発生の磁気嵐時のEEJ構造について Invited

    松下拓輝, 吉川顕正, 魚住禎司, 阿部修司, 藤本晶子

    STE現象報告会  2016.3 

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    Event date: 2016.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡市   Country:Japan  

  • EE-indexに基 づく赤道地磁気活動の概況報告(2015年9月~2016年3月) Invited

    藤本 晶子, 魚住 禎司, 阿部 修司, 松下 拓輝, 吉川 顕正

    平成 27年度・第2回STE現象報告会  2016.3 

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    Event date: 2016.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡市   Country:Japan  

  • Correlated temporal variations of AKR, substorm current wedge and global Pi 2 Invited

    Teiji Uozumi, A. Yoshikawa, S. Ohtani, S. Imajo, D. G. Baishev, A. V. Moiseyev, B. M. Shevtsov, and K. Yumoto

    平成27年度名古屋大学宇宙地球環境研究所研究集会 「サブストーム研究会」  2016.2 

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    Event date: 2016.2

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学 宇宙地球環境研究所   Country:Japan  

  • Development of dense magnetometer array in Peru for investigating detailed structure of EEJ International conference

    Matsushita, H, A. Yoshikawa, T. Uozumi, J. Ishitsuka, D. Rosales, O. Veliz, V. B. Alvarado and G. M. Cárdenas

    1st PSTEP International Symposium  2016.1 

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    Event date: 2016.1

    Language:English   Presentation type:Oral presentation (general)  

    Venue:ES Hall in Higashiyama campus of Nagoya University   Country:Japan  

  • Space weather environment index based on ICSWSE magnetometer network International conference

    Fujimoto, A., A. Yoshikawa, T. Uozumi, S. Abe, and H. Matsushita

    1st PSTEP International Symposium  2016.1 

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    Event date: 2016.1

    Language:English   Presentation type:Oral presentation (general)  

    Venue:ES Hall in Higashiyama campus of Nagoya University   Country:Japan  

  • 汎地球観測ネットワークを基軸とした 宇宙天気研究・教育の革新的国際展開

    吉川顕正, 花田俊也, 羽田亨

    第12回 宇宙環境シンポジウム  2015.11 

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    Event date: 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:北九州国際会議場 国際会議室   Country:Japan  

  • 九大多磁場観測網を用いた地磁気誘導電流関連研究の展開と展望

    阿部 修司, 吉川 顕正, 魚住 禎司, 藤本 晶子, 松下 拓輝, 縄田 由香利

    第5回極端宇宙天気研究会  2015.11 

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    Event date: 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋   Country:Japan  

  • 磁気圏電離圏結合の理論的研究 Invited

    吉川顕正

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (invited, special)  

    Venue:東京大学 理学部   Country:Japan  

    強磁場弱電離気体系である電離圏と、無衝突系 である磁気圏との相互作用の結果生じる磁気圏電 離圏結合系には、係わる現象の多彩さや複雑さか ら多くの未解明問題が残されている。 本研究ではこのような系で現象実現機構をシステムとして理解する事の重要性を世界に先駆けて明らかにしてきた。 さらに、理論的手法を中心に多圏間結合システム の本質的理解を強く希求する研究を積み上げ、磁気圏及び非等方的な伝導性 をもつ電離圏における磁気流体波動と、中性大気 及び固体地球での電磁波動が結合した多圏間結合 系を定式化し、そのシステム解が Hall 効果によって強くコントロールされることを発見すると ともに、その物理的メカニズムを世界で初めて明 らかにした。本講演では演者がこれまでに構築してきた多圏間結合物理学の理論体系、それからえられる様々な物理現象について紹介する。

  • Alfven wave in the weakly ionized system

    Akimasa Yoshikawa, T. Uozumi, A. Nakamizo, S.Ohtani, R. Fujii

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

  • Spatial-temporal response of space debris distribution to geomagnetic storms

    Uetsuhara T, Akimasa Yoshikawa, T. Uozumi

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.11 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

  • A new idea for the equatorial electric field asymmetries based on the global polarization effect

    Nakamizo A, Akimasa Yoshikawa, S. Ohtani, S. Imajo, A. Ieda, K. Seki

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.11 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

  • オーロラストリーマの移動に伴う磁気圏-電離圏結合対流の変動

    上谷 浩之, Akimasa Yoshikawa

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.11 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

  • FLR周波数自動検出と、それによる磁気圏プラズマ質量密度の緯度経度構造の統計解析

    北川 雄一郎, 河野 英昭, Mann Ian R, Milling David, 林 幹治, 北村 健太郎, Akimasa Yoshikawa

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.11 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

  • Harang discontinuity and ionospheric polarization field by Hall current divergence

    Aoi Nakamizo, Akimasa Yoshikawa

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京大学 理学部   Country:Japan  

  • 低緯度朝側昼夜境界付近で観測されるPi2型地磁気脈動と湾型磁場変動

    今城 峻, 吉川 顕正, 魚住 禎司, Ohtani Shinich, 中溝 葵

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京大学 理学部   Country:Japan  

  • Solar cycle variation of Equatorial Electrojet based on the EE-index

    藤本 晶子, 魚住 禎司, 阿部 修司, 今城 峻, 松下 拓輝, 吉川 顕正

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京大学 理学部   Country:Japan  

  • MAGDAS project and its new policy for data sharing

    阿部 修司, 魚住 禎司, 松下 拓輝, 藤本 晶子, 河野 英昭, 吉川 顕正

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京大学 理学部   Country:Japan  

  • (B,V)で俯瞰する磁気圏電離圏結合

    吉川顕正

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京大学 理学部   Country:Japan  

  • International alliance of geomagnetic field network observation Invited

    吉川顕正

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京大学 理学部   Country:Japan  

  • Time-dependent generalized Ohm’s Law and formation of global Cowling channel in the ionosphere International conference

    Yoshikawa A.

    14th International Symposium on Equatorial Aeronomy (ISEA)  2015.10 

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    Event date: 2015.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Bahir Dar University, Bahir Dar   Country:Ethiopia  

  • Longitudinal variation of Equatorial Electrojet and the Occurrence of its Counter Electrojet International conference

    Babatunde Rabiu, O.O.Folarin, T. Uozumi, N.S.Abdul-Hamid, A.Yoshikawa

    14th International Symposium on Equatorial Aeronomy (ISEA)  2015.10 

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    Event date: 2015.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Bahir Dar University, Bahir Dar   Country:Ethiopia  

  • 宇宙科学教育の国際的展開

    @吉川顕正、@花田俊也、@山岡均、@羽田亨

    第59回宇宙科学技術連合講演会  2015.10 

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    Event date: 2015.10 - 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:鹿児島市, かごしま県民交流センター   Country:Japan  

  • MAGDAS Network, Space Weather, and Geomagnetic Storms Invited International conference

    Yoshikawa A.

    A Conference on “Scientific Frontiers: Serving the Peripheries in Times of Change”  2015.9 

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    Event date: 2015.9

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Fr. Francis J. Heyden, SJ Hall , Manila Observatory, Ateneo de Manila Campus, Loyola Heights Quezon City   Country:Philippines  

  • The Magnetosphere-Ionosphere Coupling Invited International conference

    Yoshikawa A.

    International School on Equatorial and Low-Latitude Ionosphere, ISELLI  2015.9 

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    Event date: 2015.9

    Language:English   Presentation type:Public lecture, seminar, tutorial, course, or other speech  

    Venue:Abuja   Country:Nigeria  

  • Description of Magnetosphere-ionosphere coupling with Alfven waves Invited International conference

    Yoshikawa A.

    Olaf Amm Memorial Workshop  2015.9 

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    Event date: 2015.9

    Language:English   Presentation type:Oral presentation (general)  

    Venue:FMI, Helsinki   Country:Finland  

  • Nature of dayside ionospheric current system of Pi2 Pulsations: Comparison between equivalent currents and numerical simulation International conference

    Imajo S., A. Yoshikawa, T. Uozumi, S. Ohtani, A. Nakamizo, P. J. Chi

    AOGS12th Annual Meeting  2015.8 

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    Event date: 2015.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Singapore   Country:Singapore  

  • ICSWSE/ MAGDAS Research Project-極域-磁気赤道域電磁結合系の探査

    吉川 顕正

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • MAGDASプロジェクトと新しいデータ共有ポリシー

    阿部 修司, 魚住 禎司, 松下 拓輝, 藤本 晶子, 河野 英昭, 吉川 顕正

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • Pi2型地磁気脈動の昼間側電離層電流系: 等価電流系と数値計算の比較

    今城 峻, 吉川 顕正, 魚住 禎司, 大谷 晋一, 中溝 葵, Chi Peter

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • MAGDASネットワークによって観測された高速太陽風条件下での磁気赤道Pc 5の特徴

    秋本 開成, 藤本 晶子, 吉川 顕正, 魚住 禎司, 阿部 修司

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • Dp2イベント時の極域から磁気赤道域にかけてのグローバル電離圏電流系の特徴

    松下 拓輝, 吉川 顕正, 魚住 禎司

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • International collaboration in ground based magnetometer observations via ULTIMA: A tribute to Professor Kiyohumi Yumoto Invited

    CHI, Peter, YOSHIKAWA, Akimasa, MANN, Ian

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • 国際宇宙天気イニシアチブ プロジェクト(ISWI) Invited

    Gopalswamy Nat, 吉川 顕正

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • ICSWSEとSTELの連携についての展望 Invited

    羽田 亨, 吉川 顕正

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • 宇宙惑星科学における国際協力:過去・現在・将来

    佐々木 晶, 吉川 顕正

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • ICSWSE/ MAGDAS Projectに於ける国際宇宙天気キャパシティ・ビルディング

    吉川 顕正

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • 昼間側Pi2型地磁気脈動の等価電流分布と夜側FACの作る電離層電流系

    今城 峻, 吉川 顕正, 魚住 禎司, 大谷 晋一, 中溝 葵, 湯元清文

    平成27年度IUGONET研究集会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:立川市、東京   Country:Japan  

  • ICSWSE/MAGDAS project Invited International conference

    Akimasa Yoshikawa

    United Nations/Japan for Space Weather Symposium  2015.3 

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    Event date: 2015.3

    Language:English   Presentation type:Symposium, workshop panel (public)  

    Venue:Fukuoka   Country:Japan  

  • Computer simulation on formation of ionospheric current system accompanied by the incidence of shear Alfvén waves to the ionosphere International conference

    Estelle, Dirand, Akimasa Yoshikawa

    United Nations/Japan for Space Weather Symposium  2015.3 

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    Event date: 2015.3

    Language:English   Presentation type:Symposium, workshop panel (public)  

    Venue:Fukuoka   Country:Japan  

  • Recent developments from ICSWSE/MAGDAS Research Project Invited International conference

    Kiyohumi Yumoto, Akimasa Yoshikawa, Hideaki Kawano, S. Abe, T. Uozumi, M. Grace, G. Maeda

    AGU fall meeting  2014.12 

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    Event date: 2014.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco, USA   Country:United States  

  • ICSWSE MAGDAS project Invited International conference

    Akimasa Yoshikawa, Hideaki Kawano, S. Abe, T. Uozumi, M. Grace, G. Maeda

    National school on Space and Earth Electromagnetism(SEE) 2014  2014.12 

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    Event date: 2014.12

    Language:English   Presentation type:Symposium, workshop panel (public)  

    Venue:Langkawi National Observatory, National Space Agency, Malaysia(ANGKASA),   Country:Malaysia  

  • Space Science Capacity Building at International Center for Space Weather Science and Education (ICSWSE) Invited International conference

    Akimasa Yoshikawa, Hideaki Kawano, Shuji Abe, T. Uozumi, M. Grace, G. Maeda

    United Nations / Austria Symposium on “Space Science and the United Nations”  2014.9 

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    Event date: 2014.9

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Austrian Academy of Sciences, Institute for Space Research, Graz, Austria   Country:Austria  

  • Magnetosphere-Ionosphere Coupling through Alfven Wave, SCOSTEP/ISWI International Space Science School (ISSS) in Peru Invited International conference

    吉川 顕正

    SCOSTEP/ISWI International Space Science School (ISSS) in Peru  2014.9 

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    Event date: 2014.9

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Lima, Peru   Country:Peru  

  • Technical Presentation on the International Center for Space Weather Science and Education (ICSWSE) of Kyushu University Invited International conference

    吉川 顕正

    Geomagnetic Workshop in Medan (North Sumatra, Indonesia)  2014.9 

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    Event date: 2014.9

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Medan (North Sumatra, Indonesia), Hotel Sibayak Berastag   Country:Indonesia  

  • Theory of Cowling channel formation by reflection of shear Alfven waves from the auroral Ionosphere Invited International conference

    吉川 顕正

    AGU Chapman Conference on Low-Frequency Waves in Space Plasmas  2014.8 

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    Event date: 2014.9 - 2014.2

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Jeju Island, Republic of Korea   Country:Korea, Republic of  

    Cowlingチャンネルとは電離圏に於けるHall電流が電気伝導度勾配領域において発散成分をもつことによって生じる分極電場により、2次的に励起されるHall電流によって誘導された電流系の総称であり、本来のHall電流と2次的なHall電流が同方向に流れる事により、オーロラジェット電流や、赤道ジェット電流等の強力に強調されたジェット電流効果を生み出す基本メカニズムを内包していることは良く知られている。しかしながら、このジェット電流効果を定量的にコントロールするHall電流発散の電離圏内への閉じ込め効率、Hall電流がどれくらいの割合で電離圏内に閉じ込められ、どれくらいの割合で磁気圏に沿磁力線電流として流出するのか?それによってどれくらいの強さの2次的分極電場が生成され、どの程度ジェット電流効果が生み出されるのか?という問題が理論的にも観測的にも不明なままであった。本論文では、沿磁力線電流を形成するshear Alfven waveと相互作用するHall電流系の発散部分を一意に決定する理論枠組を構築し、Hall電流の電離圏内閉じ込め効率の定式化を初めて行う事により、電離圏で最もダイナミックに変動するジェット電流系の定量的解析を可能とする道筋を示したマイルストーン的な論文である。

  • ICSWSE/ MAGDAS Project: 極域-磁気赤道域電磁結合系の実証的研究

    Akimasa Yoshikawa, A. Nakamizo, S.Ohtani, Y. Tanaka

    Japan GeoScience Union Meeting 2014  2014.5 

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    Event date: 2014.4 - 2014.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:Pacifico Yokohama   Country:Japan  

  • VarSITIプログラム期間における国際宇宙天気科学・教育センター/MAGDASの研究プロジェクト

    河野 英昭, Akimasa Yoshikawa, 魚住 禎司, 阿部 修司, Cardinal Maria Gracita, 前田 丈二, 湯元 清文

    Japan GeoScience Union Meeting 2014  2014.4 

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    Event date: 2014.4 - 2014.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:Pacifico Yokohama   Country:Japan  

  • 電離層電流の地電流電磁的結合:非一様・非等方性伝導度の効果

    Akimasa Yoshikawa

    Japan GeoScience Union Meeting 2014  2014.5 

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    Event date: 2014.4 - 2014.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:Pacifico Yokohama   Country:Japan  

  • 磁気圏電離圏結合(異プラズマ結合システム:宇宙天気と太陽物理への一般物理の応用) Invited

    吉川 顕正

    太陽研連シンポジウム 「活動極大期を迎えた太陽研究の新たな展開、彩層プラズマ診断、宇宙天気、Solar-C」  2014.2 

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    Event date: 2014.2

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学理学研究科セミナーハウス   Country:Japan  

  • Technical presentation on the “International Center for Space Wather Science and Education”, Kyushu University Invited International conference

    Akimasa Yoshikawa

    第52回国連宇宙平和利用委員会  2014.2 

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    Event date: 2014.2

    Language:English   Presentation type:Oral presentation (general)  

    Venue:国連ウィーン本部, ウィーン   Country:Austria  

  • On formation of Global Cowling channel in the ionosphere and the generalized Ohm’s Law International conference

    Akimasa Yoshikawa

    AGU General Assembly 2013  2013.12 

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    Event date: 2013.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Moscone Convention Center, San Francisco, USA   Country:United States  

  • Rotation of the ionospheric electric potential caused by spatial gradients of ionospheric conductivity International conference

    A. Nakamizo, Akimasa Yoshikawa, Shinichi Ohtani, Akimasa Ieda, Kanako Seki

    AGU General Assembly 2013  2013.12 

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    Event date: 2013.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Moscone Convention Center, San Francisco, USA   Country:United States  

  • Progress of the MAGDAS Project During 2013 International conference

    G. Maeda, Akimasa Yoshikawa, S. Abe

    AGU General Assembly 2013  2013.12 

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    Event date: 2013.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Moscone Convention Center, San Francisco, USA   Country:United States  

  • Capacity building activities at ICSWSE International conference

    Cardinal, M.G, Akimasa Yoshikawa, Hideaki Kawano, Huixin Liu, Masakazu Watanabe, S. Abe, T. Uozumi, G. Maeda, Tohru Hada, Kiyohumi Yumoto

    SCOSTEP, International CAWSES-II meeting  2013.11 

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    Event date: 2013.11

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Nagoya, Japan   Country:Japan  

  • Rebuild of data distribution service for MAGDAS/CPMN project&#8232;, SCOSTEP, International CAWSES-II meeting International conference

    S. Abe, Akimasa Yoshikawa, Hideaki Kawano, T. Uozumi, A. Ikeda, Cardinal, M.G, G. Maeda, Kiyohumi Yumoto

    SCOSTEP, International CAWSES-II meeting  2013.11 

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    Event date: 2013.11

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Nagoya, Japan   Country:Japan  

  • MAGDAS activities of year 2013 International conference

    G. Maeda, Kiyohumi Yumoto, Hideaki Kawano, Akimasa Yoshikawa, Huixin Liu, Masakazu Watanabe, S. Abe, T. Uozumi, A. Ikeda, Cardinal, M.G

    SCOSTEP, International CAWSES-II meeting  2013.11 

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    Event date: 2013.11

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Nagoya, Japan   Country:Japan  

  • Effects of Hall-Pedersen ratio and conductivity gradients on the rotation of ionospheric electric field potential

    中溝 葵, 吉川 顕正, Ohtani Shinichi, 家田 章正, 関 華奈子

    第134回SGEPSS 総会及び講演会  2013.11 

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    Event date: 2013.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:高知大学朝倉キャンパス   Country:Japan  

  • Substorm current wedge model for Pi 2 pulsation revisited with middle-latitude MAGDAS and the Polar UVI data

    魚住 禎司, 吉川 顕正, Ohtani Shinichi, Baishev Dmitry, 阿部 修司, 河野 英昭, 湯元 清文

    第134回SGEPSS 総会及び講演会  2013.11 

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    Event date: 2013.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:高知大学朝倉キャンパス   Country:Japan  

  • Characteristic of longitudinal profile of dayside equatorial DP2 oscillation

    松下 拓輝, 吉川 顕正, 魚住 禎司, Ohtani Shinichi

    第134回SGEPSS 総会及び講演会  2013.11 

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    Event date: 2013.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:高知大学朝倉キャンパス   Country:Japan  

  • 弱電離気体系に於ける一般化された3次元オームの法則と分極電場生成について

    吉川 顕正, 中溝 葵, Ohtani Shinichi

    第134回SGEPSS 総会及び講演会  2013.11 

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    Event date: 2013.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:高知大学朝倉キャンパス   Country:Japan  

  • Pi 2型地磁気脈動に対する日の出境界の効果

    今城 峻, 吉川 顕正, 魚住 禎司, Marshall Richard, Shevtsov Boris M., 湯元 清文

    第134回SGEPSS 総会及び講演会  2013.11 

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    Event date: 2013.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:高知大学朝倉キャンパス   Country:Japan  

  • Modeling of 3-fluid dynamic and generalized Ohm’s law for understanding ionospheric dynamics Invited International conference

    Akimasa Yoshikawa

    JSPS Core-to-Core Program, 2013 ISWI and MAGDAS Africa School  2013.9 

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    Event date: 2013.9

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Abuja, Cote d'Ivoire   Country:Other  

  • MAGDAS/CPMN Project Invited International conference

    Akimasa Yoshikawa

    UN/Austria Symposium on “Space Weather Data, Instruments and Models: Looking Beyond the International Space Weather Initiative  2013.9 

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    Event date: 2013.9

    Language:English   Presentation type:Symposium, workshop panel (public)  

    Venue:Austrian Academy of Sciences, Institute for Space Research, Graz, Austria   Country:Austria  

  • MAGDAS Activities in Australia Since 2005 International conference

    G. Maeda, Kiyohumi Yumoto, Hideaki Kawano, Akimasa Yoshikawa, A. Ikeda, T. Uozumi, Huixin Liu, S. Abe, Masakazu Watanabe, Cardinal, M.G

    AOGS Annual meeting  2013.6 

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    Event date: 2013.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Brisbane, Australia   Country:Australia  

  • Remotely sensed of some parameters of the solar wind via a low-latitude Pc 5 index

    Magdi Elfadil Yousif Suliman, 吉川 顕正, 魚住 禎司, 湯元 清文

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 地球電磁気学・地球惑星圏科学の現状と将来(2)-人類活動を支える知識基盤の構築

    高橋 幸弘, 吉川 顕正, 清水 久芳, SGEPSS将来構想検討ワーキンググループ

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Symposium, workshop panel (public)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • ERG理論・モデリング・総合解析班およびERGサイエンスセンター現状報告

    関 華奈子, 三好 由純, 天野 孝伸, 齊藤 慎司, 宮下 幸長, 堀 智昭, 大村 善治, 海老原 祐輔, 能勢 正仁, 加藤 雄人, 家田 章正, 梅田 隆行, 齊藤 実穂, 北村 成寿, 中溝 葵, 瀬川 朋紀, 篠原 育, 松本 洋介, 中野 慎也, 吉川 顕正

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Symposium, workshop panel (public)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • IMAGE FUV と SuperDARN による沿磁力線電流分布の導出

    細川 敬祐, 吉川 顕正, 小川 泰信

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 極域電離圏等価電流系の季節変化

    田中 良昌, 行松 彰, 佐藤 夏雄, 堀 智昭, 吉川 顕正, 才田 聡子

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • DP2の伝播特性による電離圏電流の同定

    松下 拓輝, 吉川 顕正, 魚住 禎司, 池田 昭大

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 地球電磁気学・地球惑星圏科学の現状と将来(1) − 地球電磁気学・地球惑星圏科学の科学課題

    寺田 直樹, 吉村 令慧, 大塚 雄一, 小川 泰信, 神田 径, 櫻庭 中, 塩川 和夫, 篠原 育, 清水 久芳, 高橋 幸弘, 成行 泰裕, 藤井 郁子, 三好 由純, 山本 裕二, 吉川 顕正, SGEPSS将来構想検討ワーキンググループ

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Symposium, workshop panel (public)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • R1電流系と結合した赤道ジェット電流の電流保存について

    吉川 顕正

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 朝側で観測される東西偏波Pi 2の性質

    今城 峻, 吉川 顕正, 魚住 禎司, 大谷 晋一, 湯元 清文

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • MAGDAS capacity building activities at ICSWSE

    Maria Gracita Cardinal, 吉川 顕正, 河野 英昭, 渡辺 正和, LIU HUIXIN, Shuji Abe, Teiji Uozumi, George Maeda, Tohru Hada

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • M-I couping theory Invited International conference

    Akimasa Yoshikawa

    ECLAT Project Meeting, 2nd Project Review Graz  2013.4 

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    Event date: 2013.4

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Institute for Space Research, Graz, Austri   Country:Austria  

  • Current Closure from Polar to Equatorial Ionosphere via Cowling Channel, International conference

    Akimasa Yoshikawa

    EGU General Assembly 2013  2013.4 

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    Event date: 2013.4

    Language:English   Presentation type:Oral presentation (general)  

    Venue:ウィーン国際会議場   Country:Austria  

  • State-of-art in 3D Ionosphere and internal ionospheric dynamics effect on M-I coupling Invited International conference

    Akimasa Yoshikawa

    ISSI Forum "Near Earth Electro-magnetic Environment (Swarm and Cluster)  2013.4 

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    Event date: 2013.4

    Language:English   Presentation type:Oral presentation (general)  

    Venue:スイス国際宇宙科学研究所、ベルン   Country:Switzerland  

  • 強磁場弱電離気体系に於ける電流クロージャー:Hall電流時空間非一様性がもたらすもの Invited

    吉川 顕正

    日本物理学会第68回年次大会「プラズマ宇宙物理3学会合同セッション」  2013.3 

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    Event date: 2013.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:広島大学、広島県東広島市   Country:Japan  

  • Analogy of Magnetosphere-Ionosphere coupling and Corona-chromosphere-photosphere coupling Invited International conference

    Akimasa Yoshikawa

    ISSI Workshop on "Standing MHD Waves"  2013.2 

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    Event date: 2013.2 - 2013.3

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:スイス国際宇宙科学研究所、ベルン   Country:Switzerland  

  • Cowling チャンネルの物理 Invited

    吉川 顕正

    「国立極地研究所研究集会:極域電磁圏構造の非線形発展」  2013.2 

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    Event date: 2013.2

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所、東京都立川市   Country:Japan  

  • Technical presentation on the “International Center for Space Wather Science and Education”, Kyushu University Invited International conference

    Akimasa Yoshikawa

    第50回国連宇宙平和利用委員会  2013.2 

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    Event date: 2013.2

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:国連ウィーン本部, ウィーン   Country:Austria  

  • Cowlingチャンネル形成の理論 Invited

    吉川顕正

    国立極地研究所研究集会:極域電磁圏構造の非線形発展(観測と理論的アプローチの協働を目指して)  2012.12 

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    Event date: 2012.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所、東京都立川市   Country:Japan  

  • Formation of Cowling channel from Polar to Equatorial Ionosphere Invited International conference

    Akimasa Yoshikawa

    the 2012 AGU Fall Meeting  2012.12 

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    Event date: 2012.12

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Moscone Convention Center, San Francisco, California   Country:United States  

  • Illustration of Cowling channel coupling to the shear Alfven wave Invited

    吉川顕正

    第35回極域宙空圏シンポジウム  2012.11 

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    Event date: 2012.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所、東京都立川市   Country:Japan  

  • MI結合の理論的側面から見たEISCAT_3Dへの期待 Invited

    吉川 顕正

    EISCAT研究集会:北極・北欧における観測・研究戦略  2012.11 

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    Event date: 2012.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学,坂田ホール   Country:Japan  

  • Extraction of polarization field and magnetospheric impedance from the M-I coupled system via shear Alfven wave

    Akimasa Yoshikawa

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • SGEPSS 将来構想検討ワーキンググループ,太陽地球系科学の現状と科学課題 4:地球惑星圏における人類活動を支える知識基盤の構築

    高橋幸弘, 吉川 顕正

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:Japanese   Presentation type:Symposium, workshop panel (public)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • 将来構想の施策まとめに関するパネルディスカッション 1

    吉川 顕正

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:Japanese   Presentation type:Symposium, workshop panel (public)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • 1D simulation of Electron acceleration by Inertial Alfven wave pulse

    Run Shi, Huixin Liu, Akimasa Yoshikawa

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • The Response of the Dayside Equatorial Electrojet to Step-like Changes of IMF Bz

    Aoi Nakamizo, Akimasa Yoshikawa, T. Hori, A. Ieda, Y. Hiraki, K. Seiki, Y. Miyoshi, T. Kikuchi, Y. Ebihara

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • Formation of FAC -Cowling channel connecting from polar to equatorial ionosphere

    Akimasa Yoshikawa, Aoi Nakamizo, Shin Ohtani, Teiji Uozumi, Y. Tanaka

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • Establishment of International Center fot Space Science and education Invited International conference

    Akimasa Yoshikawa

    United Nations/Ecuador Workshop on the International Space Weather Initiative (20th Workshop of the United Nations Basic Space Science Initiative)  2012.10 

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    Event date: 2012.10

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Quito, Ecuador   Country:Ecuador  

  • Modeling of 3D Sq current system Invited International conference

    Akimasa Yoshikawa

    JSPS Core-to-Core Program, 2012 ISWI and MAGDAS School on Space Science  2012.9 

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    Event date: 2012.9

    Language:English   Presentation type:Public lecture, seminar, tutorial, course, or other speech  

    Venue:Bangdong, Indonesia   Country:Indonesia  

  • Opening of International Space Wather Science and Education Invited International conference

    Akimasa Yoshikawa

    UN/Austria Symposium on Space Weather Data Analysis  2012.9 

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    Event date: 2012.9

    Language:English   Presentation type:Oral presentation (invited, special)  

    Venue:Austrian Academy of Sciences, Institute for Space Research, Graz, Austria   Country:Austria  

  • On the importance of the Cowling/polarization mechanism for the electrodynamics of the ionosphere and magnetosphere

    吉川 顕正, Ryoichi Fujii, Olaf Amm, Heikki Vanhamakki

    2012年度日本地球惑星科学連合大会  2012.5 

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    Event date: 2012.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 宇宙天気研究キャパシティ・ビルディング(能力強化)のための拠点形成について

    湯元 清文, 吉川 顕正, 河野 英昭, LIU HUIXIN, 渡辺 正和, 池田 昭大, 前田丈二, 阿部修司, 魚住禎司

    2012年度日本地球惑星科学連合大会  2012.5 

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    Event date: 2012.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • Sq電流系に於ける3次元カウリングチャンネルモデル

    吉川 顕正, 魚住禎司, 湯元 清文

    2012年度日本地球惑星科学連合大会  2012.5 

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    Event date: 2012.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 電離圏に於ける入反射Alfven 波の分離

    吉川 顕正, 細川 敬祐, 小川 泰信

    2012年度日本地球惑星科学連合大会  2012.5 

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    Event date: 2012.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 極域から磁気赤道域にかけて形成されるCowlingチャンネル

    吉川 顕正, Shin Ohtani, 中溝葵, 魚住禎司, Kiyohumi Yumoto

    2012年度日本地球惑星科学連合大会  2012.5 

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    Event date: 2012.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 磁気圏電離圏チュートリアル Invited

    吉川顕正

    第26回大気圏シンポジウム  2012.3 

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    Event date: 2012.3

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:JAXA宇宙科学研究所・神奈川県相模原市   Country:Japan  

  • 理論的観点から見た電離圏・磁気圏結合 Invited

    吉川顕正

    国立天文台研究集会「太陽彩層と地球電離圏の接点」研究会  2012.1 

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    Event date: 2012.1

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:国立天文台・東京都三鷹市   Country:Japan  

  • A new method for describing the Cowling channel coupling to the FAC system via shear Alfven wave: Conjugate Hall current analysis International conference

    Yoshikawa A

    AGU-Fall meeting  2011.12 

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    Event date: 2011.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Moscone Convention Center&#8232;Howard Street, Between Third & Fifth Sts.&#8232;San Francisco, California, USA   Country:United States  

  • New method for describing theCowling channel coupling to the FAC system via shear Alfven wave: Conjugate Hall current analysis

    吉川顕正

    地球電磁気・地球惑星圏学会,第130回総会・講演会  2011.11 

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    Event date: 2011.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:神戸大学六甲第2キャンパス.   Country:Japan  

  • A new method for describing the Cowling channel coupling to the FAC system via shear Alfven wave: Conjugate Hall current analysis Invited International conference

    Yoshikawa A

    Workshop on Physical Processes in Non-Uniform Finite Magnetospheric Systems-50 Years of Tamao's Resonant Mode Coupling Theory  2011.9 

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    Event date: 2011.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Nishijin plaza, Fukuoka, Japan   Country:Japan  

  • A new method for describing the Cowling channel coupling to the FAC system via shear Alfven wave: Conjugate Hall current analysis Invited

    吉川顕正

    NICT/STEL共催 2011年度中間圏・熱圏・電離圏(MTI)研究集会  2011.8 

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    Event date: 2011.8

    Language:Others   Presentation type:Oral presentation (invited, special)  

    Venue:九州大学箱崎キャンパス   Country:Japan  

  • Principle of Geomagnetism Invited International conference

    Yoshikawa A

    ISWI/MAGDAS school on Litho-Space Weather  2011.8 

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    Event date: 2011.8 - 2011.9

    Language:Others   Presentation type:Public lecture, seminar, tutorial, course, or other speech  

    Venue:Redeemer's University , Nigeria, Lagos   Country:Other  

  • Geomagnetic Distrbances Invited International conference

    Yoshikawa A

    ISWI/MAGDAS school on Litho-Space Weather  2011.8 

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    Event date: 2011.8 - 2011.9

    Language:Others   Presentation type:Public lecture, seminar, tutorial, course, or other speech  

    Venue:Redeemer's University , Nigeria, Lagos   Country:Other  

  • A self-consistent formulation for the evolution of ionospheric conductances at the ionospheric E-region within an M-I coupling scheme International conference

    Yoshikawa A

    AGU Chapman conference on Relationship Between Auroral Phenomonology and Magnetospheric processes  2011.3 

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    Event date: 2011.2 - 2011.3

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Fairbanks, USA   Country:United States  

  • Cowling研究からみた二次元ポテンシャルソルバーの留意点 Invited

    吉川顕正

    平成22年度名古屋大学太陽地球環境研究所研究集会「GEMSIS-太陽、磁気圏、電離圏ワークショップ2010:ジオスペースにおける多圏間相互作用と高エネルギー粒子生成・消滅機構」  2010.12 

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    Event date: 2010.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:愛知県・犬山市、名鉄犬山ホテル   Country:Japan  

  • Cowlingチャンネル生成に伴う伝導度分配機構

    吉川顕正

    平成22年度国立極地研究所研究集会「極域における電離圏パラメータの非線形発展:モデル化と検証」  2010.12 

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    Event date: 2010.12

    Presentation type:Oral presentation (general)  

    Venue:国立極地研究所   Country:Japan  

  • Cowlingチャンネル研究の展開 Invited

    吉川顕正

    平成22年度名古屋大学太陽地球環境研究所研究集「EISCAT研究集会  2010.12 

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    Event date: 2010.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:東京都、小金井市、情報研究通信機構   Country:Japan  

  • 2009 年11 月にトロムソで観測された準定常オーロラパッチ

    田中良昌, 小川泰信, 宮岡宏, 海老原祐輔, 吉川顕正, 才田聡子, A. T. Weatherwax

    平成22年度名古屋大学太陽地球環境研究所研究集「EISCAT研究集会  2010.12 

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    Event date: 2010.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:東京都、小金井市、情報研究通信機構   Country:Japan  

  • 電流キャリア遷移過程を考慮した電気伝導度発展方程式の考察

    吉川顕正

    第34回極域宙空圏シンポジウム  2010.12 

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    Event date: 2010.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所   Country:Japan  

  • 磁気圏電離圏結合系に於ける電流キャリア遷移過程を考慮した電気伝導度モデリングとその帰結

    吉川 顕正, 中溝 葵, 魚住 禎司, 田中 良昌, 大谷 晋一

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • Hall Conjugate Analysis for extraction of Cowling Channel Invited International conference

    Yoshikawa A

    FMI-Invitation seminar  2010.9 

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    Event date: 2010.9

    Language:Others   Presentation type:Public lecture, seminar, tutorial, course, or other speech  

    Venue:FMI, Helsinki, Finland   Country:Finland  

  • Generalized Cowling Channel in the global ionosphere Invited International conference

    Yoshikawa A

    FMI-Invitation seminar  2010.8 

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    Event date: 2010.8

    Language:Others   Presentation type:Public lecture, seminar, tutorial, course, or other speech  

    Venue:FMI, Helsinki, Finland   Country:Finland  

  • Magnetosphere-ionosphere coupling process for poleward moving auroral arcs International conference

    Y.-M. Tanaka, Y. Ebihara, S. Saita, and A. Yoshikawa

    2010 Western Pacific Geophysics Meeting, 22–25 June 2010 &#8232;Taipei, Taiwan  2010.6 

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    Event date: 2010.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Taipei, Taiwan   Country:Taiwan, Province of China  

  • Formation of Cowling Channel through the Inductive MI-Coupling Process Invited International conference

    Yoshikawa A., O Amm, H Vanhamäki, and R Fujii

    2010 Western Pacific Geophysics Meeting, 22–25 June 2010 &#8232;Taipei, Taiwan  2010.6 

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    Event date: 2010.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Taipei, Taiwan   Country:Austria  

  • On the Harang-discontinuity type ionospheric potential field deformation derived from the multi- functional ionospheric potential solver Invited International conference

    Yoshikawa A., and S Ohtani

    2010 Western Pacific Geophysics Meeting, 22–25 June 2010 &#8232;Taipei, Taiwan  2010.6 

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    Event date: 2010.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Taipei, Taiwan   Country:Austria  

  • Alfven波をつうじたMI結合系でのCowling-channelの形成

    吉川 顕正

    日本地球惑星連合2010年大会  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張メッセ   Country:Japan  

  • 極域における磁気圏電離圏結合過程

    田中 良昌, 吉川 顕正

    日本地球惑星連合2010年大会  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張メッセ   Country:Japan  

  • 多機能型電離圏ポテンシャルソルバーによって導出された電離圏対流変形の要因分離:ハラング連続性の考察

    吉川 顕正

    日本地球惑星連合2010年大会  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張メッセ   Country:Japan  

  • Formation of Cowling Channel through the MI-Coupling Process via Shear Alfven Wave Invited International conference

    Yoshikawa A., O Amm and R Fujii

    EGU Spring meeting  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Vienne, Austria   Country:Austria  

  • Empirical Sq field model obtained from the 210°MMCPMN data during 1996-2007 International conference

    Y. Yamazaki, K. Yumoto, H. Terada, Y. Kakinami, T. Uozumi, S. Abe, A. Yoshikawa and CPMN Group

    AGU Fall meeting  2009.12 

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    Event date: 2009.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Moscone Convention Center&#8232;Howard Street, Between Third & Fifth Sts.&#8232;San Francisco, California, USA   Country:United States  

  • The α- and β-current separation of MI-coupled system using Whalen-relation and Hall conjugate current analysis International conference

    Yoshikawa A

    AGU Fall meeting  2009.12 

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    Event date: 2009.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Moscone Convention Center&#8232;Howard Street, Between Third & Fifth Sts.&#8232;San Francisco, California, USA   Country:United States  

  • 低高度MHD擾乱からのCowling-channel抽出手法の開発 International conference

    吉川顕正

    The 33rd Symposium on Space and Upper Atmospheric Sciences in the Polar Regions  2009.11 

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    Event date: 2009.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所   Country:Japan  

  • Long-term Sq variation in the 210 magnetic meridian region International conference

    Yamazaki Y., K. Yumoto, T. Uozumi, and A. Yoshikawa

    URSI/COSPAR INTERNATIONAL REFERENCE IONOSPHERE WORKSHOP  2009.11 

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    Event date: 2009.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Inamori Hall, Kagoshima University, Kagoshima   Country:Japan  

  • 一般化Cowling効果の記述と電離圏対流の変形 International conference

    吉川顕正

    第5回 磁気圏-電離圏複合系における対流に関する研究会  2009.10 

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    Event date: 2009.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:名古屋大学 高等総合研究館1階カンファレンス室   Country:Japan  

  • 磁気圏電離圏結合電流系の包括的記述と理解:Alfvenic-coupling をベースとしたアプローチ

    吉川顕正, 田中良昌, 中田裕之, 中溝葵

    第126回 SGEPSS総会および講演会  2009.9 

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    Event date: 2009.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:金沢大学角間キャンパス   Country:Japan  

  • アルフェン波を介在したオーロラ帯の磁気圏電離圏結合

    田中良昌, 吉川顕正

    第126回 SGEPSS総会および講演会  2009.9 

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    Event date: 2009.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:金沢大学角間キャンパス   Country:Japan  

  • グローバルシミュレーションの為の一般化Alfvenic MI-couplingアルゴリズム

    吉川顕正

    JST/CREST「リアルタイム宇宙天気シミュレーションの研究」チーム成果発表会  2009.8 

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    Event date: 2009.8

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:九州地区国立大学共同研修所, 大分県九重町   Country:Japan  

  • 宇宙天気研究のための時系列データマイニングの応用~動的・へテロなシステムからの知識発見

    徳永旭将, 吉川顕正, 湯元清文

    H21年度名古屋大学太陽地球環境研究所「太陽地球惑星系統合型モデル・シミュレータ構築に向けた研究集会」  2009.8 

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    Event date: 2009.8

    Language:Others   Presentation type:Oral presentation (general)  

    Country:Japan  

  • Hall 共役電流法によるAlfvenic MI-coupling系のα・β channel separation Invited

    吉川顕正

    H21年度名古屋大学太陽地球環境研究所「太陽地球惑星系統合型モデル・シミュレータ構築に向けた研究集会」  2009.8 

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    Event date: 2009.8

    Language:Others   Presentation type:Oral presentation (invited, special)  

    Country:Japan  

  • Global MHD simulation using Alvenic-coupling algorithm (Yoshikawa algorithm)

    中田裕之, 吉川顕正

    H21年度名古屋大学太陽地球環境研究所「太陽地球惑星系統合型モデル・シミュレータ構築に向けた研究集会」  2009.8 

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    Event date: 2009.8

    Language:Others   Presentation type:Oral presentation (general)  

    Country:Japan  

  • Alfvenic-coupling algorithm for analysis of FAC system International conference

    Yoshikawa A

    The workshop on large-scale field-aligned current systems and associated processes in the magnetosphere and ionosphere  2009.7 

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    Event date: 2009.7

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:国立統計数理研究所   Country:Japan  

  • 磁気圏電離圏結合に於けるHall電流の発散により生成された分極場の役割

    吉川顕正

    日本地球惑星科学連合2009年大会  2009.5 

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    Event date: 2009.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉, 幕張国際会議場   Country:Japan  

  • Pi 2 型地磁気脈動の生成・伝播機構解明に関する知見獲得のための独立成分分析の応用

    徳永旭将, 吉川顕正, 魚住禎司, 樋口知之, 中村和幸, 湯元清文

    日本地球惑星科学連合2009年大会  2009.5 

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    Event date: 2009.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉, 幕張国際会議場   Country:Japan  

  • Annual and Semi-annual Variations of Equivalent Sq Current System along the 210 MM

    山崎洋介, 湯元清文, 吉川顕正

    日本地球惑星科学連合2009年大会  2009.5 

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    Event date: 2009.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉, 幕張国際会議場   Country:Japan  

  • 磁気圏電離圏結合における Hall 電流発散の役割

    吉川顕正

    平成20年度名古屋大学太陽地球環境研究所研究集会  2009.3 

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    Event date: 2009.3

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ   Country:Japan  

  • Convolutive Blind Source Separation of Pi 2 magnetic pulsations observed on the ground International conference

    Tokunaga T., A. Yoshikawa, T. Uozumi, K. Yumoto, MAGDAS Group

    International Symposium: Fifty Years after IGY - Modern Information Technologies and Earth and Solar Sciences  2008.11 

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    Event date: 2008.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:産業技術総合研究所つくば市   Country:Japan  

  • Electromagnetic MI-coupling algorithm through magnetic shear and compression flow for Global M-I coupled Simulation Invited International conference

    Yoshikawa A., A. Nakamizo, and T. Tanaka

    Michigan-Japan Space Science Workshop  2008.11 

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    Event date: 2008.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:University of Michigan, USA   Country:United States  

  • 地上多点ネットワークデータの活用:MAGDAS/ CPMNデータの料理の仕方 Invited

    吉川顕正

    第107回生存圏シンポジウム/SGEPSS波動分科会「磁気圏および宇宙空間のプラズマ波動の観測と理論」  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:日石仙台ビル   Country:Japan  

  • 地上多点同時観測されたPi 2型地磁気脈動への独立成分分析の適用–時空間混合モデル

    徳永 旭将, 吉川顕正, 魚住 禎司, 湯元 清文

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • Nighttime and Daytime Equatorial Pi 2 Pulsations Observed at the MAGDAS/CPMN Stations MAGDAS/CPMN

    平山有紀, 湯元清文, 魚住禎司, 吉川顕正

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • SFE*s observed at Dip-equator CPMN stations: Characteristics and possible mechanisms

    山崎洋介, 湯元清文, 吉川顕正, 亘慎一, 歌田久司

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • SFE*s observed at Dip-equator CPMN stations: Characteristics and possible mechanisms

    山崎洋介, 湯元清文, 吉川顕正, 亘慎一, 歌田久司

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • ULTIMAで求めた電離層Sq電流系の太陽風電場依存性

    寺田大師, 吉川顕正, 藤本晶子, 魚住禎司, 湯元清文

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • Separation of Sq current system into Cowling-Electrojet current channel using Hall conjugate current analysis

    吉川顕正, 陣英克, 三好勉信, 魚住禎司, 藤井良一, 宮原三郎, 糸長雅弘, 湯元清文

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • The realization of substorm processes by the eigenmode decomposition method in global MHD simulations

    中溝葵, 吉川顕正

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • 磁気圏電離圏間の対流・電流・物質流結合

    吉川顕正

    第2回GEMISISワークショップ  2008.8 

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    Event date: 2008.8

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:名古屋大学太陽地球環境研究所   Country:Japan  

  • 内部境界条件に於ける誘導効果とBrの処理:仮想モノポールの取り扱いについて

    吉川顕正

    STE研究集会「太陽地球/惑星系統合型モデル・シミュレータ構築に向けた研究集会  2008.8 

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    Event date: 2008.8

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:,地球シミュレーションセンター   Country:Japan  

  • Quantitative evaluations of substorm- associated Pi 2 magnetic pulsations observed at dayside equatorial latitudes by means of ICA

    Tokunaga T., A. Yoshikawa, T. Uozumi, K. Yumoto

    第32回極域宙空圏シンポジウム  2008.8 

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    Event date: 2008.8

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:東京、板橋、国立極地研究所   Country:Japan  

  • Formation of Cowling channel in the global ionosphere

    Yoshikawa A

    第32回極域宙空圏シンポジウム  2008.8 

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    Event date: 2008.8

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:東京、板橋、国立極地研究所   Country:Japan  

  • SFE*s Observed at Dip-equator CPMN Stations

    Yamazaki Y, K. Yumoto, A. Yoshikawa, S. Watari and H. Utada

    第32回極域宙空圏シンポジウム  2008.8 

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    Event date: 2008.8

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:東京、板橋、国立極地研究所   Country:Japan  

  • The Relationship Between the Two- dimensional Distribution Characteristics of Global Mode Pi 2 Pulsations Extracted by ICA and Auroral Breakups International conference

    Tokunaga, T., A. Yoshikawa, T. Uozumi., and K. Yumoto

    AOGS 2008 meeting  2008.6 

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    Event date: 2008.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Busan, Korea   Country:Korea, Republic of  

  • 3D-Cowling Channel Model in the Sq Current System, Invited International conference

    Yoshiawa A., Uozumi, T., and K. Yumoto

    AOGS 2008 meeting  2008.6 

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    Event date: 2008.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Busan, Korea   Country:Korea, Republic of  

  • The two-dimensional distribution of global mode Pi 2 pulsations extracted by Independent Component Analysis and the position of auroral breakup

    T. Tokunaga, A. Yoshikawa, T. Uozumi, K. Yumoto, CPMN Group

    日本地球惑星科学連合2008年大会  2008.5 

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    Event date: 2008.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張   Country:Japan  

  • Cowling効果同定の為のHall共役電流法の開発

    吉川顕正, 魚住禎司, 糸長雅弘, 湯元清文

    日本地球惑星科学連合2008年大会  2008.5 

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    Event date: 2008.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張   Country:Japan  

  • 磁気圏非定常MHD過程とその磁気圏-電離圏結合過程

    中溝葵, 吉川顕正

    日本地球惑星科学連合2008年大会  2008.5 

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    Event date: 2008.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張   Country:Japan  

  • Characteristics of Pi2 electric and magnetic pulsations observed at the low-latitude CPMN magnetometers and a FM-CW radar

    池田昭大, 湯元清文, 魚住禎司, 篠原学, 野崎憲朗 吉川顕正, 塩川和夫

    日本地球惑星科学連合2008年大会  2008.5 

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    Event date: 2008.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張   Country:Japan  

  • Nighttime and Daytime Equatorial Pi 2 Pulsations Observed at the MAGDAS/CPMN Stations

    平山有紀, 湯元清文, 魚住禎司, 吉川顕正, MAGDAS/CPMN Group

    日本地球惑星科学連合2008年大会  2008.5 

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    Event date: 2008.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張   Country:Japan  

  • Characteristics of SFEs observed at the dip-equator CPMN stations

    YAMAZAKI Y., K. YUMOT, A. YOSIKAWA, S. ABE, A. IKEDA, T.A TOKUNAGA, Y. NUMATA, S. WATARI, H. UTADA and Y. KIYOHUMI

    日本地球惑星科学連合2008年大会  2008.5 

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    Event date: 2008.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張   Country:Japan  

  • Hall conjugates current analysis for extraction of Cowling effect from nonuniform-anisotropically conducting ionospheric current system International conference

    Yoshikawa A.

    EISCAT International Symposium  2008.3 

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    Event date: 2008.3

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:NIPR, Tokyo   Country:Japan  

  • Sq研究の新展開

    吉川顕正, 魚住禎司, 三好勉信, 公田浩子, 平野隆, 糸長雅弘, 湯元清文顕正

    第3回ジオスペース環境科学研究会  2008.3 

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    Country:Japan  

  • 独立成分分析によって抽出されたグローバルなPi2型地磁気脈動の波動特性について

    徳永 旭将, 公田 浩子, 吉川 顕正, 魚住 禎司, 河野 英昭, 湯元 清文, 環太平洋地磁気観測グループ

    地球惑星科学関連学会合同大会  2006.5 

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    Language:Others   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ国際会議場   Country:Japan  

  • CPMNデータ解析に基づくSq中心の変動と沿磁力線電流・赤道ジェット電流の関係

    公田 浩子, 吉川 顕正, 魚住 禎司, 湯元 清文

    地球惑星科学関連学会合同大会  2006.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • Spatio-temporal development of ionospheric current system and its relation to atmospheric waveguide modes

    吉川 顕正

    幕張メッセ国際会議場  2006.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • Comparison between High-Latitude Pi 2 Pulsations Extracted by ICA (Independent Component Analysis) and AKR International conference

    T. Tokunaga, A. Morikawa, H. Kohta, A. Yoshikawa, T. Uozumi, K. Yumoto and MAGDAS/CPMN group

    Future Perspectives of Space Plasma and Particle Instrumentation and International Collaborations  2006.11 

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    Language:Others   Presentation type:Oral presentation (general)  

    Venue:立教大学   Country:Japan  

  • Some Features of Sq Dynamics Analyzed by MAGDAS/CPMN Data International conference

    H. Kohta, A. Yoshikawa, T. Uozumi, K. Yumoto and MAGDAS/CPMN Group

    Future Perspectives of Space Plasma and Particle Instrumentation and International Collaborations  2006.11 

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    Language:Others   Presentation type:Oral presentation (general)  

    Venue:立教大学   Country:Japan  

  • Comparison of the ionospheric electric field and the geomagnetic field at the time of SC International conference

    A. Ikeda, M. Shinohara, A. Yoshikawa, K. Nozaki, K. Yumoto

    Future Perspectives of Space Plasma and Particle Instrumentation and International Collaborations  2006.11 

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    Language:Others   Presentation type:Oral presentation (general)  

    Venue:立教大学   Country:Japan  

  • New coupling algorithm for global magnetosphere-ionosphere- thermosphere coupling simulation

    吉川 顕正

    地球電磁気・地球惑星圏学会第120回講演会  2006.11 

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    Language:Others   Presentation type:Oral presentation (general)  

    Venue:相模原産業会   Country:Japan  

  • MAGDAS/CPMNによるSqダイナミクス特性

    公田浩子, 吉川顕正, 魚住禎司, 湯元清文, MAGDAS/CPMNグループ

    地球電磁気・地球惑星圏学会第120回講演会  2006.11 

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    Venue:相模原産業会   Country:Japan  

  • 改良した磁気圏電離圏結合アルゴリズムを用いたグローバルMHDシミュレーション

    中田裕之, 吉川顕正, 田中高史

    地球電磁気・地球惑星圏学会第120回講演会  2006.11 

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    Venue:相模原産業会   Country:Japan  

  • Global Wave characteristics of Pi 2 Pulsations Extracted by Independent Component Analysis International conference

    T. Tokunaga, H. Kohta, A. Yoshikawa, T. Uozumi, H. Kawano, K. Yumoto

    AGU Fall Meeting  2006.12 

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    Venue:San Francisco   Country:United States  

  • Monitoring of Ionosphere-Atmosphere Electrodynamic Coupling by Geomagnetic Network Data International conference

    Hiroko KOHTA, Akimasa YOSHIKAWA, Teiji UOZUMI, Kiyohumi YUMOTO

    AGU Fall Meeting  2006.12 

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    Venue:San Francisco   Country:United States  

  • 磁気嵐シミュレータの方向性について

    吉川顕正

    名古屋大学太陽地球環境研究所研究集会  2007.2 

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    Venue:名古屋大学太陽地球環境研究所東山キャンパス   Country:Japan  

  • 磁気嵐シミュレータ検討会からの報告 Invited

    吉川顕正

    名古屋大学太陽地球環境研究所研究集会  2007.3 

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    Venue:情報通信機構   Country:Japan  

  • 3次元電離圏におけるCowling Channelの形成モデル

    吉川顕正, 川野圭子, 魚住禎司, 公田浩子, 宮原三郎, 湯元清文

    日本地球惑星科学連合大会  2007.5 

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    Venue:幕張メッセ, 千葉   Country:Japan  

  • Independent Component Analysis of Nightside Magnetospheric Forced Pi2 Oscillations ovserved at the CPMN Stations

    Tokunaga T., H. Kohta, A. Yoshikawa, T. Uozumi, H. Kawano, K. Yumoto and CPMN/MAGDAS Group

    日本地球惑星科学連合大会  2007.5 

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    Venue:幕張メッセ, 千葉   Country:Japan  

  • Change in Ionospheric Electric Field and Geomagnetic Field due to Solar Wind Variations at the time of SC International conference

    Ikeda A., M.Shinohara, A.Yoshikawa, K.Nozaki, A.Shinbori, K.Yumoto

    IAGA at the IUGG General Assembly 2007  2007.7 

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    Venue:Perugia, 2-13 July   Country:Italy  

  • Cowling channel formation model in the 3d-ionosphere, International conference

    A. Yoshikawa

    IAGA at the IUGG General Assembly 2007  2007.7 

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    Venue:Perugia, 2-13 July   Country:Italy  

  • 3D-Cowling effect in the Sq current system Invited International conference

    A. Yoshikawa

    ISSI teams meeting for "Ionosphere-magnetosphere coupling and induction effects in a three-dimensional ionosphere model"  2007.9 

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    Language:Others   Presentation type:Symposium, workshop panel (public)  

    Venue:International Space Science Institute, Bern, Switzerland, 5-9 September, 2007.   Country:Switzerland  

  • 3D-Cowling Channel Model in the Sq Current System

    吉川顕正, 公田浩子, 川野圭子, 魚住禎司, 藤井良一, 宮原 三郎, 湯元 清文

    第122回地球電磁気・地球惑星圏学会  2007.9 

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    Venue:名古屋大学野依記念学術交流館   Country:Japan  

  • Sq-EEJ電流系の三次元結合モデル

    吉川顕正

    STE研究所研究集会 『第4回 磁気圏-電離圏複合系における対流に関する研究会』  2007.11 

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    Language:Others   Presentation type:Oral presentation (general)  

    Country:Japan  

  • Hall conjugates current analysis for extraction of Cowling effect from nonuniform-anisotropically conducting ionospheric current system International conference

    A. Yoshikawa

    EISCAT International Symposium  2008.3 

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    Venue:NIPR,TOKYO   Country:Japan  

  • Quantum Calculation of Classical Kinetic Equations: A Novel Approach for Numerical Analysis of 6D Boltzmann-Maxwell Equations in Collisionless Plasmas Using Quantum Computing

    Hayato Higuchi, Juan William Pedersen, Akimasa Yoshikawa

    2023.6 

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    Event date: 2023.6

    A novel quantum algorithm for solving the Boltzmann-Maxwell equations of the
    6D collisionless plasma is proposed. The equation describes the kinetic
    behavior of plasma particles in electromagnetic fields and is known for the
    classical first-principles equations in various domains, from space to
    laboratory plasmas. We have constructed a quantum algorithm for a future
    large-scale quantum computer to accelerate its costly computation. This
    algorithm consists mainly of two routines: the Boltzmann solver and the Maxwell
    solver. Quantum algorithms undertake these dual procedures, while classical
    algorithms facilitate their interplay. Each solver has a similar structure
    consisting of three steps: Encoding, Propagation, and Integration. We conducted
    a preliminary implementation of the quantum algorithm and performed a parallel
    validation against a comparable classical approach. IBM Qiskit was used to
    implement all quantum circuits.

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    Other Link: http://arxiv.org/pdf/2306.05967v1

  • Multi-spacecraft observations of widespread solar proton transport in the heliosphere

    OBARA Takahiro, YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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    Event date: 2023

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  • 太陽フレア発生時のシューマン共鳴の特性

    池田昭大, 魚住禎司, 吉川顕正, 藤本晶子, 阿部修司

    大気電気学会誌(Web)  2023 

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  • Large-scale research project “Study of coupling processes in the solar-terrestrial system“

    山本衛, 小川泰信, 塩川和夫, 吉川顕正, 岩井一正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Mid- and low-latitude electric fields response to CW development during isolated substorms

    林萌英, 吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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    Event date: 2023

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  • Quasi-6-Day Wave Modulation of the Inter-Hemispheric Field-Aligned Currents (IHFACs)

    高山久美, 吉川顕正, 三好勉信

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Schumann resonance parameters at Kuju and global lightning activity

    IKEDA Akihiro, UOZUMI Teiji, YOSHIKAWA Akimasa, FUJIMOTO Akiko, ABE Shuji

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Extraction model of ionospheric echoes for time-series ionogram images based-on penalized motion detection

    HIROSHIGE Yu, FUJIMOTO Akiko, IKEDA Akihiro, ABE Shuji, YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • CEJ Effects on Plasma Bubble Generation

    加藤彰紘, 吉川顕正, 藤本晶子

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • On the global characteristics of Pi2 and Pc4 wave generation associated with substorms

    橋本明史, 吉川顕正, 魚住禎司

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • A study on the impact of Sprites on the Global Electrical Circuit by ELF electromagnetic wave observation

    古谷享一, 吉川顕正, 池田昭大

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Geomagnetic Field Observation Project by YOTSUBA-KULOVER Satellite with COTS Magnetomete

    KITAMURA Kentarou, MASUI Hirokazu, ABE Shuji, UOZUMI Teiji, TERAMOTO Mariko, FUJIMOTO Akiko, SANO Kei, YOSHIKAWA Akimasa, CHO Mengu

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Evolution of M-I convection depending on the Alfven conductance as simulated by global MHD model with Alfvenic coupling

    NAKAMIZO Aoi, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa, NAKATA Hiroyuki, FUKAZAWA Keiichiro, TANAKA Takashi

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Multiple-event study of substorm electric-field penetration based on simultaneous observation of 630-nm airglow enhancements

    森田早紀, 塩川和夫, 大塚雄一, 西谷望, 新堀淳樹, 惣宇利卓弥, 藤本晶子, 吉川顕正, 西岡未知, PERWITASARI Septi, 山本衛

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Analysis of electromagnetic field structure in the auroral acceleration region using 3D collisional Hall MHD simulation

    川上航典, 吉川顕正, 深沢圭一郎

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Self-Consistent Quantum Calculations of the 6D Boltzmann-Maxwell System in Collisionless Plasmas Using Quantum Computer

    樋口颯人, PEDERSEN Juan William, 吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • The Impact of the Geomagnetic Storm Event of February 2022 on the Inner Radiation Belt by Test Particle Simulations

    GIRGIS Kirolosse, HADA Tohru, MATSUKIYO Shuichi, MATSUKIYO Shuichi, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa, CHIAN Abraham, CHIAN Abraham

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Severe erosion of the plasmasphere caused by the ring current particle injection into the deep inner magnetosphere

    尾花由紀, 吉川顕正, 丸山奈緒美, 新堀淳樹, 中村紗都子, JUN ChaeWoo, 堀智昭, 三好由純, 橋本久美子, 熊本篤志, 土屋史紀, 笠原禎也, 松岡彩子, 風間洋一, WANG Shiang-Yu, 浅村和史, 篠原育, 横田勝一郎, 桂華邦裕, 笠原慧

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Development of Affine connections to describe 3D evolving magnetic vector fields and its application to space physics

    YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • An Education Program for CubeSat Development Under Collaboration Between Engineering and Science Faculties in Different Universities

    北村健太郎, 増井博一, 魚住禎司, 寺本万里子, 藤本晶子, CHO Meng, 阿部修司, 吉川顕正

    宇宙科学技術連合講演会講演集(CD-ROM)  2023 

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  • Research on the characteristics of equatorial electrojet occurrence with a peculiar decreasing trend

    池末暉, 吉川顕正, 藤本晶子

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Search for geomagnetic variation of equatorial electrojet using string matching and its application

    西口稜真, 吉川顕正, 藤本晶子

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • Scattered perpendicular flow speed in the dayside reconnection regions due to change in the IMF Bz direction

    橋本翼, 吉川顕正, 田中高史

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2023 

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  • シューマン共鳴の経験モデルの作成

    久永, 学実, 池田, 昭大, 藤本, 晶子, 古川, 翔大, 吉川, 顕正, 魚住, 禎司, 阿部, 修司

    2022.1 

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    Language:Japanese  

    Country:Other  

    type:Conference Paper
    第27回高専シンポジウム, 2022年1月22日, オンライン開催
    source:https://kosen-sympo.org/

  • シューマン共鳴の経験モデルの作成

    久永, 学実, 池田, 昭大, 藤本, 晶子, 古川, 翔大, 吉川, 顕正, 魚住, 禎司, 阿部, 修司

    2022.1 

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    Event date: 2022.1

    Language:Japanese  

    type:Conference Paper
    第27回高専シンポジウム, 2022年1月22日, オンライン開催
    source:https://kosen-sympo.org/

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  • Study of the response of the Earth’s magnetosphere to a Sun-Earth oriented interplanetary magnetic field

    城戸蓮太郎, 吉川顕正, 吉川顕正, 魚住禎司

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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    Event date: 2022

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  • A Numerical Simulation of the Formation of Poleward Boundary Intensifications of Auroral Emission due to Ionospheric Polarization

    森澤将, 吉川顕正, 大谷晋一

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • Study of coupling processes in the solar-terrestrial system

    山本衛, 小川泰信, 塩川和夫, 吉川顕正, 吉川顕正

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • Eastward Magnetic Variations in the Equatorial Latitude Associated with the IHFAC Observed on the Ground and LEO

    KITAMURA Kentarou, KITAMURA Kentarou, FUJIMOTO Akiko, FUJIMOTO Akiko, TERAMOTO Mariko, TERAMOTO Mariko, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa, ABE Shuji

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Comparison of Magnetic Variations Associated with the IHFAC Observed on the Ground and in the LEO

    KITAMURA Kentarou, FUJIMOTO Akiko, YOSHIKAWA Akimasa, ABE Shuji

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • Clarifying Horizontal Vectors of Magnetic Fields Using Principal Component Analysis

    高山久美, 吉川顕正, 三好勉信

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Investigation of the response of magnetic and electric fields in mid-latitude to the development of CW during substorms

    林萌英, 吉川顕正, 吉川顕正, 藤本晶子, OHTANI Shinichi

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Comparison of general object detection models for Ionogram sporadic E layer echoes detection

    HIROSHIGE Yu, FUJIMOTO Akiko, ABE Shuji, IKEDA Akihiro, YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • Disruption of accumulated northward IMF lines in the dayside magnetosheath due to discontinuous southward turning of IMF

    HASHIMOTO Tsubasa, YOSHIKAWA Akimasa, TANAKA Takashi

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • Analysis of EEJ structure in M-I coupling system using IGRF model and quasi-three-dimensional potential solver

    伊集院拓也, 吉川顕正, 三好勉信, 品川裕之, 藤原均, 陣英克, 中溝葵, 垰千尋, 塩川和夫

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • High available of general object detection models for detection of E/Es layer echo on FM-CW Ionograms

    HIROSHIGE Yu, FUJIMOTO Akiko, ABE Shuji, IKEDA Akihiro, YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Evolution of electrostatic potential in magnetosphere-ionospheric system as simulated by global MHD model with Alfvenic-coupling

    NAKAMIZO Aoi, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa, NAKATA Hiroyuki, FUKAZAWA Keiichiro, TANAKA Takashi

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Evolution of electrostatic potential in magnetosphere-ionosphere system as simulated by global MHD model with Alfvenic-coupling

    NAKAMIZO Aoi, YOSHIKAWA Akimasa, NAKATA Hiroyuki, FUKAZAWA Keiichiro, TANAKA Takashi

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • On the electron acceleration process as a carrier of field-aligned current and its energy conversion process in the Alfven wavefront

    YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • M-I Coupling at High Latitude via Alfven Waves; Combined Effects through Polarization, Induction and Conductance Evolution

    森澤将, 吉川顕正, 吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Development of Quantum Algorithm for Clarifying Auroral Electron Acceleration Mechanism by Collisional Boltzmann-Maxwell Equation

    樋口颯人, 吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Physics of Magnetosphere-Ionosphere Coupling System from the Collisional Three-Fluid Model.

    樋口颯人, 吉川顕正

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • How is stacked northward IMF removed from the dayside magnetosheath region due to the southward IMF reversal?

    橋本翼, 吉川顕正, 田中高史

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Schumann resonance parameters at Kuju during intense solar activity

    IKEDA Akihiro, UOZUMI Teiji, YOSHIKAWA Akimasa, FUJIMOTO Akiko, ABE Shuji

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Characteristics and Causes of Morning side Pc3 Pulsations

    小原隆博, 吉川顕正, 魚住禎司, 阿部修司

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • Development of Affine Connection for Describing Spatiotemporal Evolving 3D Magnetic Vector Fields

    吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2022 

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  • Recent activities and future plans of MAGDAS project under new organization

    ABE Shuji, FUJIMOTO Akiko, UOZUMI Teiji, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • Control of switching two observation modes on FM-CW ionospheric observation system based on reinforcement learning

    FUJIMOTO Akiko, MIKURIYA Toru, ABE Shuji, IKEDA Akihiro, YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • Modeling of Magnetosphere-Ionosphere-Atmosphere System to Elucidate the Coupling Process in the Space-Earth Transition Region

    YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)  2022 

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  • Seasonal variation of inter-hemispheric field-aligned currents deduced from time-series analysis of the equatorial geomagnetic field data during solar cycle 23–24

    Manjula Ranasinghe, Akiko Fujimoto, Akimasa Yoshikawa, Chandana Jayaratne

    Earth, Planets and Space  2021.12  SPRINGER

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    Event date: 2021.12

    Language:English  

    The east–west component of magnetic field variation (∆D-component) at Davao station (Philippines, geomagnetic latitude: – 2.22˚N) are used to investigate the characteristics of the long-term Inter-Hemispheric Field-Aligned Currents (IHFACs) based on the time-series analysis from August 1998 to July 2020. Recent in situ satellite and ground-based observations have reported that dusk-side current polarity of IHFAC is often opposite to that of the noon IHFAC, being inconsistent with Fukushima's IHFACs model. We investigated the consistency of the dusk-side IHFAC polarity derived from the observations with the polarity expected from Fukushima’s IHFACs model and examined the solar cycle dependence of IHFACs. It was confirmed that the dusk-side IHFACs during June and December solstices flow in the same direction of the noontime IHFACs, which was consistent with the IHFAC polarities suggested by the Fukushima model. The dusk-side IHFACs around March and September–November months disagreed with the Fukushima model. The ∆D variations clearly showed seasonal asymmetry in the dawn and noon sectors, whereas the ∆D variations in the dusk sector demonstrated seasonal symmetry. Solar cycle dependence of IHFACs was exhibited in the dusk sector. For the dawn and noon sectors, the yearly peak-to-peak ∆D amplitude in the later solar cycle SC24 decreased by about 35% in comparison with the earlier solar cycle SC23. In contrast, the dusk-side yearly peak-to-peak ∆D amplitude increased by about 200%. The dusk-side IHFAC yearly amplitude tended to be in inverse proportion to solar activity. [Figure not available: see fulltext.]

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    Other Link: https://link.springer.com/content/pdf/10.1186/s40623-021-01481-6.pdf

  • 磁気赤道域における特異的な太陽フレア効果(SFE*)の発生要因の探究—Research on the causes of specific solar flare effects (SFE∗) in the dip equator

    安永, 朗宏, 藤本, 晶子, 吉川, 顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2021.10 

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    Event date: 2021.10

    Language:Japanese  

    Country:Other  

    Research on the causes of specific solar flare effects (SFE*) in the dip equator

  • Research on the causes of specific solar flare effects (SFE*) in the dip equator

    安永朗宏, 藤本晶子, 吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2021.10 

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    Event date: 2021.10

    Language:Japanese  

    type:Conference Paper
    第150回地球電磁気・地球惑星圏学会(SGEPSS)総会および講演会, 2021年10月31日-11月4日

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  • Study of coupling processes in the solar-terrestrial system=Current status in 2021=

    YAMAMOTO Mamoru, HASHIGUCHI Hiroyuki, YOKOYAMA Tatsuhiro, MIYAOKA Hiroshi, OGAWA Yasunobu, SHIOKAWA Kazuo, NOZAWA Satonori, YOSHIKAWA Akimasa, TSUDA Toshitaka

    日本地球惑星科学連合大会予稿集(Web)  2021 

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    Event date: 2021

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  • Characteristics of dusk-side IHFAC polarity during storm and quiet times

    FUJIMOTO Akiko, YOSHIKAWA Akimasa, RANASINGHE Manjula, JAYARATNE Chandana

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2021 

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    Event date: 2021

    Language:English  

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  • Implementation of Alfvenic Coupling in Global MHD Magnetosphere Simulation

    NAKAMIZO Aoi, YOSHIKAWA Akimasa, NAKATA Hiroyuki, FUKAZAWA Keiichiro, TANAKA Takashi

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2021 

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  • Characteristics of wave in the plasmasphere during global-mode wave events: Analysis of data from ground magnetometers at middle and low latitudes

    YAMATANI Yuta, KAWANO Hideaki, KAWANO Hideaki, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa

    極域科学シンポジウム(Web)  2021 

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    Event date: 2021

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  • Progress of the SDR-based dual-band scintillation detector development and its application for space weather study

    ABE Shuji, FUJIMOTO Akiko, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2021 

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    Event date: 2021

    Language:English  

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  • D-region ionospheric effects for 2016 eruptions of Mt. Aso using LF transmitter signals

    OHYA Hiroyo, ORITO Yuhi, TSUCHIYA Fuminori, YAMAMOTO Masa-yuki, NAKATA Hiroyuki, YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)  2021 

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  • Feasibility Study of Space Weather Observation by CubeSat in LEO

    KITAMURA Kentarou, CHO Mengu, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa, UOZUMI Teiji, ABE Shuji, TERAMOTO Mariko, FUJIMOTO Akiko

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2021 

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    Event date: 2021

    Language:English  

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  • The magnetospheric plasma density profile on the Japanese meridian plane: Its dependence on the magnetospheric and sun-related activities

    ONAKA Aoi, KAWANO Hideaki, KAWANO Hideaki, UOZUMI Teiji, ABE Shuji, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa

    極域科学シンポジウム(Web)  2021 

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    Event date: 2021

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  • Seasonal and long-term variations in the Schumann Resonance observed at Kuju Japan

    IKEDA Akihiro, UOZUMI Teiji, YOSHIKAWA Akimasa, FUJIMOTO Akiko, ABE Shuji

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2021 

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    Event date: 2021

    Language:English  

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  • Development of an autonomous FM-CW ionospheric observation system based on reinforcement learning

    MIKURIYA Toru, FUJIMOTO Akiko, ABE Shuji, IKEDA Akihiro, YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)  2021 

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    Event date: 2021

    Language:English  

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  • Implementation of SDR-based scintillation detector system and preliminary observation with magnetometer and radar

    Shuji Abe, Akiko Fujimoto, Akimasa Yoshikawa

    地球電磁気・地球惑星圏学会 第148回 総会・講演会(2020年 秋学会)  2020.11 

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    Event date: 2020.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Country:Other  

  • 朝側Pc-3 の出現を決める太陽風磁場の方向について

    小原 隆博, 吉川 顕正, 魚住 禎, 阿部 修司

    地球電磁気・地球惑星圏学会 第148回 総会・講演会(2020年 秋学会)  2020.11 

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    Event date: 2020.11

    Language:Japanese  

    Country:Other  

  • Seasonal dependence of semidiurnal equatorial magnetic variation during quiet and disturbed periods

    Akiko Fujimoto, Akimasa Yoshikaw, Teiji Uozumi, Shuji Abe

    地球電磁気・地球惑星圏学会 第148回 総会・講演会(2020年 秋学会)  2020.11 

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    Event date: 2020.11

    Language:Japanese  

    Country:Other  

  • Schumann resonance parameters at Kuju during solar flares and solar proton events

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikaw, Akiko Fujimoto, Shuji Abe

    地球電磁気・地球惑星圏学会 第148回 総会・講演会(2020年 秋学会)  2020.11 

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    Event date: 2020.11

    Language:English  

    Country:Other  

  • Characterization of counter electrojet current according to specific time frame in Southeast Asian sector International conference

    Nur Izzati Mohd Rosli, Nurul Shazana Abdul Hamid, Mardina Abdullah、Akimasa Yoshikawa, Teiji Uozumi

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Event date: 2020.7

    Language:English   Presentation type:Oral presentation (general)  

    Country:Other  

  • Correlations of earthquake properties with geomagnetic ULF precursor characteristics over multiple events International conference

    Muhammad Khairul Adib Muhammad Yusof, Mardina Abdullah, Nurul Shazana Abdul Hamid, Suaidi Ahadi, Akimasa Yoshikawa

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Event date: 2020.7

    Language:English   Presentation type:Oral presentation (general)  

    Country:Other  

  • 3D current system of auroral vortices in the discrete arc estimated by auroral tomography and local KRM methods International conference

    田中 良昌, 小川 泰信, 門倉 昭, 西山 尚典, 吉川 顕正, Gustavsson Bjorn, Kauristie Kirsti, Enell Carl-fredrik、Brandstrom Urban, Sergienko Tima, Kozlovsky Alexander, Raita Tero, Vanhamaki Heikki

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Event date: 2020.7

    Language:English   Presentation type:Oral presentation (general)  

    Venue:オンライン   Country:Other  

  • Development of SDR-based scintillation detector system integrated with MAGDAS project

    藤本 晶子, 阿部 修司, 吉川 顕正

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Language:English  

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  • Comparison of FM-CW Ionosonde and MAGDAS observations with S4 index in Peru during 15-18 March 2019 International conference

    藤本 晶子, 吉川 顕正, 池田 昭大, 阿部 修司, 林 萌英

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Event date: 2020.7

    Language:English   Presentation type:Oral presentation (general)  

    Country:Other  

  • Longitudinal Variation and Peak Time of Equatorial Electrojet Current from Ground and Satellite Measurements

    Nurul Shazana Abdul Hamid, Wan Nur Izzaty Ismail, Mardina Abdullah、Akimasa Yoshikawa, Teiji Uozumi, Zahira Mohd Razi

    JpGU-AGU Joint Meeting 2020  2020.7 

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  • 太陽地球系結合過程の研究基盤形成 =計画の現状2020=

    山本 衛, 橋口 浩之, 横山 竜宏, 宮岡 宏, 小川 泰信, 塩川 和夫, 野澤 悟, 吉川 顕正, 津田 敏隆

    JpGU-AGU Joint Meeting 2020  2020.7 

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  • サブストーム中における近地球磁気圏内での磁場変動の緯度方向分布

    今城 峻, 能勢 正仁, 相田 真里, 東尾 奈々, 松本 晴久, 古賀 清一, 吉川 顕正, 三好 由純

    JpGU-AGU Joint Meeting 2020  2020.7 

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    Country:Other  

  • Recent and future activities of ICSWSE and MAGDAS project

    阿部 修司, 藤本 晶子, 魚住 禎司, 吉川 顕正

    jpGU-AGU Joint Meeting 2020  2020.7 

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  • Dynamics of the Ionosphere/Plasmasphere System: Comparisons Between Arase/PWE and the IPE Model

    Yuki Obana, Naomi Maruyama, Atsuki Shinbori, Kumiko Hashimoto, Mariangel Fedrizzi, Masahito Nose, Yuichi Otsuka, Nozomu Nishitani, Tomoaki Hori, Atsushi Kumamoto, Fuminori Tsuchiya, Shoya Matsuda, Ayako Matsuoka, Yoshiya Kasahara, Akimasa Yoshikawa, Yoshizumi Miyosh, Iku Shinohara

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • MIセンサを用いた地磁気微小変動のテスト観測

    中村 拓真, 能勢 正仁, 阿部 修司, 魚住 禎司, 吉川 顕正, 青山 均, 河野 剛健, 北村 健太郎

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • 日本子午面上のプラズマ密度分布

    #糸山 隆仁, @河野 英昭, @魚住 禎司, @阿部 修司, @吉川顕正

    第146回地球電磁気・地球惑星圏学会総会・講演会(2019年秋学会)  2019.10 

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    Event date: 2019.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:熊本市国際交流会館 (熊本市中央区)   Country:Japan  

  • Seasonal dependence of semidiurnal equatorial magnetic variation during quiet and disturbed periods

    Akiko Fujimoto, Akimasa Yoshikawa, Teiji Uozumi, Shuji Abe

    10th Anniversary International Conference on Solar-Terrestrial Relations and Physics of Earthquake Precursors, STRPEP 2019  2019.11 

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    Event date: 2019.10

    Language:English  

    Venue:Paratunka   Country:Russian Federation  

    The analysis of 20-year long-term semidiurnal lunar tidal variations gave the evidence that the semidiurnal variations are completely different between the magnetic quiet and disturbed periods. This is the first time that the seasonal dependence of disturbance-time semidiurnal variation has been provided from the analysis of the EE-index. We found the Kp dependence of semidiurnal variation: For full and new moon phase, counter troughs are amplified during disturbance time, possibly related to disturbance dynamo. For all moon phase, there are positive enhancements in dawn and strong depressions after sunset, resulting from the penetration of polar electric filed. For Seasonal dependence, semidiurnal variations are divided to three seasonal groups, and characterized as deep trough, enhanced crest and weak structure for D-solstice, Equinoxes and J-solstice, respectively. There is no significant longitudinal difference between Ancon and Davao, except for the amplitude of semidiurnal variations. The deep troughs occur during D-solstice and the enhanced crests during Equinoxes, at both Ancon and Davao.

  • Axisymmetric conductivities of Jupiter's middle- and low-latitude ionosphere

    中村勇貴, 寺田綱一郎, 垰千尋, 寺田直樹, 笠羽康正, 北元, 中溝葵, 吉川顕正, 大谷晋一, 土屋史紀, 鍵谷将人, 坂野井健, 村上豪, 吉岡和夫, 木村智樹, 山崎敦, 吉川一朗

    日本地球惑星科学連合2019年大会  2019.5 

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    Event date: 2019.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張メッセ   Country:Japan  

  • An extreme erosion of the plasmasphere during the 7–10 September 2017 storm

    尾花 由紀, 丸山 奈緒美, 新堀 淳樹, 橋本 久美子, Fedrizzi Mariangel, 能勢 正仁, 大塚 雄一, 西谷 望, 堀 智昭, 熊本 篤志, 土屋 史紀, 松田 昇也, 松岡 彩子, 笠原 禎也, 吉川 顕正, 三好 由純, 篠原 育

    日本地球惑星科学連合2019年大会  2019.5 

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    Event date: 2019.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉、幕張メッセ   Country:Japan  

  • Statistical Study of Selective Transport of Energetic Oxygen Ions During Magnetic Storms Observed by Van Allen Probes in 2013-20

    Kenji Mitani, Kanako Seki, Kunihiro Keika[, Matina Gkioulidou, Louis J. Lanzerotti, Donald Mitchell, Craig A. Kletzing, Akimasa Yoshikawa, Yuki Obana

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • Contribution of ULF and chorus waves to the radiation belt dynamics based on Arase observations and BATSRUS+CRCM simulation

    Naoko Takahashi, Kanako Seki, Mariko Teramoto, Mei-Ching Fok, Yihua Zheng, Kazuo Shiokawa, Dmitry Baishev, Akimasa Yoshikawa, Tsutomu Nagatsuma, Ayako Matsuoka, Yoshiya Kasahara, Nana Higashio, David Hartley

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • FLR の自動同定とそれを用いた磁気嵐中の磁気圏プラズマ密度の解析

    #篠置 仁崇, @河野 英昭, Mann Ian R., 林 幹治, @吉川 顕正, @MAGDAS/CPMN グループ 吉川 顕正

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • Axisymmetric conductivities of Jupiter’s middle- and low-latitude ionosphere

    Yuki Nakamura, Koichiro Terada, Chihiro Tao, Naoki Terada, Yasumasa Kasaba, Hajime Kita, Aoi Nakamizo, Akimasa Yoshikawa, Shinichi Ohtani, Fuminori Tsuchiya, Masato Kagitani, Takeshi Sakanoi, Go Murakami, Kazuo Yoshioka, Tomoki Kimura, Atsushi Yamazaki, Ichiro Yoshikaw

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • Tomography analysis of westward traveling surge observed in February, 2018

    Yoshimasa Tanaka, Yasunobu Ogawa, Akira Kadokura, Takanori Nishiyama, Akimasa Yoshikawa

    第144回 地球電磁気・地球惑星圏学会総会・講演会(2018年 秋学会)  2018.11 

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    Event date: 2018.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:名古屋大学東山キャンパス   Country:Japan  

  • Global response of Magnetic field and Ionosonde observations to intense solar flares on 6 and 10 September 2017

    Akiko Fujimoto, Akimasa Yoshikawa, Akihiro Ikeda

    9th International Conference "Solar-Terrestrial Relations and Physics of Earthquake Precursors", STRPEP 2018  2018.11 

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    Event date: 2018.10

    Language:English  

    Venue:Paratunka, Kamchatka Region   Country:Russian Federation  

    Intense X-ray fluxes during solar flares are known to cause enhanced ionization in the Earth's ionospheric D, E and F region. This sudden change of ionospheric electron density profile is serious problem to radio wave communication and navigation system. The ground magnetograms often record the sudden change in the sunlit hemisphere during the enhanced X-ray flux, due to the sudden increase in the global ionospheric current system caused by the flare-induced enhanced ionospheric conductivity. These geomagnetic field disturbances are known as "solar flare effects" (SFEs) or geomagnetic crochets [Campbell, 2003]. The typical SFE is increase variation on the equatorial magnetic data. On Ionosonde observation during solar flare event, the High-Frequency (HF) radio wave blackout is often detected in ionogram due to the sudden disturbance in ionosphere. Two intense X-class solar flares occurred on 6 and 10 September 2017. We investigated the magnetic field and Ionosonde responses to the intense solar flare events. Dayside magnetic field variations sudden increased due to the ionospheric disturbance resulting from solar flare. There is no response in night side magnetometer data. The magnitude of SFE (magnetic field) is independent of solar flare X-ray magnitude. We found HF radio wave blackout in ionogram at dayside Ionosonde stations. The duration of blackout is dependent of latitude and local time of Ionosonde stations. There is the different feature of ionogram at night side.

  • Schumann resonance parameters at Kuju station during solar flares

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe

    9th International Conference "Solar-Terrestrial Relations and Physics of Earthquake Precursors", STRPEP 2018  2018.11 

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    Event date: 2018.10

    Language:English  

    Venue:Paratunka, Kamchatka Region   Country:Russian Federation  

    We examined the Schumann resonance (SR) at low-latitude station KUJ by comparing with solar X-ray flux and solar proton flux at a geostationary orbit. For intense solar activity in October-November 2003, the reaction of the SR frequency to X-ray enhancement and SPEs was different. The SR frequency in H component increased at the time of the Xray enhancement. The response of SR seems to be caused by the increase of the electron density in the ionospheric D region which ionized by the enhanced solar X-ray flux. In the case of the SPEs, the SR frequency in D component decreased with enhancement of solar proton flux. We suggest that the SPEs caused the decrease of altitude on the ionopheric D region at high-latitude region, and the SR frequency decreased.

  • Global response of Magnetic field and Ionosonde observations to intense solar flares on 6 and 10 September 2017

    Akiko Fujimoto, Akimasa Yoshikawa, Akihiro Ikeda

    9th International Conference "Solar-Terrestrial Relations and Physics of Earthquake Precursors", STRPEP 2018  2018.11 

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    Event date: 2018.10

    Language:English  

    Venue:Paratunka, Kamchatka Region   Country:Russian Federation  

    Intense X-ray fluxes during solar flares are known to cause enhanced ionization in the Earth's ionospheric D, E and F region. This sudden change of ionospheric electron density profile is serious problem to radio wave communication and navigation system. The ground magnetograms often record the sudden change in the sunlit hemisphere during the enhanced X-ray flux, due to the sudden increase in the global ionospheric current system caused by the flare-induced enhanced ionospheric conductivity. These geomagnetic field disturbances are known as "solar flare effects" (SFEs) or geomagnetic crochets [Campbell, 2003]. The typical SFE is increase variation on the equatorial magnetic data. On Ionosonde observation during solar flare event, the High-Frequency (HF) radio wave blackout is often detected in ionogram due to the sudden disturbance in ionosphere. Two intense X-class solar flares occurred on 6 and 10 September 2017. We investigated the magnetic field and Ionosonde responses to the intense solar flare events. Dayside magnetic field variations sudden increased due to the ionospheric disturbance resulting from solar flare. There is no response in night side magnetometer data. The magnitude of SFE (magnetic field) is independent of solar flare X-ray magnitude. We found HF radio wave blackout in ionogram at dayside Ionosonde stations. The duration of blackout is dependent of latitude and local time of Ionosonde stations. There is the different feature of ionogram at night side.

  • Schumann resonance parameters at Kuju station during solar flares

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe

    9th International Conference "Solar-Terrestrial Relations and Physics of Earthquake Precursors", STRPEP 2018  2018.11 

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    Event date: 2018.10

    Language:English  

    Venue:Paratunka, Kamchatka Region   Country:Russian Federation  

    We examined the Schumann resonance (SR) at low-latitude station KUJ by comparing with solar X-ray flux and solar proton flux at a geostationary orbit. For intense solar activity in October-November 2003, the reaction of the SR frequency to X-ray enhancement and SPEs was different. The SR frequency in H component increased at the time of the Xray enhancement. The response of SR seems to be caused by the increase of the electron density in the ionospheric D region which ionized by the enhanced solar X-ray flux. In the case of the SPEs, the SR frequency in D component decreased with enhancement of solar proton flux. We suggest that the SPEs caused the decrease of altitude on the ionopheric D region at high-latitude region, and the SR frequency decreased.

  • Global response of Magnetic field and Ionosonde observations to intense solar flares on 6 and 10 September 2017

    Akiko Fujimoto, Akimasa Yoshikawa, Akihiro Ikeda

    9th International Conference "Solar-Terrestrial Relations and Physics of Earthquake Precursors", STRPEP 2018  2018.11 

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    Event date: 2018.10

    Language:English  

    Venue:Paratunka, Kamchatka Region   Country:Russian Federation  

    Intense X-ray fluxes during solar flares are known to cause enhanced ionization in the Earth's ionospheric D, E and F region. This sudden change of ionospheric electron density profile is serious problem to radio wave communication and navigation system. The ground magnetograms often record the sudden change in the sunlit hemisphere during the enhanced X-ray flux, due to the sudden increase in the global ionospheric current system caused by the flare-induced enhanced ionospheric conductivity. These geomagnetic field disturbances are known as "solar flare effects" (SFEs) or geomagnetic crochets [Campbell, 2003]. The typical SFE is increase variation on the equatorial magnetic data. On Ionosonde observation during solar flare event, the High-Frequency (HF) radio wave blackout is often detected in ionogram due to the sudden disturbance in ionosphere. Two intense X-class solar flares occurred on 6 and 10 September 2017. We investigated the magnetic field and Ionosonde responses to the intense solar flare events. Dayside magnetic field variations sudden increased due to the ionospheric disturbance resulting from solar flare. There is no response in night side magnetometer data. The magnitude of SFE (magnetic field) is independent of solar flare X-ray magnitude. We found HF radio wave blackout in ionogram at dayside Ionosonde stations. The duration of blackout is dependent of latitude and local time of Ionosonde stations. There is the different feature of ionogram at night side.

  • Schumann resonance parameters at Kuju station during solar flares

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe

    9th International Conference "Solar-Terrestrial Relations and Physics of Earthquake Precursors", STRPEP 2018  2018.11 

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    Event date: 2018.10

    Language:English  

    Venue:Paratunka, Kamchatka Region   Country:Russian Federation  

    We examined the Schumann resonance (SR) at low-latitude station KUJ by comparing with solar X-ray flux and solar proton flux at a geostationary orbit. For intense solar activity in October-November 2003, the reaction of the SR frequency to X-ray enhancement and SPEs was different. The SR frequency in H component increased at the time of the Xray enhancement. The response of SR seems to be caused by the increase of the electron density in the ionospheric D region which ionized by the enhanced solar X-ray flux. In the case of the SPEs, the SR frequency in D component decreased with enhancement of solar proton flux. We suggest that the SPEs caused the decrease of altitude on the ionopheric D region at high-latitude region, and the SR frequency decreased.

  • Estimation of time derivative of horizontal geomagnetic component for GIC assesment in Malaysia during quiet period

    Nornabilah Mohd Anuar, Farah Adilah Mohd Kasran, Zatul Iffah Abdul Latif, Siti Amalina Ence Ab Rahim, Arif Manut, Mohamad Huzaimy Jusoh, Normi Abdul Hadi, Akimasa Yoshikawa

    8th International Conference on System Engineering and Technology, ICSET 2018  2019.1 

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    Event date: 2018.10

    Language:English  

    Venue:Bandung   Country:Indonesia  

    This paper presents the preliminary observation on the possible Geomagnetic Induced Current (GIC) activities at Malaysia region during the quiet period of solar cycle 24 (year 2017). In fact, the damage of power system operation might lead to the malfunction of the transformer, which is the main component of the power system. Previously, the cause of the damage has been identified in the long-term investigation, where it drives from the space weather effect so-called (GIC). In this work, the quiet period has been selected by respecting the value of K-Planetary index (Kp) must be less than 3 extracted from OMNIWeb data source. The main objective of the current work is to investigate the behavior of the GIC amplitude at Malaysia region as well as to identify the parameter (ionospheric current and magnetospheric current) that contribute significantly towards the GIC activity at Malaysia region. The type of analysis was carried out using the data of geomagnetic field by extracting the time derivative of the horizontal component (dH/dt) as the indicator for GIC activity. The geomagnetic data was obtained from the MAGDAS observatories at Langkawi (LKW), Perak (PER), and Johor (JOH) stations. Subsequently, the dH/dt value is less than 30 nT/min represent no GIC activity occurred during that particular date for all three stations. However, the results revealed that the ionospheric current, DP2 corresponds well to the dH/dt amplitude. Plus, the latitudinal correlation gave the best representation of the control factor of GIC activity.

  • Estimation of time derivative of horizontal geomagnetic component for GIC assesment in Malaysia during quiet period

    Nornabilah Mohd Anuar, Farah Adilah Mohd Kasran, Zatul Iffah Abdul Latif, Siti Amalina Ence Ab Rahim, Arif Manut, Mohamad Huzaimy Jusoh, Normi Abdul Hadi, Akimasa Yoshikawa

    8th International Conference on System Engineering and Technology, ICSET 2018  2019.1 

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    Event date: 2018.10

    Language:English  

    Venue:Bandung   Country:Indonesia  

    This paper presents the preliminary observation on the possible Geomagnetic Induced Current (GIC) activities at Malaysia region during the quiet period of solar cycle 24 (year 2017). In fact, the damage of power system operation might lead to the malfunction of the transformer, which is the main component of the power system. Previously, the cause of the damage has been identified in the long-term investigation, where it drives from the space weather effect so-called (GIC). In this work, the quiet period has been selected by respecting the value of K-Planetary index (Kp) must be less than 3 extracted from OMNIWeb data source. The main objective of the current work is to investigate the behavior of the GIC amplitude at Malaysia region as well as to identify the parameter (ionospheric current and magnetospheric current) that contribute significantly towards the GIC activity at Malaysia region. The type of analysis was carried out using the data of geomagnetic field by extracting the time derivative of the horizontal component (dH/dt) as the indicator for GIC activity. The geomagnetic data was obtained from the MAGDAS observatories at Langkawi (LKW), Perak (PER), and Johor (JOH) stations. Subsequently, the dH/dt value is less than 30 nT/min represent no GIC activity occurred during that particular date for all three stations. However, the results revealed that the ionospheric current, DP2 corresponds well to the dH/dt amplitude. Plus, the latitudinal correlation gave the best representation of the control factor of GIC activity.

  • Estimation of time derivative of horizontal geomagnetic component for GIC assesment in Malaysia during quiet period

    Nornabilah Mohd Anuar, Farah Adilah Mohd Kasran, Zatul Iffah Abdul Latif, Siti Amalina Ence Ab Rahim, Arif Manut, Mohamad Huzaimy Jusoh, Normi Abdul Hadi, Akimasa Yoshikawa

    8th International Conference on System Engineering and Technology, ICSET 2018  2019.1 

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    Event date: 2018.10

    Language:English  

    Venue:Bandung   Country:Indonesia  

    This paper presents the preliminary observation on the possible Geomagnetic Induced Current (GIC) activities at Malaysia region during the quiet period of solar cycle 24 (year 2017). In fact, the damage of power system operation might lead to the malfunction of the transformer, which is the main component of the power system. Previously, the cause of the damage has been identified in the long-term investigation, where it drives from the space weather effect so-called (GIC). In this work, the quiet period has been selected by respecting the value of K-Planetary index (Kp) must be less than 3 extracted from OMNIWeb data source. The main objective of the current work is to investigate the behavior of the GIC amplitude at Malaysia region as well as to identify the parameter (ionospheric current and magnetospheric current) that contribute significantly towards the GIC activity at Malaysia region. The type of analysis was carried out using the data of geomagnetic field by extracting the time derivative of the horizontal component (dH/dt) as the indicator for GIC activity. The geomagnetic data was obtained from the MAGDAS observatories at Langkawi (LKW), Perak (PER), and Johor (JOH) stations. Subsequently, the dH/dt value is less than 30 nT/min represent no GIC activity occurred during that particular date for all three stations. However, the results revealed that the ionospheric current, DP2 corresponds well to the dH/dt amplitude. Plus, the latitudinal correlation gave the best representation of the control factor of GIC activity.

  • The First Solar-Powered MAGDAS-9 Installation and Possible Geomagnetically Induced Currents Study at Johor International conference

    Zatul Iffah Abdul Latiff, Mohamad Huzaimy Jusoh, Aznilinda Zainuddin, Nurhani Kasuan, Munirah Onn Muhammad, Asraf Hairuddin, Suhana Mohamed, Akimasa Yoshikawa

    International Conference on Space Weather and Satellite Application (ICeSSAT2018)  2018.8 

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    Event date: 2018.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Shah, Alam, Selangor   Country:Malaysia  

  • Assessment of the Geomagnetically Induced Current (GIC) at Low Latitude Region based on MAGDAS Data

    N. Mohd Anuar, F. A. Mohd Kasran, M. Abbas, M. H. Jusoh, S. A. Enche Ab Rahim, N. Abdul Hadi, Akimasa Yoshikawa, Z. Mohd Radzi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The geomagnetically induced current (GICs) impact is no longer concentrated at high latitude region strictly. The objective of this study was to extend the GICs observation conducted at equatorial region using geomagnetic data extracted from magnetometer installed at Langkawi National Observatory (LNO), Malaysia for the long-term analysis involving the solar cycle 24. The observation is now continued with the GICs comparison between LKW stations with five low latitude station which is BCL, PTN, MND, DAW, and TWV obtained from the magnetic data acquisition system (MAGDAS). The assessment of the GICs behavior revealed the possibility of LKW station experiences GICs is high, based on the time derivative of the horizontal component (dH/dt) value. Extend from that, the GICs estimation was successful done by applying the plane wave method as a model to calculate the North-South and the East-West component, Ex and Ey respectively. The equation of the GICs was provided by excluding the topology constant parameters, which is a and b constant and the value of the underground conductivity for low latitude station. Subsequently, the comparison was limited in years of 2008 - 2014 due to insufficient geomagnetic data. Indeed, the GICs calculation is able to derive the GICs estimation and showed a good agreement with the corresponding value of the time derivative of the horizontal component. However, the accurate current value (A) is able to gain by conducting a direct measurement of the high voltage power transmission system.

  • The first solar-powered Magdas-9 installation and possible geomagnetically induced currents study at Johor, Malaysia

    Zatul Iffah Abd Latiff, Mohamad Huzaimy Jusoh, Farah Adilah Mohd Kasran, Siti Amalina Enche Ab Rahim, Munirah Onn, Aznilinda Zainuddin, Muhammad Asraf Hairuddin, Nurhani Kasuan, Muhammad Muzamil Mustam, Suhana Mohamed, Yoshikawa Akimasa

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The Magnetic Data Acquisition System (MAGDAS-9) was successfully installed at Universiti Teknologi MARA Johor, Pasir Gudang Campus, Malaysia (JOH station), under the joint collaboration between International Center for Space Weather Science and Education (ICSWSE), National Space Agency (ANGKASA) and UiTM Johor. This is the first solar-powered magnetometer under the Magnetic Data Acquisition System of Circum-pan Pacific Magnetometer Network (MAGDAS/CPMN). In this paper, construction process, installation process and analysis of first geomagnetic observations at MAGDAS JOH station are presented. In addition, analysis on time derivative of horizontal component of geomagnetic field (dH/dt) to indicate the possibility of Geomagnetically Induced Currents (GIC) occurrences is also presented in this paper. The obtained geomagnetic components: H, D, Z and Total F are approximately similar to World Magnetic Model 2015 (WMM2015) while the diurnal variation from this geomagnetic observation showing a good variation pattern. The analysis of dH/dt has indicated 2 significant events of GIC.

  • The first solar-powered Magdas-9 installation and possible geomagnetically induced currents study at Johor, Malaysia

    Zatul Iffah Abd Latiff, Mohamad Huzaimy Jusoh, Farah Adilah Mohd Kasran, Siti Amalina Enche Ab Rahim, Munirah Onn, Aznilinda Zainuddin, Muhammad Asraf Hairuddin, Nurhani Kasuan, Muhammad Muzamil Mustam, Suhana Mohamed, Yoshikawa Akimasa

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The Magnetic Data Acquisition System (MAGDAS-9) was successfully installed at Universiti Teknologi MARA Johor, Pasir Gudang Campus, Malaysia (JOH station), under the joint collaboration between International Center for Space Weather Science and Education (ICSWSE), National Space Agency (ANGKASA) and UiTM Johor. This is the first solar-powered magnetometer under the Magnetic Data Acquisition System of Circum-pan Pacific Magnetometer Network (MAGDAS/CPMN). In this paper, construction process, installation process and analysis of first geomagnetic observations at MAGDAS JOH station are presented. In addition, analysis on time derivative of horizontal component of geomagnetic field (dH/dt) to indicate the possibility of Geomagnetically Induced Currents (GIC) occurrences is also presented in this paper. The obtained geomagnetic components: H, D, Z and Total F are approximately similar to World Magnetic Model 2015 (WMM2015) while the diurnal variation from this geomagnetic observation showing a good variation pattern. The analysis of dH/dt has indicated 2 significant events of GIC.

  • Relationship between plasma bubble and ionospheric current, equatorial electrojet, and equatorial counter electrojet

    T. Akiyama, A. Yoshikawa, A. Fujimoto, T. Uozumi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    In recent years, it has been clarified from previous studies that plasma bubbles and equatorial electrojets (EEJs) are related. In general, EEJs are calculated by subtracting the magnetic field H component of the magnetic equator from that at low latitude. However, in this study, EE-index data at Langkawi (magnetic equator), which includes all local current systems, were used for the analysis during the period from January 1, 2011, to November 8, 2014. By using the EE-index, it was found that plasma bubbles tend to occur for larger EEJ strengths. This result differs from the previous studies. In addition, if an equatorial counter electrojet (CEJ) occurs, it is understood that plasma bubbles will rarely occur due to the westward current; however, we found that when the lunar tidal effect is strong, plasma bubbles can occur even in conjunction with CEJs. Finally, we want to find the relationship between plasma bubbles and ionospheric current to predict them.

  • Relationship between plasma bubble and ionospheric current, equatorial electrojet, and equatorial counter electrojet

    T. Akiyama, A. Yoshikawa, A. Fujimoto, T. Uozumi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    In recent years, it has been clarified from previous studies that plasma bubbles and equatorial electrojets (EEJs) are related. In general, EEJs are calculated by subtracting the magnetic field H component of the magnetic equator from that at low latitude. However, in this study, EE-index data at Langkawi (magnetic equator), which includes all local current systems, were used for the analysis during the period from January 1, 2011, to November 8, 2014. By using the EE-index, it was found that plasma bubbles tend to occur for larger EEJ strengths. This result differs from the previous studies. In addition, if an equatorial counter electrojet (CEJ) occurs, it is understood that plasma bubbles will rarely occur due to the westward current; however, we found that when the lunar tidal effect is strong, plasma bubbles can occur even in conjunction with CEJs. Finally, we want to find the relationship between plasma bubbles and ionospheric current to predict them.

  • Electromagnetic induction responses to geomagnetic disturbances at low-and-mid-latitudes

    Mio Nakahara, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The geomagnetically induced current (GIC) is one of the most widely recognized phenomena caused by geomagnetic disturbances. Realistic predictions of magnetic field fluctuations may be used to evaluate the induction of electric fields to ground surfaces, and thus to estimate the occurrence of GICs. Although many GICs occur at high latitudes, they are now being studied at low and mid-latitudes as well. The purpose of this research was to understand the dynamics, observation, and prediction in Japan for GICs occurring at the low and mid-latitudes. In this study, the influence of geomagnetic field variations on Earth's electric field was examined. The magnetic field and the electric field components of 3 observation points for 1 year in 2015 are visually examined, and the characteristics of the fluctuations of the magnetic field and the surface electrical field were also analysed.

  • Electromagnetic induction responses to geomagnetic disturbances at low-and-mid-latitudes

    Mio Nakahara, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The geomagnetically induced current (GIC) is one of the most widely recognized phenomena caused by geomagnetic disturbances. Realistic predictions of magnetic field fluctuations may be used to evaluate the induction of electric fields to ground surfaces, and thus to estimate the occurrence of GICs. Although many GICs occur at high latitudes, they are now being studied at low and mid-latitudes as well. The purpose of this research was to understand the dynamics, observation, and prediction in Japan for GICs occurring at the low and mid-latitudes. In this study, the influence of geomagnetic field variations on Earth's electric field was examined. The magnetic field and the electric field components of 3 observation points for 1 year in 2015 are visually examined, and the characteristics of the fluctuations of the magnetic field and the surface electrical field were also analysed.

  • Characteristic of the Disturbed Days Ionospheric Current System in the 180-Degree Magnetic Meridian

    Siti Nurbaiti Ibrahim, Mohammad Huzaimy Jusoh, Ahmad Asari Sulaiman, Akimasa Yoshikawa, Zahira Mohd Radzi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The behavior of the ionospheric current during disturbed days using 10 geomagnetic observatories along 180-degree magnetic meridian was analysed. Separation of external and internal current during geomagnetic storm on 12 April until 15 April 2012 data was carried out using spherical harmonic analysis method. The contour of day to day variation of total current, external current and internal current were distinguished based on geomagnetic storm phase. These current then were correlate with the solar wind parameter, IMF Bz, and geomagnetic indices in order to identify their relationship. The results reveal that these current intensities were found higher during the initial phase. This due to the enhancement of the magnetic field during the initial phase caused by the increment of solar wind dynamic pressure and southward IMF Bz. Hence, the induced current identified in the internal current. This study demonstrated that the electric current induction can be obtained from the weak geomagnetic storm.

  • Characteristic of the Disturbed Days Ionospheric Current System in the 180-Degree Magnetic Meridian

    Siti Nurbaiti Ibrahim, Mohammad Huzaimy Jusoh, Ahmad Asari Sulaiman, Akimasa Yoshikawa, Zahira Mohd Radzi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The behavior of the ionospheric current during disturbed days using 10 geomagnetic observatories along 180-degree magnetic meridian was analysed. Separation of external and internal current during geomagnetic storm on 12 April until 15 April 2012 data was carried out using spherical harmonic analysis method. The contour of day to day variation of total current, external current and internal current were distinguished based on geomagnetic storm phase. These current then were correlate with the solar wind parameter, IMF Bz, and geomagnetic indices in order to identify their relationship. The results reveal that these current intensities were found higher during the initial phase. This due to the enhancement of the magnetic field during the initial phase caused by the increment of solar wind dynamic pressure and southward IMF Bz. Hence, the induced current identified in the internal current. This study demonstrated that the electric current induction can be obtained from the weak geomagnetic storm.

  • Assessment of the Geomagnetically Induced Current (GIC) at Low Latitude Region based on MAGDAS Data

    N. Mohd Anuar, F. A. Mohd Kasran, M. Abbas, M. H. Jusoh, S. A. Enche Ab Rahim, N. Abdul Hadi, A. Yoshikawa, Z. Mohd Radzi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The geomagnetically induced current (GICs) impact is no longer concentrated at high latitude region strictly. The objective of this study was to extend the GICs observation conducted at equatorial region using geomagnetic data extracted from magnetometer installed at Langkawi National Observatory (LNO), Malaysia for the long-term analysis involving the solar cycle 24. The observation is now continued with the GICs comparison between LKW stations with five low latitude station which is BCL, PTN, MND, DAW, and TWV obtained from the magnetic data acquisition system (MAGDAS). The assessment of the GICs behavior revealed the possibility of LKW station experiences GICs is high, based on the time derivative of the horizontal component (dH/dt) value. Extend from that, the GICs estimation was successful done by applying the plane wave method as a model to calculate the North-South and the East-West component, Ex and Ey respectively. The equation of the GICs was provided by excluding the topology constant parameters, which is a and b constant and the value of the underground conductivity for low latitude station. Subsequently, the comparison was limited in years of 2008 - 2014 due to insufficient geomagnetic data. Indeed, the GICs calculation is able to derive the GICs estimation and showed a good agreement with the corresponding value of the time derivative of the horizontal component. However, the accurate current value (A) is able to gain by conducting a direct measurement of the high voltage power transmission system.

  • Assessment of the Geomagnetically Induced Current (GIC) at Low Latitude Region based on MAGDAS Data

    N. Mohd Anuar, F. A. Mohd Kasran, M. Abbas, M. H. Jusoh, S. A. Enche Ab Rahim, N. Abdul Hadi, A. Yoshikawa, Z. Mohd Radzi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The geomagnetically induced current (GICs) impact is no longer concentrated at high latitude region strictly. The objective of this study was to extend the GICs observation conducted at equatorial region using geomagnetic data extracted from magnetometer installed at Langkawi National Observatory (LNO), Malaysia for the long-term analysis involving the solar cycle 24. The observation is now continued with the GICs comparison between LKW stations with five low latitude station which is BCL, PTN, MND, DAW, and TWV obtained from the magnetic data acquisition system (MAGDAS). The assessment of the GICs behavior revealed the possibility of LKW station experiences GICs is high, based on the time derivative of the horizontal component (dH/dt) value. Extend from that, the GICs estimation was successful done by applying the plane wave method as a model to calculate the North-South and the East-West component, Ex and Ey respectively. The equation of the GICs was provided by excluding the topology constant parameters, which is a and b constant and the value of the underground conductivity for low latitude station. Subsequently, the comparison was limited in years of 2008 - 2014 due to insufficient geomagnetic data. Indeed, the GICs calculation is able to derive the GICs estimation and showed a good agreement with the corresponding value of the time derivative of the horizontal component. However, the accurate current value (A) is able to gain by conducting a direct measurement of the high voltage power transmission system.

  • The first solar-powered Magdas-9 installation and possible geomagnetically induced currents study at Johor, Malaysia

    Zatul Iffah Abd Latiff, Mohamad Huzaimy Jusoh, Farah Adilah Mohd Kasran, Siti Amalina Enche Ab Rahim, Munirah Onn, Aznilinda Zainuddin, Muhammad Asraf Hairuddin, Nurhani Kasuan, Muhammad Muzamil Mustam, Suhana Mohamed, Akimasa Yoshikawa

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The Magnetic Data Acquisition System (MAGDAS-9) was successfully installed at Universiti Teknologi MARA Johor, Pasir Gudang Campus, Malaysia (JOH station), under the joint collaboration between International Center for Space Weather Science and Education (ICSWSE), National Space Agency (ANGKASA) and UiTM Johor. This is the first solar-powered magnetometer under the Magnetic Data Acquisition System of Circum-pan Pacific Magnetometer Network (MAGDAS/CPMN). In this paper, construction process, installation process and analysis of first geomagnetic observations at MAGDAS JOH station are presented. In addition, analysis on time derivative of horizontal component of geomagnetic field (dH/dt) to indicate the possibility of Geomagnetically Induced Currents (GIC) occurrences is also presented in this paper. The obtained geomagnetic components: H, D, Z and Total F are approximately similar to World Magnetic Model 2015 (WMM2015) while the diurnal variation from this geomagnetic observation showing a good variation pattern. The analysis of dH/dt has indicated 2 significant events of GIC.

  • Relationship between plasma bubble and ionospheric current, equatorial electrojet, and equatorial counter electrojet

    T. Akiyama, Akimasa Yoshikawa, A. Fujimoto, T. Uozumi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    In recent years, it has been clarified from previous studies that plasma bubbles and equatorial electrojets (EEJs) are related. In general, EEJs are calculated by subtracting the magnetic field H component of the magnetic equator from that at low latitude. However, in this study, EE-index data at Langkawi (magnetic equator), which includes all local current systems, were used for the analysis during the period from January 1, 2011, to November 8, 2014. By using the EE-index, it was found that plasma bubbles tend to occur for larger EEJ strengths. This result differs from the previous studies. In addition, if an equatorial counter electrojet (CEJ) occurs, it is understood that plasma bubbles will rarely occur due to the westward current; however, we found that when the lunar tidal effect is strong, plasma bubbles can occur even in conjunction with CEJs. Finally, we want to find the relationship between plasma bubbles and ionospheric current to predict them.

  • Electromagnetic induction responses to geomagnetic disturbances at low-and-mid-latitudes

    Mio Nakahara, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The geomagnetically induced current (GIC) is one of the most widely recognized phenomena caused by geomagnetic disturbances. Realistic predictions of magnetic field fluctuations may be used to evaluate the induction of electric fields to ground surfaces, and thus to estimate the occurrence of GICs. Although many GICs occur at high latitudes, they are now being studied at low and mid-latitudes as well. The purpose of this research was to understand the dynamics, observation, and prediction in Japan for GICs occurring at the low and mid-latitudes. In this study, the influence of geomagnetic field variations on Earth's electric field was examined. The magnetic field and the electric field components of 3 observation points for 1 year in 2015 are visually examined, and the characteristics of the fluctuations of the magnetic field and the surface electrical field were also analysed.

  • Characteristic of the Disturbed Days Ionospheric Current System in the 180-Degree Magnetic Meridian

    Siti Nurbaiti Ibrahim, Mohammad Huzaimy Jusoh, Ahmad Asari Sulaiman, Akimasa Yoshikawa, Zahira Mohd Radzi

    1st International Conference on Space Weather and Satellite Application 2018, ICeSSAT 2018  2019.3 

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    Event date: 2018.8

    Language:English  

    Venue:Shah Alam, Selangor   Country:Malaysia  

    The behavior of the ionospheric current during disturbed days using 10 geomagnetic observatories along 180-degree magnetic meridian was analysed. Separation of external and internal current during geomagnetic storm on 12 April until 15 April 2012 data was carried out using spherical harmonic analysis method. The contour of day to day variation of total current, external current and internal current were distinguished based on geomagnetic storm phase. These current then were correlate with the solar wind parameter, IMF Bz, and geomagnetic indices in order to identify their relationship. The results reveal that these current intensities were found higher during the initial phase. This due to the enhancement of the magnetic field during the initial phase caused by the increment of solar wind dynamic pressure and southward IMF Bz. Hence, the induced current identified in the internal current. This study demonstrated that the electric current induction can be obtained from the weak geomagnetic storm.

  • Equatorial Electrojet and Ionospheric Profile Parameters at Peruvian Station During Solar Minimum International conference

    Saeed Abioye BELLO, Mardina ABDULLAH, Nurul Shazana ABDUL HAMID, Bodo REINISCH, Akimasa YOSHIKAWA

    AOGS2018 15th Annual Meeting  2018.6 

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    Event date: 2018.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Waikiki, Hawai   Country:United States  

  • Longitudinal profile of equatorial electrojet derived from ground and satellite based magnetometers International conference

    Wan Nur Izzaty Ismail, Nurul Shazana Abdul Hamid, Mardina Abdullah, Akimasa Yoshikawa

    2018 UKM FST Postgraduate Colloquium  2019.6 

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    Event date: 2018.4

    Language:English  

    Venue:Selangor   Country:Malaysia  

    The intense current that flowing eastward in the dayside in the E layer of ionosphere at dip equator region is known as equatorial electrojet (EEJ). In this work, we attempt to compare the longitudinal profile of EEJ current estimated from the Challenging Minisatellite Payload (CHAMP) and European Space Agency satellite (SWARM) with the ground-based magnetometer network from six equatorial observatory pairs across the globe. Ground magnetometer were obtained from the network such as MAGDAS, INTERMAGNET and IIG. We process our data using the EUEL index during quiet days for ground measurement. Then, correlation coefficient were obtained after applying appropriate normalization techniques for both measurements. Analysis showed the longitudinal variations of EEJ current from ground indicates that this current was strongest at South American (77 °W) and Southeast Asian (99.78°E). Meanwhile, satellite measurement shows four peaks of EEJ current at -100°W, 0°E, 100°E and 180° E which are at North America, Atlantic ocean, Southeast Asian and Pacific ocean respectively.

  • Statistical study of equatorial geomagnetic crochets

    Norhani Muhammad Nasir Annadurai, Nurul Shazana Abdul Hamid, Akimasa Yoshikawa

    2018 UKM FST Postgraduate Colloquium  2019.6 

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    Event date: 2018.4

    Language:English  

    Venue:Selangor   Country:Malaysia  

    This study present the statistical investigation of equatorial geomagnetic crochets due to strong solar flare of class M to X. Our analysis utilized data from eight magnetometer stations provided by MAGnetic Data Acquisition System network (MAGDAS) at different longitudes sector during period from January 2008 to March 2015. We have considered 52 cases of solar flare events. Based on our analysis, 65% of the studied solar flares show no effect on geomagnetic variation with most of it from class M8, M9 and X1. The absence of solar flare effect might due to the influence of coronal mass ejection (CME) on the observation data or due to the station's location is at nighttime. The other 35% shows geomagnetic crochets to the magnetic data variation where majority are mix effect dominated by positive crochets. Apart from that, we also found an interesting solar flare effect where negative geomagnetic crochets were detected from all equatorial magnetometer data. The unique effect is due to X-class solar flare on 9th August 2011. Further investigation using extended latitudinal and longitudinal magnetometer is recommended to observe the whole picture of the solar flare effect to global ionospheric current.

  • Longitudinal profile of equatorial electrojet derived from ground and satellite based magnetometers

    Wan Nur Izzaty Ismail, Nurul Shazana Abdul Hamid, Mardina Abdullah, Akimasa Yoshikawa

    2018 UKM FST Postgraduate Colloquium  2019.6 

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    Event date: 2018.4

    Language:English  

    Venue:Selangor   Country:Malaysia  

    The intense current that flowing eastward in the dayside in the E layer of ionosphere at dip equator region is known as equatorial electrojet (EEJ). In this work, we attempt to compare the longitudinal profile of EEJ current estimated from the Challenging Minisatellite Payload (CHAMP) and European Space Agency satellite (SWARM) with the ground-based magnetometer network from six equatorial observatory pairs across the globe. Ground magnetometer were obtained from the network such as MAGDAS, INTERMAGNET and IIG. We process our data using the EUEL index during quiet days for ground measurement. Then, correlation coefficient were obtained after applying appropriate normalization techniques for both measurements. Analysis showed the longitudinal variations of EEJ current from ground indicates that this current was strongest at South American (77 °W) and Southeast Asian (99.78°E). Meanwhile, satellite measurement shows four peaks of EEJ current at -100°W, 0°E, 100°E and 180° E which are at North America, Atlantic ocean, Southeast Asian and Pacific ocean respectively.

  • Statistical study of equatorial geomagnetic crochets International conference

    Norhani Muhammad Nasir Annadurai, Nurul Shazana Abdul Hamid, Akimasa Yoshikawa

    2018 UKM FST Postgraduate Colloquium  2019.6 

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    Event date: 2018.4

    Language:English  

    Venue:Selangor   Country:Malaysia  

    This study present the statistical investigation of equatorial geomagnetic crochets due to strong solar flare of class M to X. Our analysis utilized data from eight magnetometer stations provided by MAGnetic Data Acquisition System network (MAGDAS) at different longitudes sector during period from January 2008 to March 2015. We have considered 52 cases of solar flare events. Based on our analysis, 65&#37; of the studied solar flares show no effect on geomagnetic variation with most of it from class M8, M9 and X1. The absence of solar flare effect might due to the influence of coronal mass ejection (CME) on the observation data or due to the station's location is at nighttime. The other 35&#37; shows geomagnetic crochets to the magnetic data variation where majority are mix effect dominated by positive crochets. Apart from that, we also found an interesting solar flare effect where negative geomagnetic crochets were detected from all equatorial magnetometer data. The unique effect is due to X-class solar flare on 9th August 2011. Further investigation using extended latitudinal and longitudinal magnetometer is recommended to observe the whole picture of the solar flare effect to global ionospheric current.

  • S-310-44 号機による Sq 電流系付近の DC/AC 電場観測

    石坂 圭吾, 阿部 琢美, 熊本 篤志, 田中 真, 吉川 顕正, 松下 拓輝

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Multipoint observation of Pc5 pulsations by QZS-1, THEMIS, and MAGDAS/KTN on the same L shell

    Shun Imajo, Masahito Nose, Nana Higashio, Hideki Koshiishi, Reiko Nomura, Kiyokazu Koga, Akimasa Yoshikawa

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • 電離圏ポテンシャルソルバーによる木星内部磁気圏電場の太陽風応答の研究

    寺田 綱一朗, 垰 千尋, 寺田 直樹, 笠羽 康正, 北 元, 中溝 葵, 吉川 顕正, Ohtani Shinichi, 土屋 史 紀, 鍵谷 将人, 坂野井 健, 村上 豪, 吉岡 和夫, 木村 智樹, 山崎 敦, 吉川 一朗

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Adjustment of the offset level for the simplified magnetometer using MI sensor

    Kentarou Kitamura, Rei Tanaka, Masahito Nose, Teiji Uozumi, Akimasa Yoshikawa

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • QZSとMAGDASによる磁気圏FAC-電離圏電流回路の長期間同時観測:統計解析

    安倍松 侑太, 河野 英昭, 東尾 奈々, 松本 晴久, Moiseev Alexey, Baishev Dmitry, 魚住 禎司, 阿部 修 司, 吉川 顕正, MAGDAS/CPMN グループ 吉川 顕正

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • 地上隣接 2 観測点での磁場の差分データを用いた、MSTID に伴う地上磁場変動の統計解析

    大筆 想, 河野 英昭, 津川 卓也, 西岡 未知, 塩川 和夫, 大塚 雄一, 魚住 禎司, 阿部 修司, 吉川 顕 正, MAGDAS/CPMN グループ 吉川 顕正

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Impact evaluation of space weather activities on space debris model

    Shuji Abe, Toshiya Hanada, Akimasa Yoshikawa, Takayuki Hirai, Satomi Kawamoto

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Dependence of Schumann resonance parameters on solar activity

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe, Hiromasa Nozawa, Manabu Shinohara

    第142回地球電磁気・地球惑星圏学会  2017.10 

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    Event date: 2017.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:京都大学宇治キャンパス   Country:Japan  

  • Characteristics of Schumann Resonance Parameters at Kuju Station

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe, Hiromasa Nozawa, Manabu Shinohara

    8th International Conference on Solar-Terrestrial Relations and Physics of Earthquake Precursors, STREEP 2017  2017.10 

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    Event date: 2017.9

    Language:English  

    Venue:Paratunka, Kamchatka   Country:Russian Federation  

    The ground magnetic field variation in the extremely low frequency (ELF) range has been measured by an induction magnetometer at Kuju, Japan (KUJ; M.Lat. = 23.4 degrees, M. Lon. = 201.0 degrees) since 2003. The first mode of the Schumann resonance (SR) around 8 Hz can be seen at KUJ. The SR in H (horizontal northward component) shows maximum peaks around 08 UT and 15 UT. In the case of D (horizontal eastward component), the SR shows its maximum peak around 08 UT. These peaks are coincident with the enhancement of lightning activity in Africa and Asia. Thus, we found the influence of the lightning activity on the observed SR at KUJ.

  • Monitoring of Space and Earth electromagnetic environment by MAGDAS project Collaboration with IKIR-Introduction to ICSWSE/MAGDAS project

    Akimasa Yoshikawa, Akiko Fujimoto, Akihiro Ikeda, Teiji Uozumi, Shuji Abe

    8th International Conference on Solar-Terrestrial Relations and Physics of Earthquake Precursors, STREEP 2017  2017.10 

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    Event date: 2017.9

    Language:English  

    Venue:Paratunka, Kamchatka   Country:Russian Federation  

    For study of coupling processes in the Solar-Terrestrial System, International Center for Space Weather Science and Education (ICSWSE), Kyushu University has developed a real time magnetic data acquisition system (the MAGDAS project) around the world. The number of observational sites is increasing every year with the collaboration of host countries. Now at this time, the MAGDAS Project has installed 78 real time magnetometers-so it is the largest magnetometer array in the world. The history of global observation at Kyushu University is over 30 years and number of developed observational sites is over 140. Especially, Collaboration between IKIR is extended back to 1990's. Now a time, we are operating Flux-gate magnetometer and FM-CW Radar. It is one of most important collaboration for space weather monitoring. By using MAGDAS data, ICSWSE produces many types of space weather index, such as EE-index (for monitoring long tern and shot term variation of equatorial electrojet), Pc5 index (for monitoring solar-wind velocity and high energy electron flux), Sq-index (for monitoring global change of ionospheric low and middle latitudinal current system), and Pc3 index (for monitoring of plasma density variation at low latitudes). In this report, we will introduce recent development of MAGDAS/ICSWSE Indexes project and topics for new open policy for MAGDAS data will be also discussed.

  • Characteristics of Schumann Resonance Parameters at Kuju Station

    Akihiro Ikeda, Teiji Uozumi, Akimasa Yoshikawa, Akiko Fujimoto, Shuji Abe, Hiromasa Nozawa, Manabu Shinohara

    8th International Conference on Solar-Terrestrial Relations and Physics of Earthquake Precursors, STREEP 2017  2017.10 

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    Event date: 2017.9

    Language:English  

    Venue:Paratunka, Kamchatka   Country:Russian Federation  

    The ground magnetic field variation in the extremely low frequency (ELF) range has been measured by an induction magnetometer at Kuju, Japan (KUJ; M.Lat. = 23.4 degrees, M. Lon. = 201.0 degrees) since 2003. The first mode of the Schumann resonance (SR) around 8 Hz can be seen at KUJ. The SR in H (horizontal northward component) shows maximum peaks around 08 UT and 15 UT. In the case of D (horizontal eastward component), the SR shows its maximum peak around 08 UT. These peaks are coincident with the enhancement of lightning activity in Africa and Asia. Thus, we found the influence of the lightning activity on the observed SR at KUJ.

  • Monitoring of Space and Earth electromagnetic environment by MAGDAS project Collaboration with IKIR-Introduction to ICSWSE/MAGDAS project

    Akimasa Yoshikawa, Akiko Fujimoto, Akihiro Ikeda, Teiji Uozumi, Shuji Abe

    8th International Conference on Solar-Terrestrial Relations and Physics of Earthquake Precursors, STREEP 2017  2017.10 

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    Event date: 2017.9

    Language:English  

    Venue:Paratunka, Kamchatka   Country:Russian Federation  

    For study of coupling processes in the Solar-Terrestrial System, International Center for Space Weather Science and Education (ICSWSE), Kyushu University has developed a real time magnetic data acquisition system (the MAGDAS project) around the world. The number of observational sites is increasing every year with the collaboration of host countries. Now at this time, the MAGDAS Project has installed 78 real time magnetometers-so it is the largest magnetometer array in the world. The history of global observation at Kyushu University is over 30 years and number of developed observational sites is over 140. Especially, Collaboration between IKIR is extended back to 1990's. Now a time, we are operating Flux-gate magnetometer and FM-CW Radar. It is one of most important collaboration for space weather monitoring. By using MAGDAS data, ICSWSE produces many types of space weather index, such as EE-index (for monitoring long tern and shot term variation of equatorial electrojet), Pc5 index (for monitoring solar-wind velocity and high energy electron flux), Sq-index (for monitoring global change of ionospheric low and middle latitudinal current system), and Pc3 index (for monitoring of plasma density variation at low latitudes). In this report, we will introduce recent development of MAGDAS/ICSWSE Indexes project and topics for new open policy for MAGDAS data will be also discussed.

  • Decomposition of the wave elements of the global high-correlation Pi 2 International conference

    Teiji Uozumi, Akimasa Yoshikawa, Shinichi Ohtani, D G Baishev, A V Moiseyev, B M Shevtsov

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • 電離圏ポテンシャルソルバーによる木星内部磁気圏電場の太陽風応答の研究 International conference

    寺田 綱一朗, 垰 千尋, 土屋 史紀, 笠羽 康正, 北 元, 中溝 葵, 吉川 顕正, 大谷 晋一, 土屋 史紀, 鍵谷 将人, 坂野井 健, 村上 豪, 吉岡 和夫, 木村 智樹, 山崎 敦, 吉川 一朗

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Local time and seasonal variations of the amplitude of the main impulse (MI) of geomagnetic sudden commencements in the low-latitude and equatorial regions International conference

    新堀 淳樹, 菊池 崇, 荒木 徹, 池田 昭大, 魚住 禎司, 歌田 久司, 長妻 努, 吉川 顕正

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • 久住におけるシューマン共鳴の長期変動 International conference

    池田 昭大, 魚住 禎司, 吉川 顕正, 藤本 晶子, 阿部 修司, 野澤 宏大

    日本地球惑星科学連合2017大会  2017.5 

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    Event date: 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Longitudinal Variation of EEJ Current during Different Phases of Solar Cycle

    W. N.I. Ismail, N. S.A. Hamid, M. Abdullah, Akimasa Yoshikawa, T. Uozumi

    2017 International Conference on Space Science and Communication: Space Science for Sustainability, IconSpace 2017  2017.6 

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    Event date: 2017.5

    Language:English  

    Venue:Kuala Lumpur   Country:Malaysia  

    The equatorial electrojet (EEJ) is an eastward current flow around the dip equator in E-region of the ionosphere within the range of 90 to 120 km altitude. The longitudinal variation of EEJ was studied using the ground-based measurement from six different longitudinal sectors. The ground magnetometer data were provided by magnetometer networks such as those from Magnetic Data Acquisition System (MAGDAS) /Circum-pan Pacific Magnetometer Network (CPMN), Indian Institute of Geomagnetism (IIG) and International Real-time Magnetic Observatory Network (INTERMAGNET). The EUEL index used in this study was calculated from geomagnetic northward H component. The H-component was normalized to the dip equator using the CM4 model. This study present results of the longitudinal variation of EEJ during the three phases of solar cycle 24: solar minimum (2008), inclination phase (2011) and solar maximum (2014). Results show that EEJ current is higher in the American sector and lowest between African and Indian sector in 2008 and 2011. On the other hand, during the year of solar maximum, this current component is comparable in American and Southeast Asian sector.

  • Peak time of equatorial electrojet from different longitude sectors during fall solar minimum

    N. S.A. Hamid, H. Liu, T. Uozumi, A. Yoshikawa, N. M.N. Annadurai

    2017 International Conference on Space Science and Communication: Space Science for Sustainability, IconSpace 2017  2017.6 

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    Event date: 2017.5

    Language:English  

    Venue:Kuala Lumpur   Country:Malaysia  

    Equatorial electrojet is an eastward flowing current at about ±3° dip equator. This current intensity is always higher during noontime as it is greatly influenced by the ionization of Earth ionosphere. Apart from that, previous study had shown that EEJ current varies with longitude and latitude as well as solar cycle. The aim of this study is to investigate the peak time of EEJ current at different longitude sectors using simultaneous data in 2009. By eliminating Sq current contribution and normalizing ground-based data from MAGDAS/CPMN, IIG and WDC network, we managed to reach our purpose and gain reliable output. We found out that EEJ is strongest in South American sector. Our results show that the peak EEJ during fall solar minimum is observed at 11 LT for South American, Indian and Southeast Asian sector but it is 1 hr earlier in African sector.

  • Longitudinal Variation of EEJ Current during Different Phases of Solar Cycle

    W. N.I. Ismail, N. S.A. Hamid, M. Abdullah, A. Yoshikawa, T. Uozumi

    2017 International Conference on Space Science and Communication: Space Science for Sustainability, IconSpace 2017  2017.6 

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    Event date: 2017.5

    Language:English  

    Venue:Kuala Lumpur   Country:Malaysia  

    The equatorial electrojet (EEJ) is an eastward current flow around the dip equator in E-region of the ionosphere within the range of 90 to 120 km altitude. The longitudinal variation of EEJ was studied using the ground-based measurement from six different longitudinal sectors. The ground magnetometer data were provided by magnetometer networks such as those from Magnetic Data Acquisition System (MAGDAS) /Circum-pan Pacific Magnetometer Network (CPMN), Indian Institute of Geomagnetism (IIG) and International Real-time Magnetic Observatory Network (INTERMAGNET). The EUEL index used in this study was calculated from geomagnetic northward H component. The H-component was normalized to the dip equator using the CM4 model. This study present results of the longitudinal variation of EEJ during the three phases of solar cycle 24: solar minimum (2008), inclination phase (2011) and solar maximum (2014). Results show that EEJ current is higher in the American sector and lowest between African and Indian sector in 2008 and 2011. On the other hand, during the year of solar maximum, this current component is comparable in American and Southeast Asian sector.

  • Peak time of equatorial electrojet from different longitude sectors during fall solar minimum

    N. S.A. Hamid, Huixin Liu, T. Uozumi, Akimasa Yoshikawa, N. M.N. Annadurai

    2017 International Conference on Space Science and Communication: Space Science for Sustainability, IconSpace 2017  2017.6 

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    Event date: 2017.5

    Language:English  

    Venue:Kuala Lumpur   Country:Malaysia  

    Equatorial electrojet is an eastward flowing current at about ±3° dip equator. This current intensity is always higher during noontime as it is greatly influenced by the ionization of Earth ionosphere. Apart from that, previous study had shown that EEJ current varies with longitude and latitude as well as solar cycle. The aim of this study is to investigate the peak time of EEJ current at different longitude sectors using simultaneous data in 2009. By eliminating Sq current contribution and normalizing ground-based data from MAGDAS/CPMN, IIG and WDC network, we managed to reach our purpose and gain reliable output. We found out that EEJ is strongest in South American sector. Our results show that the peak EEJ during fall solar minimum is observed at 11 LT for South American, Indian and Southeast Asian sector but it is 1 hr earlier in African sector.

  • MAGDAS measurement of EEJ height incorporating lithosperic image currents in dielectric ground

    Quirino Sugon Jr., Christine Chan, Clint Bennett, Felix Muga II, Daniel McNamara, Roland Otadoy, Akiko Fujimoto, Teiji Uozumi, and Akimasa Yoshikawa

    シンポジウム「太陽地球系科学に於ける地上観測の現状と課題」  2017.3 

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    Event date: 2017.3

    Language:English   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡県福岡市   Country:Japan  

  • ELF帯電波観測に基づいた雷放電によるダウンバースト現象の予測可能性

    清水千春, 佐藤光輝, 高橋幸弘, 土屋史紀, 本郷保二, 阿部修司, 吉川顕正

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • Variation of Schumann resonance parameters at Kuju

    Ikeda A., T. Uozumi, A. Yoshikawa, A. Fujimoto, S. Abe, H. Nozawa, and M. Shinohara

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • 宇宙天気活動に伴うスペースデブリ環境の長期予測

    阿部修司, 花田俊也, 吉川顕正, 平井隆之, 河本聡美

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • 低緯度―赤道域における磁気急始時の主インパルス振幅の季節変化

    新堀淳樹, 菊池崇, 荒木徹, 池田昭大, 魚住禎司, 歌田久司, 長妻努, 吉川顕正

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • 電離圏ポテンシャルソルバーによる木星内部磁気圏電場の太陽風応答の研究

    寺田綱一朗, 寺田直樹, 笠羽康正, 北元, 垰千尋, 中溝葵, 吉川顕正, Ohtani Shinichi, 土屋史 紀, 鍵谷将人, 坂野井健, 村上豪, 吉岡和夫, 木村智樹, 山崎敦, 吉川一朗

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • Correlated temporal variations of SCW, AKR and global Pi 2

    Uozumi, T., A. Yoshikawa, S. Ohtani, S. Imajo, D. G. Baishev, A. V. Moiseyev, and B. M. Shevtsov

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • FAC-電離層電流系のQZS-MAGDAS同時観測の初期統計解析

    Hideaki Kawano, Osamu Ogushi, Yuta Abematsu, Nana Higashio, Haruhisa Matsumoto, Alexey Moiseev, Dmitry Baishev, Teiji Uozumi, Shuji Abe, Akimasa Yoshikawa, Akimasa Yoshikawa MAGDAS/CPMN Group

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • 北海道-陸別第一・第二レーダーによる低緯度オーロラ発生時における電離圏対流の観測

    西谷望, 堀智昭, 片岡龍峰, 海老原祐輔, 塩川和夫, 大塚雄一, 鈴木秀彦, 吉川顕正

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • S-310-44号機観測ロケットによるSq電流系中心付近の電場観測

    安宅祐香, 石坂圭吾, 阿部琢美, 田中真, 熊本篤志, 吉川顕正, 松下拓輝

    第140回 SGEPSS総会および講演会  2016.11 

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    Event date: 2016.11 - 2017.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:福岡県福岡市   Country:Japan  

  • 長期の宇宙天気活動に伴うスペースデブリ環境の推移予測

    阿部修司, 花田俊也, 吉川顕正, 平井隆之, 河本聡美

    第7回スペースデブリワークショップ  2016.10 

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    Event date: 2016.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:宇宙航空研究開発機構調布航空宇宙センター(JAXA)(CAC)), 調布市,東京   Country:Japan  

  • 宇宙天気に伴うスペースデブリ環境推移の長期変動と予測

    阿部修司, 花田俊也, 吉川顕正, 平井隆之, 河本聡美

    第3回「太陽地球環境データ解析に基づく超高層大気の空間・時間変動の解明」  2016.10 

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    Event date: 2016.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所, 立川市, 東京   Country:Japan  

  • 宇宙天気活動に伴うスペースデブリ環境の変動と予測

    阿部修司, 花田俊也, 吉川顕正, 平井隆之, 河本聡美

    第60回宇宙科学技術連合講演会  2016.9 

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    Event date: 2016.9

    Language:English   Presentation type:Oral presentation (general)  

    Venue:函館アリーナ, 函館市, 北海道   Country:Japan  

  • Sq電流系中心の電子加熱現象解明のための観測ロケット実験速報-DC電場&超低周波波動観測- International conference

    安宅 祐香, 石坂 圭吾, 阿部 琢美, 田中 真, 熊本 篤志, 吉川 顕正, 松下 拓輝

    日本地球惑星科学連合2016大会  2016.5 

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    Event date: 2016.5 - 2017.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Relation between charge amounts of lightning discharges derived from ELF waveform data and severe weather International conference

    Chiharu Shimizu, Mitsuteru Sato, Yukihiro Takahashi, Fuminori Tsuchiya, Yasuji Hongo, Shuji Abe, Akimasa Yoshikawa

    日本地球惑星科学連合2016大会  2016.5 

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    Event date: 2016.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • 日本経度帯のプラズマ圏密度季節変化:北半球、南半球各々でのMAGDAS磁場観測からの推定・比較 International conference

    尾上彩希子, 河野英昭, 魚住禎司, Shevtsov Boris, Khomutov Sergey, Poddelskiy Igor, Marshall Richard, 吉川顕正, MAGDAS/CPMN group

    日本地球惑星科学連合2016大会  2016.5 

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    Event date: 2016.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Sq電流系中心の電子加熱現象解明のための観測ロケット実験速報-電子エネルギー分布観測- International conference

    阿部琢美, 石坂圭吾, 熊本篤志, 田中真, 高橋隆男, 松下拓輝, 吉川顕正

    日本地球惑星科学連合2016大会  2016.5 

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    Event date: 2016.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • 電離圏ポテンシャルソルバーによる木星内部磁気圏電場の太陽風応答の研究 discharges derived from ELF waveform data and severe weather International conference

    寺田綱一朗, 寺田直樹, 笠羽康正, 北, 垰千尋, 中溝葵, 吉川顕正, 大谷晋一, 土屋史紀, 鍵谷将人, 坂野井健, 村上豪, 吉岡和夫, 木村智樹, 山崎敦, 吉川一朗

    日本地球惑星科学連合2016大会  2016.5 

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    Event date: 2016.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ, 千葉県幕張市   Country:Japan  

  • Sq電流系中心付近の電子加熱現象解明のための観測ロケッ ト実験初期解析結果報告 Invited

    阿部琢美, 石坂圭吾, 熊本篤志, 高橋隆男, 田中真, 松下拓輝, 吉川顕正, MAGDAS/CPMNグループ

    電磁圏物理学シンポジウム  2016.3 

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    Event date: 2016.3

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:九州大学西新プラザ、福岡市   Country:Japan  

  • 電離圏下部Sq電流系中心付近の特異現象解明のための観測ロケット実験

    阿部 琢美, 石坂 圭吾, 熊本 篤志, 高橋 隆男, 田中 真, 吉川 顕正

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京大学 理学部   Country:Japan  

  • 昼間側Pi 2地磁気脈動の電離圏等価電流分布

    今城 峻, Akimasa Yoshikawa, 魚住 禎司, Ohtani Shinichi, 中溝 葵, 湯元 清文

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

  • IHM法とAPGM法のCARISMA・MAGDAS同時観測データへの適用:FLRパラメタの緯度依存性

    河野 英昭, Akimasa Yoshikawa, Pilipenko Viacheslav, Mann Ian R, Milling David, 才田 聡子, 北村 健太郎

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

    351. 河野 英昭, Pilipenko Viacheslav, Mann Ian R., Milling David, 才田 聡子, 北村 健太郎, 湯元 清文, 吉川 顕正, MAGDAS/CPMN グループ 吉川 顕正, (2014), IHM法とAPGM法のCARISMA・MAGDAS同時観測データへの適用:FLRパラメタの緯度依存性, 第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会),キッセイ文化ホール(長野県松本文化会館), 2014年10月31日~11月3日, 口頭発表, 2014年10月31日

  • 中規模伝搬性電離圏擾乱の地上磁場変動の同定

    下野 陽一, 河野 英昭, 津川 卓也, 西岡 未知, 塩川 和夫, 大塚 雄一, 魚住 禎司, 阿部 修司, Akimasa Yoshikawa

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.11 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

  • Daily variation of geomagnetic field Z component during geomagnetic storm

    Matsushita H, Akimasa Yoshikawa, T. Uozumi

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.11 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

  • Relationship among relativistic electron in the radiation belt, solar wind and Pc5 at dip equator

    K. Akimoto, Akimasa Yoshikawa, T. Uozumi, S. Abe

    第136回 地球電磁気・地球惑星圏学会総会・講演会(2014年 秋学会)  2014.11 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:キッセイ文化ホール(長野県松本文化会館)   Country:Japan  

  • MAGDAS/CPMN Group, Equatorial Pc 5 observed by the MAGDAS/CPMN network under high speed solar wind conditions

    Kaisei Akimoto, Akiko Fujimoto, Akimasa Yoshikawa, Teiji Uozumi, Shuji Abe

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京大学 理学部   Country:Japan  

  • Simultaneous observation of field-aligned current with QZS and MAGDAS observatories

    Osamu Ogushi, Hideaki Kawano, Nana Higashio, Haruhisa Matsumoto, Alexey Moiseev, Dmitry Baishev, Teiji Uozumi, Shuji Abe, Kiyohumi Yumoto, Akimasa Yoshikawa

    第138回 地球電磁気・地球惑星圏学会総会・講演会(2015年 秋学会)  2015.10 

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    Event date: 2015.10 - 2015.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:東京大学 理学部   Country:Japan  

  • Longitudinal and solar activity dependence of equatorial electrojet at Southeast Asian sector

    N. S.A. Hamid, Huixin Liu, T. Uozumi, G. K. Gopir, H. A. Hadin, Akimasa Yoshikawa

    4th International Conference on Space Science and Communication, IconSpace 2015  2015.9 

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    Event date: 2015.8

    Language:English  

    Venue:Langkawi   Country:Malaysia  

    In the E layer of equatorial ionosphere, the equatorial electrojet (EEJ) current interacts with the global Sq current and caused abnormally large amplitude of geomagnetic field component measured at the magnetic dip equator station. In this study, we attempted to separate EEJ and Sq at dip equator using the EUEL index derived from MAGDAS/CPMN stations. Moreover, we normalized the observation data to overcome the uncertainties due to the latitudinal variation of both EEJ and Sq currents which are neglected in most of previous studies. This new approach allowed the study of longitudinal dependence of EEJ. Analysis is performed using data from stations at East and West of Southeast Asian sector for a year of 2011. Additionally, we examined the solar activity dependence of EEJ during this inclining phase of solar cycle.

  • Variations of ULF and VLF during moderate geomagnetic storm at equatorial region

    S. N.A. Ahmad, M. H. Jusoh, F. A.M. Kasran, M. Abdullah, B. Veenadhari, T. Uozumi, S. Abe, A. Yoshikawa, M. G. Cardinal

    4th International Conference on Space Science and Communication, IconSpace 2015  2015.9 

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    Event date: 2015.8

    Language:English  

    Venue:Langkawi   Country:Malaysia  

    This paper presents variations of Ultra Low Frequency (ULF) and Very Low Frequency (VLF) during moderate geomagnetic storm using ground based observatories, Magnetic Data Acquisition System (MAGDAS)/Circum-Pan Magnetic Network (CPMN) magnetometer and Atmospheric Weather Electromagnetic System for Observation Modeling and Education (AWESOME) VLF receiver. In this analysis, the recorded ULF horizontal (H)-component are extracted from MAGDAS magnetometer at Yap Island (YAP), Federated States of Micronesia, Davao (DAV), Philippines, and Tirunelveli (TIR), India stations. VLF amplitude data were observed from VLF receiver at UKM while the transmitters are located at Katabomman (VTX), India, North West Cape (NWC), Australia and Lualualei, Hawaii (NPM), USA. The observations of the space weather conditions in this study are divided into two categories: quiet day (10 April 2010) and moderate geomagnetic storm (6 April 2010). The results show that the ULF and VLF variations are significantly affected during geomagnetic storm which geomagnetic activities are closely related with the solar parameters.

  • Longitudinal and solar activity dependence of equatorial electrojet at Southeast Asian sector

    N. S.A. Hamid, H. Liu, T. Uozumi, G. K. Gopir, H. A. Hadin, A. Yoshikawa

    4th International Conference on Space Science and Communication, IconSpace 2015  2015.9 

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    Event date: 2015.8

    Language:English  

    Venue:Langkawi   Country:Malaysia  

    In the E layer of equatorial ionosphere, the equatorial electrojet (EEJ) current interacts with the global Sq current and caused abnormally large amplitude of geomagnetic field component measured at the magnetic dip equator station. In this study, we attempted to separate EEJ and Sq at dip equator using the EUEL index derived from MAGDAS/CPMN stations. Moreover, we normalized the observation data to overcome the uncertainties due to the latitudinal variation of both EEJ and Sq currents which are neglected in most of previous studies. This new approach allowed the study of longitudinal dependence of EEJ. Analysis is performed using data from stations at East and West of Southeast Asian sector for a year of 2011. Additionally, we examined the solar activity dependence of EEJ during this inclining phase of solar cycle.

  • Variations of ULF and VLF during moderate geomagnetic storm at equatorial region

    S. N.A. Ahmad, M. H. Jusoh, F. A.M. Kasran, M. Abdullah, B. Veenadhari, T. Uozumi, S. Abe, Akimasa Yoshikawa, M. G. Cardinal

    4th International Conference on Space Science and Communication, IconSpace 2015  2015.9 

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    Event date: 2015.8

    Language:English  

    Venue:Langkawi   Country:Malaysia  

    This paper presents variations of Ultra Low Frequency (ULF) and Very Low Frequency (VLF) during moderate geomagnetic storm using ground based observatories, Magnetic Data Acquisition System (MAGDAS)/Circum-Pan Magnetic Network (CPMN) magnetometer and Atmospheric Weather Electromagnetic System for Observation Modeling and Education (AWESOME) VLF receiver. In this analysis, the recorded ULF horizontal (H)-component are extracted from MAGDAS magnetometer at Yap Island (YAP), Federated States of Micronesia, Davao (DAV), Philippines, and Tirunelveli (TIR), India stations. VLF amplitude data were observed from VLF receiver at UKM while the transmitters are located at Katabomman (VTX), India, North West Cape (NWC), Australia and Lualualei, Hawaii (NPM), USA. The observations of the space weather conditions in this study are divided into two categories: quiet day (10 April 2010) and moderate geomagnetic storm (6 April 2010). The results show that the ULF and VLF variations are significantly affected during geomagnetic storm which geomagnetic activities are closely related with the solar parameters.

  • Longitudinal and solar activity dependence of equatorial electrojet at Southeast Asian sector

    N. S.A. Hamid, Huixin Liu, T. Uozumi, G. K. Gopir, H. A. Hadin, Akimasa Yoshikawa

    4th International Conference on Space Science and Communication, IconSpace 2015  2015.9 

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    Event date: 2015.8

    Language:English  

    Venue:Langkawi   Country:Malaysia  

    In the E layer of equatorial ionosphere, the equatorial electrojet (EEJ) current interacts with the global Sq current and caused abnormally large amplitude of geomagnetic field component measured at the magnetic dip equator station. In this study, we attempted to separate EEJ and Sq at dip equator using the EUEL index derived from MAGDAS/CPMN stations. Moreover, we normalized the observation data to overcome the uncertainties due to the latitudinal variation of both EEJ and Sq currents which are neglected in most of previous studies. This new approach allowed the study of longitudinal dependence of EEJ. Analysis is performed using data from stations at East and West of Southeast Asian sector for a year of 2011. Additionally, we examined the solar activity dependence of EEJ during this inclining phase of solar cycle.

  • Variations of ULF and VLF during moderate geomagnetic storm at equatorial region

    S. N.A. Ahmad, M. H. Jusoh, F. A.M. Kasran, M. Abdullah, B. Veenadhari, T. Uozumi, S. Abe, Akimasa Yoshikawa, M. G. Cardinal

    4th International Conference on Space Science and Communication, IconSpace 2015  2015.9 

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    Event date: 2015.8

    Language:English  

    Venue:Langkawi   Country:Malaysia  

    This paper presents variations of Ultra Low Frequency (ULF) and Very Low Frequency (VLF) during moderate geomagnetic storm using ground based observatories, Magnetic Data Acquisition System (MAGDAS)/Circum-Pan Magnetic Network (CPMN) magnetometer and Atmospheric Weather Electromagnetic System for Observation Modeling and Education (AWESOME) VLF receiver. In this analysis, the recorded ULF horizontal (H)-component are extracted from MAGDAS magnetometer at Yap Island (YAP), Federated States of Micronesia, Davao (DAV), Philippines, and Tirunelveli (TIR), India stations. VLF amplitude data were observed from VLF receiver at UKM while the transmitters are located at Katabomman (VTX), India, North West Cape (NWC), Australia and Lualualei, Hawaii (NPM), USA. The observations of the space weather conditions in this study are divided into two categories: quiet day (10 April 2010) and moderate geomagnetic storm (6 April 2010). The results show that the ULF and VLF variations are significantly affected during geomagnetic storm which geomagnetic activities are closely related with the solar parameters.

  • 日本経度帯のプラズマ圏密度季節変化:地上磁場にFLR同定2点法を適用した長期間連続測定

    河野 英昭, 山田 哲郎, 北川 雄一郎, Shevtsov Boris, Khomutov Sergey, Poddelskiy Igor, 吉川 顕正, MAGDAS/CPMN group

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • Generation of geomagnetic Pc5 pulsations by compressional waves penetrating from the solar wind: a case study

    BAISHEV, Dmitry, MULLAYAROV, Victor SAMSONOV, Sergey MISHIN, Vladimir, UOZUMI, Teiji, YOSHIKAWA, Akimasa, KOGA, Kiyokazu, MATSUMOTO, Haruhisa

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • ELF波形から推定された雷放電の放電電荷量と極端気象現象との関係

    清水 千春, 佐藤 光輝, 高橋 幸弘, 土屋 史紀, 本間 規泰, 本郷 保二, 阿部 修司, 吉川 顕正

    日本地球惑星科学連合2015年大会  2015.5 

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    Event date: 2015.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張市, 幕張メッセ   Country:Japan  

  • The features of vertical component of daily geomagnetic field during geomagnetic storm International conference

    H. Matsushita, Akimasa Yoshikawa

    United Nations/Japan for Space Weather Symposium  2015.3 

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    Event date: 2015.3

    Language:English   Presentation type:Symposium, workshop panel (public)  

    Venue:Fukuoka   Country:Japan  

  • Characteristics of equatorial Pc 5 during electron flux enhancement International conference

    K. Akimoto, Akimasa Yoshikawa

    United Nations/Japan for Space Weather Symposium  2015.3 

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    Event date: 2015.3

    Language:English   Presentation type:Symposium, workshop panel (public)  

    Venue:Fukuoka   Country:Japan  

  • The features of vertical component of daily geomagnetic field during geomagnetic storm International conference

    H. Matsushita, Akimasa Yoshikawa

    United Nations/Japan for Space Weather Symposium  2015.3 

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    Event date: 2015.3

    Language:English   Presentation type:Symposium, workshop panel (public)  

    Venue:Fukuoka   Country:Japan  

  • Improved Hodograph Method and the Amplitude-Phase Gradient Method to estimate the latitude dependence of the FLR frequency, plasma density, and the resonance width using data from a ground magnetometer pair: Application to CARISMA and MAGDAS station pairs in North America International conference

    Hideaki Kawano, V. Pilipenko, I. Mann, D. Milling, S. Saita, K. Kitamura, Kiyohumi Yumoto, Akimasa Yoshikawa

    AGU fall meeting  2014.12 

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    Event date: 2014.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco, USA   Country:United States  

  • Relationship between Relativistic Electron Flux in the Inner Magnetosphere and ULF Pulsation on the Ground Associated with Long-term Variations of Solar Wind International conference

    Kitamura K., T. Nagatsuma, O. Troshichev, T. Obara, H. Koshiishi, S. Saita, Akimasa Yoshikawa, Kiyohumi Yumoto

    AGU fall meeting  2014.12 

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    Event date: 2014.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco, USA   Country:United States  

  • Pi 2 Pulsations Associated with Ionospheric Currents Produced By Oscillating Nightside Field-Aligned Currents International conference

    Imajo S., T. Uozumi, S. Ohtani, A. Nakamizo, Kiyohumi Yumoto, Akimasa Yoshikawa

    AGU fall meeting  2014.12 

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    Event date: 2014.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco, USA   Country:United States  

  • A Proposal of Global Data System for Solar-Terrestrial Sciencea, AGU fall meeting International conference

    Iyemori T, K. Shiokawa, T. Nakamura, T. Obara, Kiyohumi Yumoto, T. Tsuda, K. Shibata, I. Shinohara, Y. Takahashi, Akimasa Yoshikawa, B. Ritschel

    AGU fall meeting  2014.12 

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    Event date: 2014.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:San Francisco, USA   Country:United States  

  • 電離層伝導度の定式化

    家田 章正, 大山 伸一郎, 藤井 良一, 中溝 葵, 堀 智昭, 西谷 望, Akimasa Yoshikawa

    Japan GeoScience Union Meeting 2014  2014.4 

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    Event date: 2014.4 - 2014.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:Pacifico Yokohama   Country:Japan  

  • JAXA準天頂衛星とMAGDAS地上観測点による沿磁力線電流の同時観測

    竹内 勇人, 河野 英昭, Akimasa Yoshikawa, 東尾 奈々, 松本 晴久, Baishev Dmitry G, 魚住 禎司, 阿部 修司, 湯元 清文

    Japan GeoScience Union Meeting 2014  2014.4 

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    Event date: 2014.4 - 2014.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:Pacifico Yokohama   Country:Japan  

  • 磁気赤道におけるDP2侵入電場の午前・午後非対称性について

    松下 拓輝, Akimasa Yoshikawa, 魚住 禎司, 池田 昭大, 大谷 晋一

    Japan GeoScience Union Meeting 2014  2014.4 

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    Event date: 2014.4 - 2014.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:Pacifico Yokohama   Country:Japan  

  • 朝夕昼夜境界付近で観測されるPi 2型地磁気脈動の性質

    今城 峻, Akimasa Yoshikawa, 魚住 禎司, 大谷 晋一, 中溝 葵, Marshall Richard, Shevtsov Boris M, Akulichev Victor A, Sukhbaatar Usnikh, 河野 英昭

    Japan GeoScience Union Meeting 2014  2014.4 

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    Event date: 2014.4 - 2014.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:Pacifico Yokohama   Country:Japan  

  • 北海道HFレーダーと地上磁場におけるPc 4脈動の同時観測研究

    尾花 由紀, 西谷 望, 堀 智昭, 寺本 万里子, 能勢 正仁, Akimasa Yoshikawa

    Japan GeoScience Union Meeting 2014  2014.4 

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    Event date: 2014.4 - 2014.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:Pacifico Yokohama   Country:Japan  

  • Latitude profiles of the FLR frequency and the resonance width estimated by using the improved hodograph method and the APGM method International conference

    Hideaki Kawano, Viacheslav Pilipenko, Ian R. Mann, David K. Milling, Kentarou Kitamura, Akimasa Yoshikawa, Kiyohumi Yumoto

    AGU General Assembly 2013  2013.12 

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    Event date: 2013.12

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Moscone Convention Center, San Francisco, USA   Country:United States  

  • Pc5 activity during geomagnetic storm in Indonesia International conference

    Nuraeni, F., A. Santoso, C. Y. Yatini, Akimasa Yoshikawa, S. Abe, Kiyohumi Yumoto

    SCOSTEP, International CAWSES-II meeting  2013.11 

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    Event date: 2013.11

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Nagoya, Japan   Country:Japan  

  • Report of capacity-building activities of Japan during CAWSES-II period International conference

    Ueno, S, Kiyohumi Yumoto, Akimasa Yoshikawa, K. Makita, K. Munakata, A Mizuno, T. Tsuda

    SCOSTEP, International CAWSES-II meeting  2013.11 

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    Event date: 2013.11

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Nagoya, Japan   Country:Japan  

  • Development of QSAT-EOS : Residual magnetism measurement toward the analysis of low altitude magnetic disturbance,

    和田 宏太朗, 吉川 顕正, 魚住 禎司, 阿部 修司, 湯元 清文

    第134回SGEPSS 総会及び講演会  2013.11 

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    Event date: 2013.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:高知大学朝倉キャンパス   Country:Japan  

  • FMCWレーダードップラーモードによる磁気嵐中の極域侵入電場の観測

    有金 聡, 北村 健太郎, 長妻 努, 近藤 巧, 吉川 顕正, 湯元 清文

    第134回SGEPSS 総会及び講演会  2013.11 

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    Event date: 2013.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:高知大学朝倉キャンパス   Country:Japan  

  • 改良一観測点法を用いた宙空プラズマ密度分布の診断に向けて

    太田 聡, 河野 英昭, 魚住 禎司, 阿部 修司, 吉川 顕正, MAGDAS/CPMNグループ

    第134回SGEPSS 総会及び講演会  2013.11 

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    Event date: 2013.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:高知大学朝倉キャンパス   Country:Japan  

  • The relation between amplitudes of a global-mode Pc 5 pulsations and geosynchronous electron fluxes

    Magdi E Yousif Suliman, Akimasa Yoshikawa, K. Yumoto, Hideaki Kawano, Teiji Uozumi, S. Abe, M. G. Cardinal, Paolo Palangio, Lynn Kaisan

    2013 3rd IEEE International Conference on Space Science and Communication, IconSpace 2013  2013.12 

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    Event date: 2013.7

    Language:English  

    Venue:Melaka   Country:Malaysia  

    Associative relationship between magnetospheric ULF waves in the Pc 5 range (1.7-6.7 mHz) and high energetic particles on the geosynchronous orbit has been investigated in detail in past studies. In particular, there has been interest in the efficiency of global Pc 5 waves, i.e., those having small m-numbers, in accelerating particles [1]. In this paper we investigated this feature by using energetic electron fluxes at geosynchronous orbits, and by using low-latitude global-mode Pc 5 pulsations: We used superposed epoch analyses to show correlations.

  • The relation between amplitudes of a global-mode Pc 5 pulsations and geosynchronous electron fluxes

    Magdi E.Yousif Suliman, A. Yoshikawa, K. Yumoto, H. Kawano, Teiji Uozumi, S. Abe, M. G. Cardinal, Paolo Palangio, Lynn Kaisan

    2013 3rd IEEE International Conference on Space Science and Communication, IconSpace 2013  2013.12 

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    Event date: 2013.7

    Language:English  

    Venue:Melaka   Country:Malaysia  

    Associative relationship between magnetospheric ULF waves in the Pc 5 range (1.7-6.7 mHz) and high energetic particles on the geosynchronous orbit has been investigated in detail in past studies. In particular, there has been interest in the efficiency of global Pc 5 waves, i.e., those having small m-numbers, in accelerating particles [1]. In this paper we investigated this feature by using energetic electron fluxes at geosynchronous orbits, and by using low-latitude global-mode Pc 5 pulsations: We used superposed epoch analyses to show correlations.

  • Ionospheric Current Identified by Propagation Characteristics of DP2 and Pc5 International conference

    Hiroki MATSUSHITA, Akimasa Yoshikawa, T. Uozumi, A. Ikeda, Kiyohumi Yumoto

    AOGS Annual meeting  2013.6 

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    Event date: 2013.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Brisbane, Australia   Country:Australia  

    81. Hiroki MATSUSHITA, Akimasa YOSHIKAWA, Teiji UOZUMI, Akihiro IKEDA, Kiyohumi YUMOTO (2013), Ionospheric Current Identified by Propagation Characteristics of DP2 and Pc5, AOGS Annual meeting, 24-28, June, 2013, Brisbane, Australia

  • Characteristics of Quarter-Wave ULF Pulsations Around the Dawn Terminator International conference

    Yuki OBANA, Frederick MENK, Colin WATERS, Murray SCIFFER, Akimasa Yoshikawa, Farideh HONARY, Mark MOLDWIN, Ian MANN, David BOTELE, Vassilis ANGELOPOULOS, Chris RUSSELL

    AOGS Annual meeting  2013.6 

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    Event date: 2013.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Brisbane, Australia   Country:Australia  

  • Characteristics of Azimuthally Polarized Pi 2 on the Morning Side International conference

    Shun Imajo, Akimasa Yoshikawa, T. Uozumi, S.Ohtani, Kiyohumi Yumoto

    AOGS Annual meeting  2013.6 

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    Event date: 2013.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:Brisbane, Australia   Country:Australia  

  • タスマニア-ニュージーランド地磁気観測網による磁力線共鳴振動の詳細観測

    尾花 由紀, 塩川和夫, 寺本万里, 柿並義宏, 才田聡子, 吉川 顕正, 田中良昌, Frederick W. Menk, Colin L. Waters, Craig J. Rodger

    2013年度日本地球惑星科学連合大会  2013.5 

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    Event date: 2013.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 極域昼夜境界近傍の電流系について

    田中 良昌, 佐藤 夏雄, 行松 彰, 堀智昭, 吉川 顕正, 高崎 聡子

    第3回極域科学シンポジウム  2012.11 

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    Event date: 2012.11

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所、東京都 立川市   Country:Japan  

  • Global-mode Pc 5 pulsations: Ground distribution and correlation with energetic particles in the inner magnetosphere

    Magdi Yousif suliman, Kiyohumi Yumoto, Akimasa Yoshikawa, Teiji Uozumi

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • 極域昼夜境界近傍の電離圏電流系 International conference

    田中 良昌, 行松 彰, 佐藤 夏雄, 堀 智昭, 吉川 顕正

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • 地上低緯度と静止軌道で同時観測された Pi 2 の強度の統計解析

    今城 峻, 湯元 清文, 魚住禎司, 古賀 清一, 小原 隆博, Hideaki Kawano, 吉川 顕正, 阿部修司, 池田 昭

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • Seismo-electromagnetic anomalies in ELF range observed by an induction magnetometer in Kuju

    Daijirou Tanaka, Shuji Abe, Teiji Uozumi, Hideaki Kawano, Akimasa Yoshikawa, Huixin Liu, Kiyohumi Yumoto

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • Substorm current wedge model for Pi 2 pulsation revisited with the morphology of the global high-correlation Pi 2

    Teiji Uozumi, Kiyohumi Yumoto, Akimasa Yoshikawa

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • The Response of the Dayside Equatorial Electrojet to Step-like Changes of IMF Bz

    Shin Ohtani, Teiji Uozumi, Hideaki Kawano, Akimasa Yoshikawa, Kiyohumi Yumoto

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • The relationship between solar wind parameters and dayside equatorial Pc 4 pulsations

    Maria Gracita Cardinal, Hideaki Kawano, Kiyohumi Yumoto, Akimasa Yoshikawa, Teiji Uozumi, Shuji Abe, Babatunde Rabiu

    第132回 地球電磁気・地球惑星圏学会総会・講演会  2012.10 

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    Event date: 2012.10

    Language:English   Presentation type:Oral presentation (general)  

    Venue:札幌コンベンションセンター   Country:Japan  

  • Characteristics of Quarter-Wave ULF Pulsations around the dawn terminator International conference

    Yuki Obana, Akimasa Yoshikawa

    AOGS 10th Annual Meeting  2012.6 

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    Event date: 2012.6

    Language:English   Presentation type:Oral presentation (general)  

    Venue:&#8232;Brisbane Convention & Exhibition Centre, Australia   Country:Japan  

  • Solar cycle dependence of the solar wind control on the geomagnetic activity

    Nurul Shazana Abdul Hamid, 湯元 清文, LIU HUIXIN, 魚住禎司, 河野 英昭, 吉川 顕正, Mo-hamad Huzaimy Bin Jusoh

    2012年度日本地球惑星科学連合大会  2012.5 

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    Event date: 2012.5

    Language:English   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • MAGDAS地磁気観測ネットワークを用いた中間圏-熱圏-電離圏結合過程の研究

    阿部修司, 湯元 清文, Hideaki Kawano, 吉川 顕正, 魚住禎司, 前田丈二, 池田 昭大

    2012年度日本地球惑星科学連合大会  2012.5 

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    Event date: 2012.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • タスマニア-ニュージーランド地域の新しい地磁気観測網によるULF周波数帯地磁気脈動の観測

    尾花由紀, 柿並 義宏, 才田 聡子, 吉川 顕正, 田中 良昌

    2012年度日本地球惑星科学連合大会  2012.5 

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    Event date: 2012.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 低緯度Pi2観測時の磁気圏内での空間的磁場変動

    今城 峻, 湯元 清文, 魚住禎司, 古賀 清一, 小原 隆博, Hideaki Kawano, 吉川 顕正, 阿部修司, 池田 昭

    2012年度日本地球惑星科学連合大会  2012.5 

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    Event date: 2012.5

    Language:Japanese   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ,千葉県幕張市   Country:Japan  

  • 1/4波長モード磁力線共鳴振動の空間分布と共鳴特性について

    尾花由紀, Menk Frederick W., Waters Colin L., Sciffer Murray D., 吉川顕正, 吉川一朗, Moldwin Mark, Mann Ian R., Boteler David, Angelopoulos Vassilis, Russell C. T.

    地球電磁気・地球惑星圏学会,第130回総会・講演会  2011.11 

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    Event date: 2011.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:神戸大学六甲第2キャンパス.   Country:Japan  

  • 地上–静止軌道で同時観測されたサブストーム・カレントウェッジの上向き/下向き沿磁力線電流に伴うPi 2地磁気脈動

    魚住 禎司, 湯元 清文, 今城 峻, 古賀 清一, 小原 隆博, Baishev Dmitry, Shevtsov Boris M., Milling David, Mann Ian R., 池田 昭大, 阿部 修司, 吉川 顕正, 河野 英昭

    地球電磁気・地球惑星圏学会,第130回総会・講演会  2011.11 

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    Event date: 2011.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:神戸大学六甲第2キャンパス.   Country:Japan  

  • Timing relation between positive bay onsets, Pi 2onsets, auroral initial brightenings and auroral breakups

    徳永 旭将, 中村 和幸, 樋口 知之, 魚住 禎司, 吉川 顕正, 森岡 昭, 湯元 清文, MAGDAS/CPMNグループ 湯元 清文

    地球電磁気・地球惑星圏学会,第130回総会・講演会  2011.11 

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    Event date: 2011.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:神戸大学六甲第2キャンパス.   Country:Japan  

  • タスマニア-ニュージーランド地域における新しい地磁気観測計画:初期解析結果について

    尾花 由紀, 塩川 和夫, 吉川 顕正, 田中 良昌, 才田 聡子, Frederick. W. Menk, Colin. L. Waters, Brian. J. Fraser, Craig. J. Rodger

    日本惑星連合2011年大会  2011.5 

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    Event date: 2011.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ、千葉県幕張市   Country:Japan  

  • 地上-静止軌道で同時観測されたサブストーム・カレントウエッジに伴うPi 2地磁気脈動

    魚住 禎司, 湯元 清文, 古賀 清一, 小原 隆博, B. M. シェフトソフ, S. I. ソロブエフ, 池田 昭大, 阿部 修司, 吉川 顕正, 河野 英昭

    日本惑星連合2011年大会  2011.5 

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    Event date: 2011.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ、千葉県幕張市   Country:Japan  

  • FM-CWレーダーとMAGDASによって観測された長周期の磁場・電場変動

    池田 昭大, 湯元 清文, 柿並 義宏, 篠原 学, 野崎 憲朗, 長妻 努, 吉川 顕正, B. M. Shevtsov, V. V. Bychkov, Q. M. Sugon, Jr., D. McNamara

    日本惑星連合2011年大会  2011.5 

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    Event date: 2011.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ、千葉県幕張市   Country:Japan  

  • Singular Value Transformationを用いた地上磁場からのサブストームオンセットの同定

    徳永 旭将, 湯元 清文, 魚住 禎司, 吉川 顕正, 中村 和幸, 樋口 知之, 池田 大輔, MAGDAS/CPMN グループ

    日本惑星連合2011年大会  2011.5 

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    Event date: 2011.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ、千葉県幕張市   Country:Japan  

  • 朝側オーロラパッチのドリフト振動とULF地磁気脈動の関係

    田中 良昌, 海老原 祐輔, 吉川 顕正, 才田 聡子, 小川 泰信, 宮岡 宏, Allan Weatherwax

    日本惑星連合2012年大会  2011.5 

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    Event date: 2011.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:幕張メッセ、千葉県幕張市   Country:Japan  

  • AKR modulation and Global Pi 2 oscillation: Jan. 24, 1997 event International conference

    Teiji Uozumi, K. Yumoto, T. Tokunaga, S. I. Solovyev, B. M. Shevtsov, R. Marshall, K. Liou, S. Ohtani, S. Abe, A. Ikeda, K. Kitamura, A. Yoshikawa, H. Kawano, and M. Itonaga

    AGU Chapman Conference on Relationship Between Auroral Phenomenology and Magnetospheric Processes  2011.3 

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    Event date: 2011.3

    Presentation type:Oral presentation (general)  

    Venue:Fairbanks, Alaska   Country:United States  

  • 変化点検出を応用した時系列データからの突発現象の前兆検出アルゴリズム

    徳永旭将, 池田大輔, 中村和幸, 樋口知之, 吉川顕正, 魚住禎司, 藤本晶子, 森岡昭, 湯元清文, CPMN Group

    第 81 回「数理モデル化と問題解決(MPS)研究会」合同研究会  2010.12 

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    Event date: 2010.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:九州大学伊都キャンパス総合学習プラザ   Country:Japan  

  • Night-side DP-2 type fluctuations observed by the FM-CW Radar and MAGDAS stations International conference

    Ikeda, A., K Yumoto, T Uozumi, S Abe, M Shinohara, K Nozaki, A.Yoshikawa, V Bychkov, B Shevtsov, Q Sugon, and D McNamara

    2010 AGU Fall Meeting  2010.12 

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    Event date: 2010.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:San Francisco   Country:United States  

  • Various Aspect of the Field Line Resonance Phenomena Observed at the South Pole Station International conference

    Tanaka, Y.-M., Y. Ebihara, A. Yoshikawa, S. Saita, A. T. Weatherwax

    2010 AGU Fall Meeting  2010.12 

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    Event date: 2010.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:San Francisco   Country:United States  

  • Multipoint Observation of Quarter-Wave Length, Standing Alfvén Modes International conference

    Obana Y., I. Yoshikawa, F. W. Menk, C. L. Waters, M. D. Sciffer, A. Yoshikawa, M. B. Moldwin, I. R. Mann, and D. Boteler

    2010 AGU Fall Meeting  2010.12 

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    Event date: 2010.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:San Francisco   Country:United States  

  • 南極点基地の地磁気・光学観測で捉えた磁力線共鳴現象

    田中良昌, 海老原祐輔, 吉川顕正, 才田聡子, A. T. Weatherwax

    第34回極域宙空圏シンポジウム  2010.12 

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    Event date: 2010.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:国立極地研究所   Country:Japan  

  • New Pi 2 Index Based on MAGDAS/CPMN Network Data

    坂井 美菜, 魚住 禎司, 徳永 旭将, 河野 英昭, 吉川 顕正, 池田 昭大, 阿部 修司, 湯元 清文, MAGDAS/CPMNグループ

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • AKR modulation and Global Pi 2 oscillation: Jan.24, 1997 event

    魚住 禎司, 湯元 清文, Solovyev Stepan I. Shevtsov Boris M., Marshall Richard, Liou Kan, 大谷 晋一, 阿部 修司, 北村 健太郎, 吉川 顕正, 河野 英昭, 糸長 雅弘

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • 南極点基地で観測されたPoleward Moving Auroral Arcsとその解釈

    田中 良昌, 海老原 祐輔, 吉川 顕正, 才田 聡子, Weatherwax Allan

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • Long-term Sun-Earth system variations based on MAGDAS/CPMN data

    湯元 清文, 阿部 修司, 山崎 洋介, 魚住 禎司, 吉川 顕正, 藤本 晶子, 篠原 学, Jusoh Mohamad, Huzaimy, IUGONETプロジェクトチーム, MAGDAS/CPMNグループ

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • Long-term Sun-Earth system variations based on MAGDAS/CPMN data

    湯元 清文, 阿部 修司, 山崎 洋介, 魚住 禎司, 吉川 顕正, 藤本 晶子, 篠原 学, Jusoh Mohamad, Huzaimy, IUGONETプロジェクトチーム, MAGDAS/CPMNグループ

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • Characteristics of the night-side DP-2 type fluctuations observed by MAGDAS/CPMN

    池田 昭大, 湯元 清文, 魚住 禎司, 阿部 修司, 篠原 学, 野崎 憲朗, 吉川 顕正, Shevtsov Boris M., Bychkov Vasily, Sugon Quirino, McNamara Daniel, MAGDAS/CPMNグループ

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • タスマニア-ニュージーランド地域における磁力線共鳴1/4 λ・高調波モードの観測計画

    尾花 由紀, 塩川 和夫, 吉川 顕正, 田中 良昌, 才田 聡子, Menk Frederick W., Waters Colin L., Fraser Brian J.

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • 4分の1波長モード定在アルフヴェン波の励起条件について

    尾花 由紀, 吉川 一朗, Menk Frederick W., Waters Colin L., Sciffer Murray D., 吉川 顕正, Moldwin Mark, Mann Ian R., Boteler David

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • ERG計画における連携地上ネットワーク観測

    塩川 和夫, 西谷 望, 菊池 崇, 大塚 雄一, 三好 由純, 藤井 良一, 湯元 清文, 河野 英昭, 吉川 顕正, 篠原 学, 北村 健太郎, 佐藤 夏雄, 行松 彰, 山岸 久雄, 門倉 昭, 小川 泰信, 田中 良昌, 長妻 努, 田口 真, 細川 敬祐, 橋本 久美子, 尾崎 光紀, 大矢 浩代, ERG連携地上観測グループ

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • ERG計画における連携地上ネットワーク観測

    塩川 和夫, 西谷 望, 菊池 崇, 大塚 雄一, 三好 由純, 藤井 良一, 湯元 清文, 河野 英昭, 吉川 顕正, 篠原 学, 北村 健太郎, 佐藤 夏雄, 行松 彰, 山岸 久雄, 門倉 昭, 小川 泰信, 田中 良昌, 長妻 努, 田口 真, 細川 敬祐, 橋本 久美子, 尾崎 光紀, 大矢 浩代, ERG連携地上観測グループ

    地球電磁気・地球惑星圏学会,第128回総会・講演会  2010.11 

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    Event date: 2010.10 - 2010.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:沖縄県市町村自治会   Country:Japan  

  • Detecting precursory events in time series data by an extension of singular spectrum transformation

    Terumasa Tokunaga, Daisuke Ikeda, Kazuyuki Nakamura, Tomoyuki Higuchi, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto, Akira Morioka, Kiyofumi Yumoto

    10th WSEAS International Conference on Applied Computer Science, ACS'10  2010.12 

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    Event date: 2010.10

    Language:English  

    Venue:Iwate   Country:Japan  

    To predict an occurrence of extraordinary phenomena, such as earthquakes, failures of engineering system and financial market crushes, it is important to identify precursory events in time series. However, existing methods are limited in their applicability for real world precursor detections. Recently, Ide and Inoue [1] have developed an SSA-based change-point detection method, called singular spectrum transformation (SST). In this paper, we extend the SST so that it is applicable for real world precursor detections, focusing on the wide applicability of the conventional SST. Although the SST is suitable for detecting various types of change-points, detecting precursors can be far more difficult than expected because, in general, real world time series contains measurement noise and non-stationary trends. Furthermore, precursory events are usually observed as minute and less-visible fluctuations preceding an onset of massive fluctuations of extraordinary phenomena and therefore they are easily over-looked. To overcome this, we extend the conventional SST to the multivariable SST, focusing on the synchronism detection of precursory events in multiple sequences of univariate time series. First, we would like to define the problem setting of real world precursory detections and consider its difficulties. Second, the multivariable SST is introduced. Third, we apply SST to geomagnetic time series data and show the multivariable SST is more suitable than the conventional SST for real world precursor detections. Finally, we show further experimental results using artificial data to evaluate the reliability of SST-based precursor detections.

  • Detecting Precursory Events in Time Series Data by an Extension of Singular Spectrum Transformation International conference

    Tokunaga T., Daisuke Ikeda, Kazuyuki Nakamura, Tomoyuki Higuchi, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto, Akira Morioka, Kiyohumi Yumoto and CPMN group

    the 10th WSEAS International Conference on Applied Computer Science  2010.10 

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    Event date: 2010.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Iwate   Country:Japan  

  • Detecting Precursory Events in Time Series Data by an Extension of Singular Spectrum Transformation International conference

    Tokunaga T., Daisuke Ikeda, Kazuyuki Nakamura, Tomoyuki Higuchi, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto, Akira Morioka, Kiyohumi Yumoto and CPMN group

    the 10th WSEAS International Conference on Applied Computer Science  2010.10 

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    Event date: 2010.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Iwate   Country:Japan  

  • Detecting precursory events in time series data by an extension of singular spectrum transformation

    Terumasa Tokunaga, Daisuke Ikeda, Kazuyuki Nakamura, Tomoyuki Higuchi, Akimasa Yoshikawa, Teiji Uozumi, Akiko Fujimoto, Akira Morioka, Kiyofumi Yumoto

    10th WSEAS International Conference on Applied Computer Science, ACS'10  2010.12 

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    Event date: 2010.10

    Language:English  

    Venue:Iwate   Country:Japan  

    To predict an occurrence of extraordinary phenomena, such as earthquakes, failures of engineering system and financial market crushes, it is important to identify precursory events in time series. However, existing methods are limited in their applicability for real world precursor detections. Recently, Ide and Inoue [1] have developed an SSA-based change-point detection method, called singular spectrum transformation (SST). In this paper, we extend the SST so that it is applicable for real world precursor detections, focusing on the wide applicability of the conventional SST. Although the SST is suitable for detecting various types of change-points, detecting precursors can be far more difficult than expected because, in general, real world time series contains measurement noise and non-stationary trends. Furthermore, precursory events are usually observed as minute and less-visible fluctuations preceding an onset of massive fluctuations of extraordinary phenomena and therefore they are easily over-looked. To overcome this, we extend the conventional SST to the multivariable SST, focusing on the synchronism detection of precursory events in multiple sequences of univariate time series. First, we would like to define the problem setting of real world precursory detections and consider its difficulties. Second, the multivariable SST is introduced. Third, we apply SST to geomagnetic time series data and show the multivariable SST is more suitable than the conventional SST for real world precursor detections. Finally, we show further experimental results using artificial data to evaluate the reliability of SST-based precursor detections.

  • IONOSPHERIC ELECTRIC AND GROUND MAGNETICPC5 VARIATIONS AT LOW-LATITUDE STATIONS International conference

    Ikeda A., K, Yumoto, M. Shinohara, K. Nozaki, A. Yoshikawa, V. V. Bychkov, and B. M. Shevtsov

    SOLAR-TERRESTRIAL RELATIONS AND PHYSICS OF EARTHQUAKES PRECURSORS V INTERNATIONAL CONFERENCE  2010.8 

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    Event date: 2010.8

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Paratunka, Kamchatka   Country:Russian Federation  

  • Quarter Wave Field Line Resonances: Variation With Latitude Invited International conference

    F. W. Menk, Y. Obana, C. L. Waters, M. D. Sciffer, A. Yoshikawa, I. Yoshikawa, M. B. Moldwin, I. R. Mann, and D. Boteler

    38th COSPAR Scientific Assembly 2010  2010.7 

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    Event date: 2010.7

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Bremen, Germany   Country:Germany  

  • A comparison of low-latitude Pc 5pulsations observed by FM-CW ionospheric radar and MAGDAS/CPMN magnetometers Invited International conference

    Ikeda, A., K. Yumoto, M. Shinohara, K. Nozaki, T. Nagatsuma, A.Yoshikawa, T. Shimbaru, A. Fujimoto, B.M. Shevtsov, V. V. Bychkov, Q.M. Sugon, Jr., and D. McNamara

    2010 International Space Plasma Symposium  2010.6 

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    Event date: 2010.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Taipei, Taiwan   Country:Taiwan, Province of China  

  • SC and Pc 5 associated Ionospheric Electric and Ground Magnetic Field Variations at Low-latitude MAGDAS Station Invited International conference

    Ikeda A., K Yumoto, M Shinohara, K Nozaki, and A. Yoshikawa

    2010 Western Pacific Geophysics Meeting, 22–25 June 2010 &#8232;Taipei, Taiwan  2010.6 

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    Event date: 2010.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Taipei, Taiwan   Country:Taiwan, Province of China  

  • Quarter-wave modes of standing Alfvén waves detected by cross-phase analysis: Latitudinal distribution International conference

    Y Obana, F W Menk, C Waters, M D Sciffer, A. Yoshikawa, I Yoshikawa, M B Moldwin, I R Mann, D Boteler

    2010 Western Pacific Geophysics Meeting, 22–25 June 2010 &#8232;Taipei, Taiwan  2010.6 

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    Event date: 2010.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Taipei, Taiwan   Country:Taiwan, Province of China  

  • Enhancement of Equatorial Electrojet during the July 22, 2009 Solar Eclipse Event

    Teiji Uozumi, K. Yumoto, Y. Fujita, H. Watanabe, K. Imamura, M. Sakai, S. Abe, K. Kitamura, Y. Yamazaki, A. Yoshikawa, H. Kawano, Y. Kakinami, D. McNamara, A. B. Rabiu, I. A. Adimula, A. Bhattacharya, S. Alex, S. Gurubaran, S. L. G. Dutra, B. M. Shevtsov, R. Marshall and MAGDAS Group

    日本地球惑星連合2010年大会  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張メッセ   Country:Japan  

  • 低緯度・赤道MAGDAS観測点でのPc5周期帯電場・磁場変動

    池田 昭大, 湯元 清文, 魚住 禎司, 阿部 修司, 篠原 学, 野崎 憲朗, 吉川 顕正

    日本地球惑星連合2010年大会  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張メッセ   Country:Japan  

  • 特異スペクトル分析の応用による地上磁場テータからのオーロラサブストーム前兆検出

    徳永 旭将, 中村 和幸, 池田 大輔, 樋口 知之, 吉川 顕正, 魚住 禎司, 藤本 晶子, 森岡 昭, 湯元 清文

    日本地球惑星連合2010年大会  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張メッセ   Country:Japan  

  • Sq 変動経験モデルの構築とその変数依存性

    山崎洋介, 湯元清文, 吉川 顕正, 魚住 禎司

    日本地球惑星連合2010年大会  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張メッセ   Country:Japan  

  • 東アジア地域におけるグローバルSq電流系と赤道ジェット電流の関係について

    山崎洋介, 湯元清文, 吉川 顕正, 魚住 禎司

    日本地球惑星連合2010年大会  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張メッセ   Country:Japan  

  • 4分の1波長モード定在アルフヴェン波の多点同時観測:緯度方向分布について

    尾花由紀, 吉川一朗, Frederick W. Menk, Colin L. Waters, Murray D. Sciffer, 吉川顕正, Mark Moldwin, Ian R. Mann, David Boteler

    日本地球惑星連合2010年大会  2010.5 

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    Event date: 2010.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉県幕張メッセ   Country:Japan  

  • LT and MLT Dependencies of Pc 4 Amplitudes at CPMN Conjugate Stations International conference

    Y. Obana, A. Yoshikawa, R.J.Morris, B. J. Fraser, J.V.Olson, S.I. Solovyev, K. Yumoto

    AGU Fall meeting  2009.12 

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    Event date: 2009.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:&#8232;Moscone Convention Center&#8232;Howard Street, Between Third & Fifth Sts.&#8232;San Francisco, California, USA   Country:United States  

  • Ground-based observation networks for the ERG projec

    Shiokawa, K., N. Nishitani, T. Kikuchi, Y. Otsuka, R. Fujii, K. Yumoto, H. Kawano, A. Yoshikawa, N. Sato, A. Yukimatsu, H. Yamagishi, A. Kadokura, Y. Ogawa, M. Taguchi, K. Hosokawa, and K. Hashimoto

    平成20年度 磁気圏電離圏シンポジウム  2008.11 

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    Event date: 2009.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:宇宙航空研究開発機構 宇宙科学研究本部   Country:Japan  

  • FM-CW Radar Array Observation International conference

    Ikeda A., K. Yumoto, M. Shinohara, K. Nozaki, A. Yoshikawa, B.M. Shevtsov, V.V. Bychkov, D.Mcnamara

    URSI/COSPAR INTERNATIONAL REFERENCE IONOSPHERE WORKSHOP  2009.11 

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    Event date: 2009.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Inamori Hall, Kagoshima University, Kagoshima   Country:Japan  

  • New Empirical Sq Current Model based on the 210 MM CPMN Data from 1996-2007 International conference

    Terada H., Y. Yamazaki, Y. Kakinami, S. Abe, T. Uozumi, A. Yoshikawa, K. Yumoto, CPMN group

    URSI/COSPAR INTERNATIONAL REFERENCE IONOSPHERE WORKSHOP  2009.11 

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    Event date: 2009.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Inamori Hall, Kagoshima University, Kagoshima   Country:Japan  

  • DP2 type fluctuations observed by FM-CW HF radar array International conference

    Shinohara M., A. Ikeda, K. Nozaki, A. Yoshikawa, B. M. Shevtsov, V. V. Bychkov, K. Yumoto, and MAGDAS/CPMN Group

    URSI/COSPAR INTERNATIONAL REFERENCE IONOSPHERE WORKSHOP  2009.11 

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    Event date: 2009.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Inamori Hall, Kagoshima University, Kagoshima   Country:Japan  

  • Phase Relation of the Ionospheric Doppler Velocity with Magnetic Pi 2 Pulsations: FM-CW Radar and MAGDAS Observation

    池田昭大, 湯元 清文, 魚住 禎司, 篠原学, 野崎憲朗, 吉川顕正

    第126回 SGEPSS総会および講演会  2009.9 

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    Event date: 2009.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:金沢大学角間キャンパス   Country:Japan  

  • A new interpretation of high-latitude Pi 2 observed at the MAGDAS/CPMN stations

    魚住禎司, 阿部修司, 北村健太郎, 徳永旭将, 吉川顕正, 河野英昭, Marshall Richard, Morris R. J., Shevtsov Boris M., Solovyev S. I., McNamara Daniel, Liou Kan, 大谷晋一, 糸長雅弘, 湯元清文

    第126回 SGEPSS総会および講演会  2009.9 

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    Event date: 2009.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:金沢大学角間キャンパス   Country:Japan  

  • ULTIMA Magnetic Power Spectral Density and its Radial Diffusion Coefficients for Relativistic Electron Enhancement

    藤本晶子, 徳永旭将, 阿部修司, 魚住禎司, 吉川顕正, Mann Ian R., Chi Peter J., Engebretson Mark, 湯元清文, MAGDAS/CPMNグループ

    第126回 SGEPSS総会および講演会  2009.9 

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    Event date: 2009.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:金沢大学角間キャンパス   Country:Japan  

  • 地上観測されたPi 2型地磁気脈動のグローバルな 波動特性解析のための周波数領域独立成分分析の応用

    徳永旭将, 吉川顕正, 魚住禎司, 樋口知之, 中村和幸, 湯元清文, MAGDAS/CPMNグループ

    第126回 SGEPSS総会および講演会  2009.9 

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    Event date: 2009.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:金沢大学角間キャンパス   Country:Japan  

  • A detection of substorm precursors on geomagnetic data at auroral latitudes by SSA-based change-point analysis

    徳永旭将, 中村和幸, 樋口知之, 吉川顕正, 魚住禎司, 森岡昭, 湯元清文, MAGDAS/CPMNグループ

    第126回 SGEPSS総会および講演会  2009.9 

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    Event date: 2009.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:金沢大学角間キャンパス   Country:Japan  

  • 数値計算プロジェ クトの将来像と惑星電磁圏の理解の今後 Invited

    寺田直樹, 陣英克, 松本洋介, 梅田隆行, 深沢圭一郎, 三好隆博, 加藤雄人, 鈴木朋憲, 三好勉信, 藤原均, 品川裕之, 寺田香織, 村田健史, 吉川顕正, 三好由純, 中田裕之

    第126回 SGEPSS総会および講演会  2009.9 

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    Event date: 2009.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:金沢大学角間キャンパス   Country:Japan  

  • Automatic Identification of Pi 2 Pulsations using MAGDAS/CPMN Network –Toward Construction of a new Pi 2 Index–

    坂井美菜, 徳永旭将, 魚住禎司, 阿部修司, 池田昭大, 吉川顕正, 河野英昭, 湯元清文, MAGDAS/CPMNグループ

    第126回 SGEPSS総会および講演会  2009.9 

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    Event date: 2009.9

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:金沢大学角間キャンパス   Country:Japan  

  • Pi 2 Pulsations Observed by an FM-CW Ionospheric Radar and MAGDAS Magnetometer at Mid-latitude Station International conference

    Ikeda A., K. Yumoto, T. Uozumi, M. Shinohara, K. Nozaki, A. Yoshikawa, V. V. BychkovB,

    2009 UN BSS & IHY Workshop  2009.9 

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    Event date: 2009.9 - 2009.8

    Presentation type:Oral presentation (general)  

    Venue:Daejion   Country:Korea, Republic of  

    Annual and Semiannual Variations of Equivalent Sq Current System along the 210 MM CPMN Stations

  • Annual and Semiannual Variations of Equivalent Sq Current System along the 210 MM CPMN Stations International conference

    Yamazak Y.i, K. Yumoto, T. Uozumi, and A. Yoshikawa

    2009 UN BSS & IHY Workshop  2009.9 

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    Event date: 2009.9 - 2009.8

    Presentation type:Oral presentation (general)  

    Venue:Daejion   Country:Korea, Republic of  

    Annual and Semiannual Variations of Equivalent Sq Current System along the 210 MM CPMN Stations

  • Online EE-index for the Real-time Geospace Monitoring

    上野民記, 沼田有司, 山崎洋介, 湯元清文, 阿部修司, 魚住禎司, 河野英昭, 吉川顕正, 篠原学

    日本地球惑星科学連合2009年大会  2009.5 

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    Event date: 2009.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉, 幕張国際会議場   Country:Japan  

  • The spatial and temporal behavior of Pc 5 ULF at ULTIMA stations during magnetic storms

    藤本晶子, 徳永旭将, 阿部修司, 魚住禎司, 吉川顕正, MannIan R., J. EngebretsonMark, BhattacharyaArchana, McNamaraDaniel, PollittRonald W., L.G., RabiuAkeem Babatunde, 湯元清文

    日本地球惑星科学連合2009年大会  2009.5 

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    Event date: 2009.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉, 幕張国際会議場   Country:Japan  

  • Pi 2-associated Ionosperic Doppler Velocity and Magnetic Pulsation at Mid-latitude MAGDAS Station

    池田昭大, 湯元清文, 魚住禎司, 篠原学, 野崎憲朗, 吉川顕正, BychkovVasily V., ShevtsovBoris M.

    日本地球惑星科学連合2009年大会  2009.5 

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    Event date: 2009.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉, 幕張国際会議場   Country:Japan  

  • 時系列データマイニングによる動的ヘテロなシステムからの知識発見 -宇宙天気研究における大規模帰納処理システム

    徳永旭将, 中村和幸, 樋口知之, 池田大輔, 大久保翔, 藤本晶子, 吉川顕正, 湯元清文, MAGDAS/CPMNグループ

    日本地球惑星科学連合2009年大会  2009.5 

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    Event date: 2009.5

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:千葉, 幕張国際会議場   Country:Japan  

  • Global nature of Pc5 magnetic pulsation during the WHI observation campaign International conference

    Fujimoto A., T. Tokunaga, S. Abe, T. Uozumi, A. Yoshikawa, K. Yumoto and CPMN/MAGSAS Group

    AGU Fall Meeting  2008.12 

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    Event date: 2008.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:San Francisco, USA   Country:United States  

  • Low-latitude Pi2 Pulsations observed by an FM-CW Radar and CPMN Stations International conference

    Ikeda A., K. Yumoto, T. Uozumi, M. Shinohara, K. Nozaki and A. Yoshikawa

    AGU Fall Meeting  2008.12 

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    Event date: 2008.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:San Francisco, USA   Country:United States  

  • Characteristics of 3-component Magnetic Fields of Equatorial Pi 2s-MAGDAS/CPMN Observations in Daytime and Nighttime International conference

    Hirayama Y., K. Yumoto, T. Uozumi, A. Yoshikawa, MAGDAS/CPMN Group

    AGU Fall Meeting  2008.12 

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    Event date: 2008.12

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:San Francisco, USA   Country:United States  

  • MAGDAS Project at SERC for Litho-Space Weather International conference

    Yumoto K., H. Kawano, A. Yoshikawa, and MAGDAS Group

    2nd International Workshop on Space and Lithosphere Enviroment Changes in Asia (IWSLEC)  2008.11 

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    Event date: 2008.11

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:National Institute of Advanced Industrial Sciences and Technology (AIST), Tsukuba   Country:Japan  

  • Spectral Peaks of long-term EEJ variation

    沼田有司, 上野民記, 魚住禎司, 吉川顕正, 河野英昭, 湯元清文, MAGDAS/CPMNグループ

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • Global nature of Pc 5 magnetic pulsation during the WHI observation campaign

    藤本晶子, 徳永旭将, 阿部修司, 魚住禎司, 吉川顕正, 湯元清文, MAGDAS/CPMNグループ

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • Observations of Pi 2 Ionospheric Electric Fields by FM-CW radars

    池田昭大, 湯元清文, 篠原学, 魚住 禎司, 吉川顕正, 野崎 憲朗

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • モデル結合・融合方法の標準化 Invited

    寺田直樹, 中田裕之, 松本洋介, 深沢圭一郎, 陣英克, 三好勉信, 篠原育, 杉山徹, 梅田隆行, 海老原祐輔, 荻野竜樹, 加藤雄人, 金田香織, 久保勇樹, 品川裕之, 島津浩哲, 関華奈子, 田中高史, 坪内健, 中野慎也, 中村琢磨, 藤田茂, 藤原均, 三好隆博, 三好由純, 村田 健史, 吉川顕正

    第124回 SGEPSS総会および講演会  2008.10 

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    Event date: 2008.10

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:仙台市戦災復興記念館   Country:Japan  

  • FM-CW Radar Observations of Pi 2 Ionospheric Electric Fields at Low Latitude

    Ikeda A., K.Yumoto, T.Uozumi, M.Shinohara, K.Nozaki, A.Yoshikawa and K. Shiokawa

    第32回極域宙空圏シンポジウム  2008.8 

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    Event date: 2008.8

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:東京、板橋、国立極地研究所   Country:Japan  

  • Characteristics of Pi2 Electric and Magnetic Pulsations Observed at the Low-latitude CPMN Magnetometers and a FM-CW Radar International conference

    Ikeda A., K. Yumoto, T. Uozumi, M. Shinohara, K. Nozaki, A. Yoshikawa, K. Shiokawa

    AOGS 2008 meeting  2008.6 

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    Event date: 2008.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Busan, Korea   Country:Korea, Republic of  

  • Characteristics of SFEs observed at the Dip-Equator CPMN Stations International conference

    Yamazaki Y., K. Yumoto, A. Yoshikawa, S. Abe, A. Ikeda, T. Tokunaga, Y. Numata, S. Watari, H. Utada

    AOGS 2008 meeting  2008.6 

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    Event date: 2008.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Busan, Korea   Country:Korea, Republic of  

  • A New Index to Monitor Temporal and Long-Term Variations of the Equatorial Electrojet by MAGDAS/CPMN Real-Time Data: EE-Index International conference

    Uozumi T., K. Yumoto, K. Kitamura, S. Abe, Y., M. Shinohara, A. Yoshikawa, H. Kawano, T. Ueno, T. Tokunaga

    AOGS 2008 meeting  2008.6 

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    Event date: 2008.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Busan, Korea   Country:Korea, Republic of  

  • Nightside DP 2 Fluctuations Observed by FM-CW HF Radar and the MAGDAS/CPMN Network International conference

    Shinohara, M., A. Ikeda, K. Nozaki, A. Yoshikawa

    AOGS 2008 meeting  2008.6 

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    Event date: 2008.6

    Language:Others   Presentation type:Oral presentation (general)  

    Venue:Busan, Korea   Country:Korea, Republic of  

  • 大型研究計画「太陽地球系結合過程の研究基盤形成」マスタープラン2017への提案に向けて

    山本衛, 橋口浩之, 宮岡宏, 小川泰信, 塩川和夫, 野澤悟徳, 吉川顕正, 津田敏隆

    IUGONET研究集会・科学とデータ研究集会  2018.9 

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    Country:Japan  

  • Near-equatorial Pi2 and Pc3 waves observed by CHAMP and on SAMBA/MAGDAS stations

    F. Cuturrufo, V. Pilipenko, B. Heilig, M. Stepanova, H. Luehr, P. Vega, A. Yoshikawa

    ADVANCES IN SPACE RESEARCH  2015.2 

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    Country:Japan  

    We have examined simultaneous ULF activity in the Pi2 and Pc3 bands at the near-equatorial magnetic stations in South America from SAMBA and MAGDAS arrays and low-orbiting CHAMP satellite during its passage over this meridional network. At the nighttime, both Pi2 and Pc3 waves in the upper ionosphere and on the ground are nearly of the same magnitude and in-phase. At the same time, the daytime Pc3 pulsations on the ground and in space are nearly out-of-phase. Comparison of observational results with the theoretical notions on the MHD wave interaction with the system ionosphere atmosphere ground suggests that nighttime low-latitude Pi2 and Pc3 wave signatures are produced by magnetospheric fast compressional mode. The daytime near-equatorial Pc3 waves still resist a quantative interpretation. These waves may be produced by a combination of two mechanisms: compressional mode leakage through the ionosphere, and by oscillatory ionospheric current spreading towards equatorial latitudes. (C) 2014 COSPAR. Published by Elsevier Ltd. All rights reserved.

  • Lorentz Dispersion Law from classical Hydrogen electron orbits in AC electric field via geometric algebra

    Uzziel Perez, Angeleene S. Ang, Quirino M. Sugon Jr., Daniel J. McNamara, Akimasa Yoshikawa

    2015.7 

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    Country:Japan  

    We studied the orbit of an electron revolving around an infinitely massive
    nucleus of a large classical Hydrogen atom subject to an AC electric field
    oscillating perpendicular to the electron's circular orbit. Using perturbation
    theory in geometric algebra, we show that the equation of motion of the
    electron perpendicular to the unperturbed orbital plane satisfies a forced
    simple harmonic oscillator equation found in Lorentz dispersion law in Optics.
    We show that even though we did not introduce a damping term, the initial
    orbital position and velocity of the electron results to a solution whose
    absorbed energies are finite at the dominant resonant frequency
    $omega=omega_0$; the electron slowly increases its amplitude of oscillation
    until it becomes ionized. We computed the average power absorbed by the
    electron both at the perturbing frequency and at the electron's orbital
    frequency. We graphed the trace of the angular momentum vector at different
    frequencies. We showed that at different perturbing frequencies, the angular
    momentum vector traces epicyclical patterns.

  • 汎地球観測ネットワークを基軸とした宇宙天気研究・教育の革新的国際展開

    花田 俊也, 吉川 顕正, 山岡 均

    宇宙科学技術連合講演会講演集  2015.10 

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    Country:Japan  

    Innovative Globalization of Space Weather Science and Education Based on International Observation Network

  • 宇宙擾乱と地磁気誘導電流

    海老原 祐輔, 石井 守, 亘 慎一, 後藤 忠徳, 藤田 茂, 菊池 崇, 田中 高史, 久保田 康文, 吉川 顕正, 片岡 龍峰, 吉村 純, 中村 紗都子

    宇宙科学技術連合講演会講演集  2016.9 

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    Country:Japan  

    Geospace Disturbances and Geomagentically Induced Current

  • スペースデブリ環境の理解に向けて

    花田 俊也, 阿部 修司, 吉川 顕正, 藤田 浩輝

    宇宙科学技術連合講演会講演集  2016.9 

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    Country:Japan  

    Towards A Better Understanding of Space Debris Environment

  • QZSとMAGDAS地上磁力計による磁気圏FAC‐電離層電流回路の同時観測:初期統計解析

    河野英昭, 河野英昭, 小串修, 安倍松侑太, 東尾奈々, 松本晴久, MOISEEV A. V, BAISHEV D. G, 魚住禎司, 阿部修司, 吉川顕正, 吉川顕正

    宇宙航空研究開発機構特別資料 JAXA-SP-(Web)  2017.2 

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    QZSとMAGDAS地上磁力計による磁気圏FAC‐電離層電流回路の同時観測:初期統計解析

  • 長期の宇宙天気活動に伴うスペースデブリ環境の推移予測

    阿部修司, 花田俊也, 吉川顕正, 平井隆之, 河本聡美

    宇宙航空研究開発機構特別資料 JAXA-SP-(Web)  2017.3 

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    長期の宇宙天気活動に伴うスペースデブリ環境の推移予測

  • QZS(みちびき)初号機とMAGDASによる磁気圏FAC‐電離圏電流回路の同時観測に関する統計解析に向けて

    #安倍松侑太, @河野英昭, 東尾奈々, 越石英樹, 松本晴久, MOISEEV A. V, BAISHEV D. G, @魚住禎司, @阿部修司, @吉川顕正

    宇宙航空研究開発機構特別資料 JAXA-SP-(Web)  2018.1 

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    QZS(みちびき)初号機とMAGDASによる磁気圏FAC‐電離圏電流回路の同時観測に関する統計解析に向けて

  • 宇宙活動の長期的持続性のためのアジア・太平洋地域の連携

    花田 俊也, 吉川 顕正, 柳沢 俊史

    宇宙科学技術連合講演会講演集  2013.10 

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    Country:Japan  

    Asia-Pacific Regional Collaboration for Long-term Sustainability of Outer Space Activities

  • The relationship between the solar wind activity and Pc 3 magnetic pulsations at low latitudes (L~1.3)

    高崎聡子, 河野英昭, 田中良昌, 吉川顕正, 瀬戸雅弘, 飯島雅英, 湯元清文

    地球惑星関連学会2002年合同大会  2002.6 

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    Language:Others   Presentation type:Oral presentation (general)  

    Venue:国立オリンピックセンター 東京   Country:Japan  

  • Pi2型地磁気脈動と電離層電気伝導度の関係~高緯度南北共役点のデータ解析

    関悠子, 魚住禎司, 河野英昭, 吉川顕正, 湯元清文, 大谷晋一

    地球惑星関連学会2002年合同大会  2002.6 

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    Venue:国立オリンピックセンター 東京   Country:Japan  

  • 動的スケール間結合としての磁気圏・電離圏結合物理の発展

    吉川顕正

    地球電磁気将来計画シンポジウム  2002.3 

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    Venue:国立極地研究所、東京   Country:Japan  

  • FM-CWレーダによる電離層ドップラーデータとCPMN地磁気データとの比較解析研究

    石原隆一, 森一浩, 吉川顕正, 野崎憲郎, 篠原学, 湯元清文

    地球惑星関連学会2002年合同大会  2002.6 

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    Venue:国立オリンピックセンター 東京   Country:Japan  

  • 赤道域での3次元伝導度分布を考慮した電離層Sq電流のシミュレーションについて

    湯元清文, 榎木田暁子, 吉川顕正

    地球惑星関連学会2002年合同大会  2002.6 

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    Venue:国立オリンピックセンター 東京   Country:Japan  

  • Bepi-Colombo による磁場観測の重要性と惑星科学への寄与

    松岡彩子, 渋谷秀俊, 湯元清文, 河野英昭, 吉川顕正, 篠原学, 藤井良一, 中川朋子

    地球惑星関連学会2002年合同大会  2002.6 

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    Venue:国立オリンピックセンター 東京   Country:Japan  

  • Bepi-Colombo MMO 搭載磁力計の検討

    松岡彩子, 渋谷秀俊, 湯元清文, 河野英昭, 吉川顕正, 篠原学, 藤井良一, 中川朋子

    地球惑星関連学会2002年合同大会  2002.6 

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    Venue:国立オリンピックセンター 東京   Country:Japan  

  • 磁気圏対流と電離圏対流結合に於ける局所性と大域性についての考察

    吉川顕正, 糸長雅弘, 湯元清文

    地球惑星関連学会2002年合同大会  2002.6 

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    Venue:国立オリンピックセンター 東京   Country:Japan  

  • 水星表面近傍における電流クロージャーについての考察

    吉川顕正, 河野英昭, 湯元清文

    地球惑星関連学会2002年合同大会  2002.6 

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    Venue:国立オリンピックセンター 東京   Country:Japan  

  • Global Network Observations of Electric and Magnetic Field Variations for Space Weather

    湯元清文, 河野英昭, 吉川顕正, 篠原学, 野崎憲郎, 環太平洋地磁気観測グループ

    地球惑星関連学会2002年合同大会  2002.6 

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    Venue:国立オリンピックセンター 東京   Country:Japan  

  • 地上多点観測磁場変動データを用いたPc 4脈動の研究

    尾花由紀, 吉川顕正, R. J. Morris, B. J. Fraser, J. V. Olson, 湯元清文

    第26回極域における電離圏磁気圏総合観測シンポジウム  2002.7 

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    Venue:国立極地研究所、東京   Country:Japan  

  • 磁気圏電離圏結合の過渡応答時に励起される発散性ホール電流と沿磁力線電流のクロージャーによる回転性ホール電流のジェネレータについて

    吉川顕正

    第26回極域における電離圏磁気圏総合観測シンポジウム  2002.7 

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    Venue:国立極地研究所、東京   Country:Japan  

  • 中低緯度におけるM-I coupling:地上ネットワーク磁場観測からのPartial-ring current分布予測可能性について

    吉川顕正, 公田浩子, 糸長雅弘, 湯元清文

    名古屋大学太陽地球観測所共同研究集会「プラズマ圏・内部磁気圏プラズマ過程に関する研究集会」  2002.8 

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    Venue:独立行政法人通信総合研究所、 国分寺市   Country:Japan  

  • Multi-ion plasma systemとしての水星磁気圏ダイナミクスの重要性 Invited

    吉川顕正

    宇宙プラズマ/太陽系環境研究の将来構想座談会  2002.8 

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    Venue:東京工業大学 東京   Country:Japan  

  • 米国内部磁気圏探査計画の紹介

    吉川顕正

    第2回プラズマ圏・内部磁気圏研究会  2002.8 

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    Venue:通信総合研究所 国分寺市   Country:Japan  

  • 環太平洋地磁気ネットワーク, 経度の異なるデータセットを用いた同時観測によるプラズマ圏診断

    阿部 修司, 湯元 清文, 河野 英昭, 吉川 顕正, 尾花 由紀, Stepan I. Solovyev, Dmity G. Baishev, John V. Olson, Bill Worthington

    第112回地球電磁気・地球惑星圏学会  2002.11 

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    Venue:電気通信大学   Country:Japan  

  • Small Bayに伴うPi2型地磁気脈動の振幅の緯度依存性に関する研究

    関 悠子, 山口 類, 魚住 貞司, 河野 英昭, 吉川 顕正, 湯元 清文, 大谷 晋一

    第112回地球電磁気・地球惑星圏学会  2002.11 

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    Venue:電気通信大学   Country:Japan  

  • 準振動的カレントウェッジの形成に及ぼす電離層ホール効果とPi2振動

    糸長雅弘, 吉川顕正, 藤田茂

    第112回地球電磁気・地球惑星圏学会  2002.11 

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    Venue:電気通信大学   Country:Japan  

  • FM-CWレーダによるDP2変動と電離層電場変動の特性について

    森一浩, 石原隆一, 吉川顕正, 野崎憲郎, 湯元清文

    第112回地球電磁気・地球惑星圏学会  2002.11 

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    Venue:電気通信大学   Country:Japan  

  • L-2.8~5.9の多点磁場観測網で観測された磁力線振動現象の高次共鳴モードの解析

    尾花由紀, 吉川顕正, R.J.Morris, B.J. Fraser, J.V. Olson, S.I. Dolovyev, 湯元清文

    第112回地球電磁気・地球惑星圏学会  2002.11 

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    Venue:電気通信大学   Country:Japan  

  • Investigation of the plasma density in the Earth's plasmasphere at low latitudes (L~1.3) by using ground-based observations

    Satoko Takasaki, Hideaki Kawano, Yoshimasa Tanaka, Akimasa Yoshikawa, Masahiro Seto, Masahide Iijima, and Kiyohumi Yumoto .

    第112回地球電磁気・地球惑星圏学会  2002.11 

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    Venue:電気通信大学   Country:Japan  

  • Development of computer simulation code for global ionospheric current system

    Sano, T., Y. Ohnishi, A. Yoshikawa, K. Yumoto

    第112回地球電磁気・地球惑星圏学会  2002.11 

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    Venue:電気通信大学   Country:Japan  

  • Ground magnetic variations at wide range of local times during the saw-tooth event on 17-18 April

    Kentarou Kitamura, Hideaki Kawano, Shin-ichi Ohtani, Akimasa Yoshikawa, Kiyohumi Yumoto, Circum-pan Pacific Magnetometer Network Group

    第112回地球電磁気・地球惑星圏学会  2002.11 

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    Venue:電気通信大学   Country:Japan  

  • Role of field-aligned current closure via the Pedersen, Hall, and atmospheric current in the formation of ionospheric current system International conference

    Yoshikawa A., K. Yumoto, Y. Song, R.L. Lysak

    AGU 2002 Fall Meeting  2002.12 

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    Venue:Moscone Center, San Francisco   Country:United States  

  • olar Wind Activity Dependence of the Occurrence of Field-Line Resonance at low Latitudes (L~1.3) International conference

    S. Takasaki, H. Kawano, Y. Tanaka, A. Yoshikawa, M. Seto, M. Iijima, and K. Yumoto

    AGU 2002 Fall Meeting  2002.12 

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    Venue:Moscone Center, San Francisco   Country:United States  

  • Local-time Distribution of Low-latitute Ground Magnetic Disturbances at Sawtooth Injections of April 18-19, 2002 International conference

    K. Kitamura, H. Kawano, S. Ohtani, A. Yoshikawa, K. Yumoto, and CPMN Group

    AGU 2002 Fall Meeting  2002.12 

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    Venue:Moscone Center, San Francisco   Country:United States  

  • 小型衛星による内部磁気圏探査計画: 科学的意義と検討状況について Invited

    関 華奈子, 塩川 和夫, 三好 由純, 小野 高幸, 長妻 努, 小原 隆博, 能勢 正仁, 笠原 禎也, 平原 聖文, 高島 健, 浅村 和史, 笠羽 康正, 松岡 彩子, 齋藤 義文, 齋藤 宏文, 湯元 清文, 河野 英昭, 吉川

    宇宙天気シンポジウム  2003.2 

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    Venue:ホテル日航豊橋   Country:Japan  

  • 高緯度沿磁力線電流と中低緯度中性大気風ダイナモを考慮した全球電離層電流モデリング

    佐野隆行, 吉川顕正, 湯元清文

    第3回 CAWSES 電磁圏シンポジウム  2003.2 

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    Venue:九州大学国際研究交流プラザ   Country:Japan  

  • 小規模サブストームに伴うPi2型地磁気脈動の緯度依存性

    関 悠子, 山口 類, 魚住 禎司, 河野 英昭, 吉川 顕正, 湯元 清文, 大谷 晋一

    2003.3 

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    Venue:九州大学国際研究交流プラザ   Country:Japan  

  • 磁気嵐時における低緯度領域(L~1.3)プラズマ密度分布の変動について

    高崎 聡子, 河野 英昭, 田中 良昌, 吉川 顕正, 瀬戸 正弘, 飯島 雅英, 湯元 清文

    第3回 CAWSES 電磁圏シンポジウム  2003.3 

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    Venue:九州大学国際研究交流プラザ   Country:Japan  

  • 短波帯FM-CWレーダーシステム構築による新しい電離層観測手法の開発研究

    石原隆一, 吉川顕正, 湯元清文

    第3回 CAWSES 電磁圏シンポジウム  2003.3 

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    Venue:九州大学国際研究交流プラザ   Country:Japan  

  • 地上多点磁場観測データからの磁気圏−電離圏−固体地球電磁結合系情報分離の可能性についてII

    尾花 由紀, 吉川顕正, 湯元清文

    第3回 CAWSES 電磁圏シンポジウム  2003.3 

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    Venue:九州大学国際研究交流プラザ   Country:Japan  

  • 地上磁場データからの沿磁力線電流寄与成分と電離層電流寄与成分の分離アルゴリズムについて

    吉川顕正

    第3回 CAWSES 電磁圏シンポジウム  2003.3 

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    Venue:九州大学国際研究交流プラザ   Country:Japan  

  • 2002年4月18日発生の Sawtooth event における Positive Bay と Pi2 の時間空間依存性

    北村 健太郎, 河野 英昭, 大谷 晋一, 吉川 顕正, 湯元 清文

    第3回 CAWSES 電磁圏シンポジウム  2003.3 

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    Venue:九州大学国際研究交流プラザ   Country:Japan  

  • Variation of the plasma density distribution in low-L (L-1.3) region during magnetic storms

    高崎聡子, 河野 英昭, 田中 良昌, 吉川 顕正, 瀬戸 正弘, 飯島 雅英, 湯元 清文

    地球惑星関連学会2003年合同大会  2003.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • Plasmapause detection by analysis of high-latitude ground magnetometer data at multiple local times

    阿部 修司, 湯元 清文, 河野 英昭, 吉川 顕正, 尾花 由紀, 環太平洋地磁気観測グループ

    地球惑星関連学会2003年合同大会  2003.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • インバージョン法を用いたPc 3-5振幅の解析

    尾花 由紀, 吉川顕正, 湯元清文, 還太平洋地磁気観測グループ

    地球惑星関連学会2003年合同大会  2003.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • 電離層電流の全球モデリング −磁場変動の磁気圏電離圏結合

    吉川 顕正, 大西 祥人, 糸長 雅弘, 湯元 清文

    地球惑星関連学会2003年合同大会  2003.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • Ground Magnetic Variations at Low and Middle Latitude of the Sawtooth Event on April 18, 2002

    北村 健太郎, 河野 英昭, 大谷 晋一, 吉川 顕正, 湯元 清文, 環太平洋地磁気観測グループ

    地球惑星関連学会2003年合同大会  2003.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • 短波帯FM-CWレーダーシステム構築による新しい電離層観測手法の開発

    吉川顕正, 新原俊樹, 湯元清文

    九州大学森林生態圏管理学講座/演習林研究発表会  2003.7 

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    Venue:九州大学演習林セミナーハウス   Country:Japan  

  • 国内地上磁場観測チェーンの構築:内部プラズマ圏密度診断に向けて

    河野英昭, 吉川顕正, 田中良昌, 高崎聡子, 瀬戸正弘, 飯島雅英, 岡野章一 茂木 透, 魚住禎司, 北村健太郎, 湯元清文, 九大グループ

    第114回地球電磁気・地球惑星圏学会  2003.8 

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    Venue:富山大学   Country:Japan  

  • 高緯度Pc 4 地磁気脈動振幅の統計解析

    尾花由紀, 吉川顕正, 湯元清文, CPMN 観測グループ

    第114回地球電磁気・地球惑星圏学会  2003.8 

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    Venue:富山大学   Country:Japan  

  • 赤道域電離圏3次元構造の汎世界電離層電流系における役割

    糸長雅弘, 吉川顕正, 公田浩子, 大西祥人, 湯元清文, 藤田 茂

    第114回地球電磁気・地球惑星圏学会  2003.10 

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    Venue:富山大学   Country:Japan  

  • 全球的電離層電流系の数値計算モデルの構築

    大西祥人, 吉川顕正, 湯元清文

    第114回地球電磁気・地球惑星圏学会  2003.10 

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    Venue:富山大学   Country:Japan  

  • 中低緯度領域に於ける地上磁場擾乱の要因分離アルゴリズムについて

    吉川顕正, 公田浩子, 魚住禎司, 糸長雅弘, 湯元清文

    第114回地球電磁気・地球惑星圏学会  2003.10 

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    Venue:富山大学   Country:Japan  

  • FM-CW レーダーとCPMN 地上磁場観測を組み合わせたDP 2 変動相関解析について

    中村康弘, 新原俊樹, 田中良昌, 吉川顕正, 河野英昭, 福田 喬, 湯元清文, CPMN 観測グループ

    第114回地球電磁気・地球惑星圏学会  2003.10 

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    Venue:富山大学   Country:Japan  

  • MAGnetic Data Acquisition System (MAGDAS) for Realtime Monitoring of Geospace Environment ~Part 2 : Data Acquisition and Monitoring System

    entarou Kitamura, Teiji Uozumi, Yoshimasa Tanaka, Akimasa Yoshikawa, Hideaki Kawano, Masaaki Hatsuta, Masataka Toma, Daisuke Arai, Kiyohumi Yumoto

    第114回地球電磁気・地球惑星圏学会  2003.10 

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    Venue:富山大学   Country:Japan  

  • MAGnetic Data Acquisition System (MAGDAS) for Realtime Monitoring of Geospace Environment Part 1 : CPMN Magnetometer System

    Teiji Uozumi, Kentarou Kitamura, Yoshimasa Tanaka, Akimasa Yoshikawa, Hideaki Kawano, T.Omoto, S.Takehisa, M.Tada, Y.Terakado, Y.Onozawa, Kiyohumi Yumoto

    第114回地球電磁気・地球惑星圏学会  2003.10 

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    Venue:富山大学   Country:Japan  

  • Quasi-periodic Substorms during Recovery Phase of Magnetic Storm for Space Weather Study International conference

    Kitamura. K., H. Kawano, S. Ohtani, A. Yoshikawa, K. Yumoto, and the Circum-pan Pacific Magnetometer Network Group

    ACROS Fukuoka, Fukuoka  2003.11 

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    Venue:International Symposium on Information Science and Electrical Engineering 2003   Country:Japan  

  • The Diagnosis of the Plasmapause by Ground Magnetometer Network Observation at Multiple Local Times International conference

    Abe S., K. Yumoto, H. Kawano, A. Yoshikawa, Y. Obana, S. I. Solovyev, D.G. Baishev, J.V. Olson, E.W. Worthington, and the Circum-pan Pacific Magnetometer Network Group

    Information Science and Electrical Engineering 2003  2003.11 

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    Venue:ACROS Fukuoka, Fukuoka   Country:Japan  

  • Inegrated Analysis of Coordinated Ground Magnetic Field Data for Space Weather Study International conference

    Yoshikawa A., H. Kohta, M.I tonaga, T. Uozumi, K. Yumoto

    International Symposium on Information Science and Electrical Engineering 2003  2003.11 

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    Venue:ACROS Fukuoka, Fukuoka   Country:Japan  

  • Plasma Distribution in the Low-L part of the Plasma sphere during Magnetic Storms International conference

    Takasaki S., H. Kawano, Y. Tanaka, A. Yoshikawa, M. Seto, M. Iizima, and K. Yumoto

    International Symposium on Information Science and Electrical Engineering 2003  2003.11 

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    Venue:ACROS Fukuoka, Fukuoka   Country:Japan  

  • Environment Factors of PC 4 Amplitudes Observed at the CPMN Stations International conference

    Obana Y., A. Yoshikawa, J.V. Olson, R.J. Morris, B.J. Fraser, S.I. Solovyev and K. Yumoto

    International Symposium on Information Science and Electrical Engineering 2003  2003.11 

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    Venue:ACROS Fukuoka, Fukuoka   Country:Japan  

  • 地上多点磁場観測と海底ケーブルを組み合わせた、宙空電磁環境のモニタリング・モデリングの可能性について

    吉川顕正, 湯元清文

    海底ケーブルの科学的利用に関するワークショップ  2003.11 

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    Venue:海洋科学技術センター 東京連絡所   Country:Japan  

  • Evaluation of the inverse dynamic model in cerebellum during visual-vestibular interactions at different VOR gains in squirrel monkeys

    Yutaka Hirata, Akimasa Yoshikawa, Pablo M. Blazquez, Stephen M. Highstein

    Neurocomputing  2005.6 

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    Country:Japan  

    Evaluation of the inverse dynamic model in cerebellum during visual-vestibular interactions at different VOR gains in squirrel monkeys
    Generality of the cerebellar inverse dynamic model (IDM) theory was evaluated in oculomotor control in squirrel monkeys. Flocculus Purkinje cell firing patterns recorded during visual, vestibular, and their interaction paradigms at various vestibuloocular reflex (VOR) gains were reconstructed by the IDM consisting of the linear combination of eye position, velocity, and acceleration. The IDM could successfully reconstruct more than 72&#37; of the firing patterns of 138 cells, but with different sets of parameters for different paradigms and different VOR gains. This result suggests that the output of the flocculus relates to motor output, but not the motor command per se. © 2004 Elsevier B.V. All rights reserved.

  • グローバルな地上観測に基づく巨大磁気嵐時の長周期地磁気脈動の変動特性

    藤本晶子, 吉川顕正, 篠原学, 魚住禎司, 尾花由紀, 湯元清文, 環太平洋地磁気観測グループ

    地球惑星科学関連学会合同大会  2006.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • 、M-CW HFレーダーによって観測された低緯度電離圏電場のDP2型変化

    篠原 学, 野崎 憲朗, 吉川 顕正, Shevtsov Boris M., 湯元 清文

    地球惑星科学関連学会合同大会  2006.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • SC時の低緯度侵入電場と地上磁場変動や太陽風パラメーターとの関連性

    池田 昭大, 篠原 学, 吉川 顕正, 野崎 憲朗, 湯元 清文

    地球惑星科学関連学会合同大会  2006.5 

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    Venue:幕張メッセ国際会議場   Country:Japan  

  • Global Pc 5 Pulsations During an Interval of Northward IMF and High-speed Solar Wind on 31 October 2003 International conference

    Yuki Obana, K. Yumoto, A. Yoshikawa, M. Shinohara, H. Kawano, D. G. Baishev, S. I. Solovyev, and Circum-pan Pacific Magnetometer Network Group

    Western Pacific Geophysics Meeting, Bijing, China, July 24-27, 2006  2006.6 

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    Venue:Bijing, China   Country:China  

  • FM-CWレーダーによるSC時の低緯度電離層侵入電場観測

    池田昭大, 篠原学, 吉川顕正, 野崎憲朗, 湯元清文

    第30回極域宙空圏シンポジウム  2006.8 

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    Venue:国立極地研究所   Country:Japan  

  • Wave Characteristics of High-latitude Pi2 Pulsation Extracted by ICA (Independent Component Analysis),

    T. Tokunaga, H. Kohta, A. Yoshikawa, T. Uozumi, H. Kawano, K. Yumoto

    第30回極域宙空圏シンポジウム  2006.8 

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    Venue:国立極地研究所   Country:Japan  

  • Installation Plan in Antarctica

    H. Kohta, T. Uozumi, S. Abe, A. Yoshikawa, K. Yumoto and the MAGDAS/CPMN Group, MAGDAS

    第30回極域宙空圏シンポジウム  2006.8 

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    Venue:国立極地研究所   Country:Japan  

  • Comparison between high-latitude Pi 2 pulsations extracted by ICA and AKR spectrum

    T. Tokunaga, A. Morioka, H. Kohta, A. Yoshikawa, T. Uozumi, K. Yumoto, and MAGDAS/CPMN Group

    Space Science Seminor  2006.11 

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    Venue:北海道大学   Country:Japan  

  • Comparison of the ionospheric electric field and the geomagnetic field at the time of SC

    A.Ikeda, M.Shinohara, A.Yoshikawa, K.Nozaki, K.Yumoto

    Space Science Seminor  2006.11 

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    Venue:北海道大学   Country:Japan  

  • 低緯度FM-CW HFレーダーによって観測されたPc4帯の電離圏電場変動

    篠原 学, 野崎憲朗, 吉川顕正, 湯元清文, 環太平洋地磁気観測グループ

    地球電磁気・地球惑星圏学会第120回講演会  2006.11 

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    Venue:相模原産業会   Country:Japan  

  • SC時の低緯度侵入電場と地上磁場変動の比較解析

    池田 昭大, 篠原 学, 吉川 顕正, 野崎 憲朗, 湯元 清文

    地球電磁気・地球惑星圏学会第120回講演会  2006.11 

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    Venue:相模原産業会   Country:Japan  

  • 独立成分分析によって抽出された高緯度Pi 2とAKRの比較

    徳永旭将, 森岡昭, 公田浩子, 吉川顕正, 魚住禎司, 湯元清文, MAGDAS/CPMNグループ

    地球電磁気・地球惑星圏学会第120回講演会  2006.11 

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    Venue:相模原産業会   Country:Japan  

  • ERG衛星に関連した地上観測ネットワーク

    塩川和夫, 西谷望, 菊池崇, 大塚雄一, 藤井良一, 湯元清文, 河野英昭, 吉川顕正, 佐藤夏雄, 行松彰, 山岸久雄, 門倉昭, 田口真, 小川泰信, 細川敬祐, 橋本久美子, ERGプロジェクトチー

    地球電磁気・地球惑星圏学会第120回講演会  2006.11 

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    Venue:相模原産業会   Country:Japan  

  • FM-CW Radar Observation of the Electric Fields Penetrating into the Low Latitude Ionosphere at the Time of SC International conference

    Ikeda A., Shinohara M., Yoshikawa A., Nozaki K., Yumoto K.

    AGU Fall Meeting  2006.12 

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    Venue:San Francisco   Country:United States  

  • FM-CWレーダーによるDP2型電離圏電場変動の観測

    篠原学, 池田昭大, 野崎憲朗, 吉川顕正, Bychkov Vasily V., Shevtsov Boris M., 亘慎一, 北村健太郎, 湯元清文, MAGDAS/CPMN グループ

    日本地球惑星科学連合大会  2007.5 

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    Venue:幕張メッセ, 千葉   Country:Japan  

  • ERG 計画における地上ネットワーク観測

    塩川和夫, 西谷望, 菊池崇, 大塚雄一, 藤井良一, 湯元清文, 河野英昭, 吉川顕正, 佐藤夏雄, 行松彰, 山岸久雄, 門倉昭, 田口真, 小川泰信, 細川敬祐, 橋本久美子

    日本地球惑星科学連合大会  2007.5 

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    Venue:幕張メッセ, 千葉   Country:Japan  

  • 地上磁場点観測データから得られたSq等価渦電流構造の解析

    公田浩子, 吉川顕正, 魚住禎司, 湯元清文, CPMN/MAGDASグループ

    日本地球惑星科学連合大会  2007.5 

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    Venue:幕張メッセ, 千葉   Country:Japan  

  • Pi2 Magnetic and Electric Pulsations at Low Latitude: FM-CW Radar Observations

    池田昭大, 湯元清文, 篠原学, 野崎憲朗, 吉川 顕正, 魚住禎司, 徳永旭将, 平山有紀

    第31回極域宙空圏シンポジウム  2007.7 

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    Venue:国立極地研究所、東京   Country:Japan  

  • Cluster-MAGDAS/CPMN conjunction study of Pi2 wave characteristics in the inner magnetosphere

    河野英昭, 大谷晋一, 魚住禎司, 徳永旭将, 公田浩子, 吉川顕正, 阿部修司, 北村健太郎, 田中良昌, 湯元清文, Lucek Elizabeth A

    第122回地球電磁気・地球惑星圏学会  2007.9 

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    Venue:名古屋大学野依記念学術交流館   Country:Japan  

  • Characteristics of Pi2 Electric Pulsations at Low-Latitude Ionosphere: FM-CW Radar Observations

    池田昭大, 湯元清文, 篠原学, 野崎憲朗, 吉川 顕正, 魚住禎司, 徳永旭将, 平山有紀

    第122回地球電磁気・地球惑星圏学会  2007.9 

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    Venue:名古屋大学野依記念学術交流館   Country:Japan  

  • 地上観測されたPi2型地磁気脈動の相互情報量に基づく分類

    徳永旭将, 吉川顕正, 魚住禎司, 湯元清文, 環太平洋地磁気観測グループ

    第122回地球電磁気・地球惑星圏学会  2007.9 

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    Venue:名古屋大学野依記念学術交流館   Country:Japan  

  • Sc-associated Ionospheric Electric Fields at Low Latitude: FM-CW Radar Observation International conference

    Ikeda A., K.Yumoto, M.Shinohara, A.Yoshikawa, K.Nozaki, A.Shinbori

    International CAWSES Symposium  2007.10 

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    Venue:Kyoto University   Country:Japan  

  • Mutual Information based clustering of Pi 2 magnetic pulsations observed at CPMN stations International conference

    Tokunaga T., A. Yoshikawa, T. Uozumi, K. Yumoto and CPMN Group

    AGU Fall Meeting 2007  2007.12 

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    Venue:San Francisco, USA   Country:United States  

  • Mutual Information based clustering of Pi 2 magnetic pulsations observed at CPMN stations International conference

    Ikeda A., K.Yumoto, M, Shinohara, K.Nozaki, A.Yoshikawa, T.Uozumi, T.Tokunaga, Y.Hirayama

    AGU Fall Meeting 2007  2007.12 

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    Venue:San Francisco, USA   Country:United States  

  • 変化点検出を応用した時系列データからの突発現象の前兆検出アルゴリズム

    徳永 旭将, 池田 大輔, 中村 和幸, 樋口 知之, 吉川 顕正, 魚住 禎司, 藤本 晶子, 森岡 昭, 湯元 清文, CpmnGroup

    研究報告数理モデル化と問題解決(MPS)  2010.12 

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    Country:Japan  

    一般に,前兆現象は突発現象にそのものに比べて非常に目立ちにくく,その開始時刻は曖昧である.従来よく用いられてきた変化点検出法を適用した場合,このような微小で緩慢な変化は見逃されやすい.Tokunaga et al.1) では,Ide and Inoue2) の提案した特異スペクトル分析を応用した変化点検出法 (SST) を,多次元データを用いたアルゴリズム (MSST) へと拡張することで,鋭敏に前兆現象の開始時刻を推定出来ることを示した.MSST は,緩慢な変化も検出できる鋭敏な手法であるが,実データへの適用では誤検出が問題になる.本稿では,突発現象の大まかな開始時刻を予め検出し,さらに検出された時刻の前後で前兆現象の開始時刻と終了時刻を個別に探索することで,誤検出を劇的に減少させることができることを示す.

  • 変化点検出を応用した時系列データからの突発現象の前兆検出アルゴリズム

    徳永 旭将, 池田 大輔, 中村 和幸, 樋口 知之, 吉川 顕正, 魚住 禎司, 藤本 晶子, 森岡 昭, 湯元清文, CpmnGroup

    研究報告バイオ情報学(BIO)  2010.12 

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    Country:Japan  

    一般に,前兆現象は突発現象にそのものに比べて非常に目立ちにくく,その開始時刻は曖昧である.従来よく用いられてきた変化点検出法を適用した場合,このような微小で緩慢な変化は見逃されやすい.Tokunaga et al.1) では,Ide and Inoue2) の提案した特異スペクトル分析を応用した変化点検出法 (SST) を,多次元データを用いたアルゴリズム (MSST) へと拡張することで,鋭敏に前兆現象の開始時刻を推定出来ることを示した.MSST は,緩慢な変化も検出できる鋭敏な手法であるが,実データへの適用では誤検出が問題になる.本稿では,突発現象の大まかな開始時刻を予め検出し,さらに検出された時刻の前後で前兆現象の開始時刻と終了時刻を個別に探索することで,誤検出を劇的に減少させることができることを示す.

  • 沿磁力線電流を通じた磁気圏−電離圏結合系における階層間結合

    吉川顕正

    CAWSES 電磁圏シンポジウム ─沿磁力線電流から複合系へ  2002.3 

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    Venue:九州大学国際研究交流プラザ   Country:Japan  

  • Transient response of the non-uniform equatorial ionosphere to the ionospheric current of polar region

    糸長雅弘, 吉川顕正, 湯元清文

    地球惑星科学関連学会1998合同大会  1998.5 

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    Venue:東京、代々木オリンピックセンター   Country:Japan  

  • On evaporation and precipitation of energic particles by the parametric Hall coupling between shear Alfv?n and fast magnetosonic mode

    吉川顕正, 坂翁介, 菊池祟

    地球惑星科学関連学会1998合同大会  1998.5 

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    Venue:代々木オリンピックセンター   Country:Japan  

  • 磁気圏固有振動による地上磁場擾乱の電離層伝導度依存性

    中田裕行, 藤田茂, 糸長雅弘, 吉川顕正

    地球惑星科学関連学会1998合同大会  1998.5 

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    Venue:東京、代々木オリンピックセンター   Country:Japan  

  • Transient Response of the Non-Uniform Equatorial Ionosphere to the Ionospheric Current of Polar Origin International conference

    Itonaga, M., A. Yoshikawa, K. Yumoto, and S. Fujita

    1998.7 

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    Venue:Taipei   Country:Taiwan, Province of China  

  • Studies on the Ionospheric Divergent Hall Current International conference

    Yoshikawa, A., and K.Yumoto

    32 th COSPAR meeting  1998.7 

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    Venue:Nagoya   Country:Japan  

  • Wave characteristics of daytime and nighttime Pi 2 pulsations at the equatorial and low latitudes (vol 24, pg 2279, 1997)

    M Shinohara, K Yumoto, A Yoshikawa, O Saka, SI Solovyev, EF Vershinin, NB Trivedi, JM Da Costa

    GEOPHYSICAL RESEARCH LETTERS  1998.9 

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    Country:Japan  

  • 磁力線振動と電離層相互作用 -レビュー Invited

    吉川顕正

    名古屋大学太陽地球環境研究所、海外観測シンポジウム  1998.10 

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    Venue:豊川   Country:Japan  

  • ULF波動に付随する電離層電流分布について

    吉川顕正

    名古屋大学太陽地球環境研究所、海外観測シンポジウム  1998.10 

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    Venue:豊川   Country:Japan  

  • 日の出付近での低緯度Pc3の波動特性

    田中良昌, 湯元清文, 吉川顕正, 北村泰一

    第104回地球電磁気、地球惑星圏学会講演会  1998.10 

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    Venue:茨城県青少年会館   Country:Japan  

  • 定在磁力線振動の研究

    中田裕行, 藤田茂, 糸長雅弘, 吉川顕正

    名古屋大学太陽地球環境研究所、ULF波動研究集会  1999.2 

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    Venue:豊川   Country:Japan  

  • 近接場と結合した磁力線振動の分散関係について

    吉川顕正

    地球惑星科学関連学会1999合同大会  1999.6 

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    Venue:東京、代々木オリンピックセンター   Country:Japan  

  • ULF Waves and Ionosphere: Multi-step mode conversion between divergent and rotational electric field by the ionospheric Hall effect International conference

    Yoshikawa, A., and K. Yumoto

    IUGG 1999  1999.7 

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    Venue:Birmingham   Country:United Kingdom  

  • Sunrise effect on very low-latitude Pc3 pulsations International conference

    Tanaka Y.M., A. Yoshikawa and K. Yumoto

    IUGG 1999  1999.7 

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    Venue:Birmingham   Country:United Kingdom  

  • ULF Waves and the inductive ionosphere Invited International conference

    IUGG 1999  1999.7 

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    Venue:Birmingham   Country:United Kingdom  

  • 地上磁場観測と多点人工衛星の共同観測

    吉川顕正, 河野英之, 篠原学, 湯元清文

    磁気圏・電離圏シンポジウム  1999.10 

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    Venue:宇宙科学研究所   Country:Japan  

  • 非結合磁力線振動について

    糸長雅弘, 吉川顕正, 藤田 茂

    第105回地球電磁気・地球惑星圏学会講演会  1999.11 

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    Venue:仙台市民会館   Country:Japan  

  • 日の出における電離層電気伝導度非一様性の低緯度ULF波動への影響

    田中良昌, 湯元清文, 吉川顕正, 北村泰一, CPMNグループ

    第105回地球電磁気・地球惑星圏学会講演会  1999.11 

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    Venue:仙台市民会館   Country:Japan  

  • ULF波動と電離層相互作用における電離層薄層近似の妥当性について

    渡辺敬之, 吉川顕正, 湯元清文

    第105回地球電磁気・地球惑星圏学会講演会  1999.11 

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    Venue:仙台市民会館   Country:Japan  

  • 高緯度磁気共役点におけるULF波動振幅の日変化・季節変化及び周波数依存性について

    尾花由紀, 吉川顕正, 湯元清文, J.V. Olson, R.J. Morris

    第105回地球電磁気・地球惑星圏学会講演会  1999.11 

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    Venue:仙台市民会館   Country:Japan  

  • 電離層へ斜め入射した沿磁力線電流による沿磁力線電場の励起機構について

    吉川顕正, 糸長雅弘, 湯元清文, 飯島 健

    第105回地球電磁気・地球惑星圏学会講演会  1999.11 

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    Venue:仙台市民会館   Country:Japan  

  • Formation of pumping mirror region just above the ionosphere by the ionospheric Hall effect for incident shear Alfv?n wave Invited International conference

    Yoshikawa A., K. Yumoto, and T. Iijima

    AGU Fall meeting  1999.12 

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    Venue:S.F.O.   Country:United States  

  • 磁気共役点におけるPc3-5pulsationの比較研究

    尾花由紀, 吉川顕正, 湯元清文, J. V. Olson, R.J. Morris

    STE研究連絡・STP観測ネットワークの合同シンポジウム  2000.2 

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    Language:Others   Presentation type:Oral presentation (general)  

    Venue:九州大学理学部   Country:Japan  

  • 磁気圏-電離圏結合系エネルギー収支における電離層ホール効果の役割:極域オーロラジェット電流は、ジュール散逸するのか?

    吉川顕正, 藤井良一

    STE研究連絡・STP観測ネットワークの合同シンポジウム  2000.2 

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    Venue:九州大学理学部   Country:Japan  

  • グローバル地上磁場観測によるプラズマ圏の振動の推定

    田中良昌, 湯元清文, 吉川顕正, 北村泰一, 210度MMグループ

    STE研究集会  2000.2 

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    Venue:京都大学理学部   Country:Japan  

  • 極域電場の水平伝播と赤道電離層による誘導効果

    糸長雅弘, 藤田 茂, 吉川顕正, 中田裕行

    STE研究集会  2000.3 

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    Venue:京都大学理学部   Country:Japan  

  • 地上磁気共役点観測データを用いたM-I coupling過程の検証

    尾花由紀, 吉川顕正, 湯元清文, 立原祐司

    STE研究集会  2000.3 

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    Venue:京都大学理学部   Country:Japan  

  • 沿磁力線電流による磁気圏、電離圏ダイナモの結合:誘導結合と準静的結合

    吉川顕正, 飯島健, 湯元清文

    STE研究集会  2000.3 

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    Venue:京都大学理学部   Country:Japan  

  • 非一様場でのアルベーン波の保存則とその応用

    吉川顕正, 糸長雅弘

    STE研究集会  2000.3 

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    Venue:京都大学理学部   Country:Japan  

  • 磁力線定在振動に伴う地上磁場擾乱の南北非対称性について(現実的パラメータを用いた場合)

    中田裕行, 藤田茂, 吉川顕正, 糸長雅弘

    STE研究集会  2000.3 

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    Venue:京都大学理学部   Country:Japan  

  • L~1.3におけるH成分比法と位相差法による地磁気脈動共鳴構造の解明

    高崎聡子, 河野英昭, 吉川顕正, 魚住禎司, 田中良昌, 尾花由紀, 北村保夫, 瀬戸雅弘, 森岡 昭, 飯島雅英, 大矢 克, 大谷晋一, 湯元清文

    地球惑星科学関連学会2000年合同大会  2000.6 

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    Venue:代々木オリンピックセンター   Country:Japan  

  • 地上磁気変動データを用いたULF周波数の変動について / Variations of ULF frequency observed at ground based stations

    尾花 由紀, 吉川顕正, 高崎 聡子, 河野 英昭, 湯元 清文

    地球惑星科学関連学会2000年合同大会  2000.6 

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    Venue:代々木オリンピックセンター   Country:Japan  

  • 磁気圏電離圏結合でのエネルギー収支におけるホール効果の役割について

    吉川顕正, 藤井良一, 飯島健, 糸長雅弘, 湯元清文 吉川顕正, 藤井良一, 飯島健, 糸長雅弘, 湯元清文

    地球惑星科学関連学会2000年合同大会  2000.6 

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    Venue:代々木オリンピックセンター, 東京   Country:Japan  

  • The computer simulation on the validity of ionospheric thin sheet approximation in the reflection process of ULF waves at the high latitudinal inductive ionosphere

    Watanabe, M., A.Yoshikawa, and K.Yumoto

    地球惑星科学関連学会2000年合同大会  2000.6 

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    Venue:代々木オリンピックセンター   Country:Japan  

  • 地上多点同時観測によるPi 2の磁気圏内の3次元的伝播特性

    魚住禎司, 湯元清文, 吉川顕正, J. V. Olson, 赤祖父俊一, S. I. Solovyev, E. F. Vershinin, K. Liou, C.-I. Meng

    第24回極域に於ける磁気圏電離圏観測シンポジウム  2000.8 

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    Venue:国立極地研究所 東京   Country:Japan  

  • 電離層ホール電流はFACエネルギーを消費するのか?

    吉川顕正

    第24回極域に於ける磁気圏電離圏観測シンポジウム  2000.8 

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    Venue:国立極地研究所、東京   Country:Japan  

  • 地上磁気共役点観測データを用いたULF power の南北非対称性の定量的解析

    尾花由紀, 吉川顕正, 湯元清文, 塩川和夫, J.V.Olson, R.J.Morris

    第108回地球電磁気・地球惑星圏学会講演会  2000.11 

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    Venue:板橋区立文化会館   Country:Japan  

  • 磁気圏−電離圏結合系電磁擾乱エネルギー収支におけるホール効果の普遍的役割

    吉川顕正

    第108回地球電磁気・地球惑星圏学会講演会  2000.11 

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    Venue:板橋区立文化会館   Country:Japan  

  • 非一様複合系物理学としての磁気圏・電離圏結合系物理学の発展

    吉川顕正

    STE研将来計画シンポジウム  2000.11 

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    Venue:名古屋大学シンポジオン   Country:Japan  

  • Role of ionospheric Hall effect on the energy balance in the magnetosphere-ionosphere coupled system International conference

    Yoshikawa, A., R.Fujii, T.Iijima, M.Itonaga, and K.Yumoto

    First S-RAMP Conference  2000.12 

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    Venue:札幌   Country:Japan  

  • Effects on the ionospheric conditions on the pulsations observed on the geomagnetic conjugate pair stations International conference

    Obana, Y., A.Yoshikawa, K.Yumoto, J.V.Olson, R.J.Morris

    First S-RAMP Conference  2000.12 

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    Venue:札幌   Country:Japan  

  • 低高度人工衛星と地上電場・磁場多点ネットワーク観測を用いた磁気圏−電離圏結合の戦略的総合解析~電離圏対流及び電流の成長・変換・伝播・消滅素過程の解明に向けて~ Invited

    吉川顕正, 河野英昭, 湯元清文

    磁気圏−電離圏シンポジウム  2000.12 

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    Venue:宇宙科学研究所   Country:Japan  

  • 磁気圏対流−電離圏対流−電離層電流−地上磁場地場変動の結合過程

    吉川顕正, 河野英昭, 湯元清文

    比較サブストームシンポジウム  2001.2 

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    Venue:通信総合研究所、東京   Country:Japan  

  • Does the rotational Hall current absorb the field-aligned current energy? Invited International conference

    Yoshikawa, A

    JSPS Workshop in Korea  2001.3 

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    Venue:Soul   Country:Korea, Republic of  

  • Hall induced shielding effect on the geomagnetic pulsation International conference

    Yoshikawa, A

    MHD Workshop  2001.3 

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    Venue:Taipei   Country:Taiwan, Province of China  

  • Field-line resonance observed around L= 1.3 International conference

    Takasaki, S., H.Kawano, A.Yoshikawa, T.Uozumi, Y.Tanaka, Y.Obana, Y.Kitamura, M. Seto, M. Iizima, A.Morioka, and K.Yumoto

    MHD Workshop  2001.3 

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    Venue:Taipei   Country:Taiwan, Province of China  

  • 地上多点同時観測によるPi 2の磁気圏内の3次元的伝播特性

    魚住禎司, 吉川顕正, 湯元清文

    南極大陸無人多点観測に関する研究小集会  2001.3 

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    Venue:国立極地研究所、東京   Country:Japan  

  • L~1.3における地磁気脈動共鳴構造の解明−狭間隔(~50km)多点磁場観測点へのH成分比法と位相差法の応用−

    高崎聡子, 河野英昭, 吉川顕正, 魚住禎司, 田中良昌, 尾花由紀, 北村保夫, 瀬戸雅弘, 森岡 昭, 飯島雅英, 大矢 克, 大谷晋一, 湯元清文

    南極大陸無人多点観測に関する研究小集会  2001.3 

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    Venue:国立極地研究所、東京   Country:Japan  

  • 高緯度磁場変動データを用いたULF波動伝搬過程の検証

    尾花由紀, 吉川顕正, 湯元清文

    南極大陸無人多点観測に関する研究小集会  2001.3 

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    Venue:国立極地研究所、東京   Country:Japan  

  • 地上磁場多点観測により期待される成果・新しい物理

    吉川顕正

    南極大陸無人多点観測に関する研究小集会  2001.3 

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    Venue:国立極地研究所、東京   Country:Japan  

  • 南北磁気共役点で観測されるPc3-5の季節変化

    尾花由紀, 吉川顕正, 湯元清文, CPMN観測グループ

    STE・海外観測合同ワークショップ  2001.3 

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    Venue:九州大学   Country:Japan  

  • 磁気圏-電離圏系での MHD 波動とプラズマ対流

    吉川顕正

    STE・海外観測合同ワークショップ  2001.3 

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    Venue:九州大学   Country:Japan  

  • Investigation of field-line resonance structure by using the dual station H ratio technique and the phase gradient technique at L~1.3

    Takasaki, S., H.Kawano, A.Yoshikawa, T.Uozumi, Y.Tanaka, Y.Obana, Y.Kitamura, M.Seto, M.Iizima, A.Morioka, and K.Yumoto

    STE・海外観測合同ワークショップ  2001.3 

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    Venue:九州大学   Country:Japan  

  • Investigation of field-line resonance structure by using the dual station H ratio and the phase gradient techniques at L~1.3

    高崎聡子, 河野英昭, 吉川顕正, 湯元清文

    地球惑星関連学会2001年合同大会  2001.6 

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    Venue:国立代々木オリンピックセンター、東京   Country:Japan  

  • A Study of the characteristics of ULF waves observed at the geomagnetic conjugate

    尾花由紀, 吉川顕正, 湯元清文

    地球惑星関連学会2001年合同大会  2001.6 

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    Venue:国立代々木オリンピックセンター、東京   Country:Japan  

  • サブストームカレントウエッジモデルによるPi2脈動の数値シミュレーション

    地球惑星関連学会2001年合同大会

    地球惑星関連学会2001年合同大会  2001.6 

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    Venue:国立代々木オリンピックセンター、東京   Country:Japan  

  • 極域から磁気赤道域にかけての巨視的電流形成の素過程について

    吉川顕正

    地球惑星関連学会2001年合同大会  2001.6 

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    Venue:国立代々木オリンピックセンター、東京   Country:Japan  

  • 環太平洋地磁気ネットワークデータを用いたULF振幅のローカルタイム依存性の分離

    尾花由紀, 吉川顕正, 湯元清文, J.V. Olson, R.J. Morris, S.I. Solovyev, CPMN観測グループ

    第25回極域に於ける電離圏磁気圏総合観測シンポジウム  2001.7 

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    Venue:国立極地研究所、東京   Country:Japan  

  • 磁気圏−電離圏結合系の電磁誘導プロセス解明に向けて

    吉川顕正

    第25回極域に於ける電離圏磁気圏総合観測シンポジウム  2001.7 

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    Venue:国立極地研究所、東京   Country:Japan  

  • The dispersive behavior of field line oscillation in the horizontal direction produced by the inductive ionosphere International conference

    Yoshikawa, A, T. Watanabe, and K.Yumoto

    IAGA-IASPEI joint scientific assembly  2001.8 

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    Venue:Hamoi   Country:Viet Nam  

  • Generation mechanism of ionospheric Hall current system International conference

    Yoshikawa, A

    IAGA-IASPEI joint scientific assembly  2001.8 

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    Venue:Hanoi   Country:Viet Nam  

  • Role of the ionospheric Hall effect in the energy balance of magnetosphere-ionosphere coupling between MHD disturbances International conference

    Yoshikawa, A

    IAGA-IASPEI joint scientific assembly  2001.8 

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    Venue:Hanoi   Country:Japan  

  • Polarization characteristics of high-latitude PI 2’s as a function of the position to the auroral break up region International conference

    Uozumi, T., Yoshikawa, A., and K. Yumoto

    IAGA-IASPEI joint scientific assembly  2001.8 

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    Venue:Hanoi   Country:Viet Nam  

  • Quantitative analysis of the north-south asymmetry of PC 3-5 amplitudes International conference

    Obana, Y., Yoshikawa, A, and K. Yumoto

    IAGA-IASPEI joint scientific assembly  2001.8 

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    Venue:Hanoi   Country:Viet Nam  

  • 地球近傍(L~1.3)における磁力線共鳴現象の発生と太陽風活動度との関係

    高崎聡子, 河野英昭, 田中良昌, 吉川顕正, 瀬戸正弘, 飯島雅英, 湯元清文

    第110回地球電磁気・地球惑星圏学会  2001.11 

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    Venue:九州大学 福岡市   Country:Japan  

  • FM-CWレーダを用いた電離層電場観測装置の開発研究

    石原隆一, 森一浩, 吉川顕正

    第110回地球電磁気・地球惑星圏学会  2001.11 

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    Venue:九州大学 福岡市   Country:Japan  

  • 地上観測点間の時差を利用して抽出したULF振幅の地方時及び磁気地方時依存性について

    尾花由紀, 吉川顕正, 塩川和夫, R.J. Morris, J.A. Kennewell, B.J. Fraser, V.J. Olson, S.I. Solovyev, 湯元清文, CPMN観測グループ

    第110回地球電磁気・地球惑星圏学会  2001.11 

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    Venue:九州大学 福岡市   Country:Japan  

  • Excitation of a Hall current generator by FAC closure, via an divergent Hall current, during transient phase of M-I coupling

    Yoshikawa, A

    第110回地球電磁気・地球惑星圏学会  2001.11 

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    Venue:九州大学 福岡市   Country:Japan  

  • Correlations between high- and low-latitude Pi2’s as a function of the position relative to the auroral break up

    T.Uozumi, K. Yumoto, H. Kawano, A. Yoshikawa, S. Ohtani, J.v. Olson, S. Akasof, S.I. Solovyev, E.F. Vershinin, K. Liou, C.I. Meng.

    第110回地球電磁気・地球惑星圏学会  2001.11 

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    Venue:九州大学 福岡市   Country:Japan  

  • 衛星−地上観測を組み合わせたの磁気圏電離圏結合

    吉川顕正, 河野英昭, 湯元清文

    戦略的次期衛星ミッション検討シンポジウム  2002.2 

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    Venue:宇宙科学研究所 相模原市   Country:Japan  

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MISC

  • 3次元Cowlingチャンネルの理論

    Yoshikawa A., O. Amm, and R. Fujii

    2009.12

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  • 宇宙天気概況解析実験マニュアル

    Yoshikawa A., (pp.1-10), and A. Nakamizo (pp.11-20)

    2006.4

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  • 地上多点磁場観測と海底ケーブルを組み合わせた宙空電磁環境のモニタリング/モデリングの可能性について

    吉川顕正、河野英昭、公田浩子、高崎聡子、魚住禎司、北村健太郎、湯元清文

    4D地球・ 海洋・環境科学研究の幕開け-海底ケーブルの科学的利用による海洋観測の新時代-、月刊地球, VOL. 26, NO. 5, 307-314, 2004   2004.12

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    Language:Japanese   Publishing type:Article, review, commentary, editorial, etc. (scientific journal)  

  • Quantum Calculation of Classical Kinetic Equations: A Novel Approach for Numerical Analysis of 6D Boltzmann-Maxwell Equations in Collisionless Plasmas Using Quantum Computing

    Hayato Higuchi, Juan William Pedersen, Akimasa Yoshikawa

    2023.6

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    A novel quantum algorithm for solving the Boltzmann-Maxwell equations of the
    6D collisionless plasma is proposed. The equation describes the kinetic
    behavior of plasma particles in electromagnetic fields and is known for the
    classical first-principles equations in various domains, from space to
    laboratory plasmas. We have constructed a quantum algorithm for a future
    large-scale quantum computer to accelerate its costly computation. This
    algorithm consists mainly of two routines: the Boltzmann solver and the Maxwell
    solver. Quantum algorithms undertake these dual procedures, while classical
    algorithms facilitate their interplay. Each solver has a similar structure
    consisting of three steps: Encoding, Propagation, and Integration. We conducted
    a preliminary implementation of the quantum algorithm and performed a parallel
    validation against a comparable classical approach. IBM Qiskit was used to
    implement all quantum circuits.

    DOI: 10.22541/essoar.168748458.80915597/v1

    arXiv

    researchmap

    Other Link: http://arxiv.org/pdf/2306.05967v1

  • Search for geomagnetic variation of equatorial electrojet using string matching and its application

    西口稜真, 吉川顕正, 藤本晶子

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Scattered perpendicular flow speed in the dayside reconnection regions due to change in the IMF Bz direction

    橋本翼, 吉川顕正, 田中高史

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Mid- and low-latitude electric fields response to CW development during isolated substorms

    林萌英, 吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Multi-spacecraft observations of widespread solar proton transport in the heliosphere

    OBARA Takahiro, YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • 太陽フレア発生時のシューマン共鳴の特性

    池田昭大, 魚住禎司, 吉川顕正, 藤本晶子, 阿部修司

    大気電気学会誌(Web)   17 ( 1 )   40 - 41   2023   ISSN:1882-0549

  • Large-scale research project “Study of coupling processes in the solar-terrestrial system“

    山本衛, 小川泰信, 塩川和夫, 吉川顕正, 岩井一正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Multi-event study of 630-nm airglow enhancement during substorms based on ground-based observations in Japan

    森田早紀, 塩川和夫, 大塚雄一, 新堀淳樹, 惣宇利卓弥, 藤本晶子, 吉川顕正, 西岡未知, PERWITASARI Septi

    日本地球惑星科学連合大会予稿集(Web)   2023   2023

  • Quasi-6-Day Wave Modulation of the Inter-Hemispheric Field-Aligned Currents (IHFACs)

    高山久美, 吉川顕正, 三好勉信

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Schumann resonance parameters at Kuju and global lightning activity

    IKEDA Akihiro, UOZUMI Teiji, YOSHIKAWA Akimasa, FUJIMOTO Akiko, ABE Shuji

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Extraction model of ionospheric echoes for time-series ionogram images based-on penalized motion detection

    HIROSHIGE Yu, FUJIMOTO Akiko, IKEDA Akihiro, ABE Shuji, YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • CEJ Effects on Plasma Bubble Generation

    加藤彰紘, 吉川顕正, 藤本晶子

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • On the global characteristics of Pi2 and Pc4 wave generation associated with substorms

    橋本明史, 吉川顕正, 魚住禎司

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • A study on the impact of Sprites on the Global Electrical Circuit by ELF electromagnetic wave observation

    古谷享一, 吉川顕正, 池田昭大

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Geomagnetic Field Observation Project by YOTSUBA-KULOVER Satellite with COTS Magnetomete

    KITAMURA Kentarou, MASUI Hirokazu, ABE Shuji, UOZUMI Teiji, TERAMOTO Mariko, FUJIMOTO Akiko, SANO Kei, YOSHIKAWA Akimasa, CHO Mengu

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Evolution of M-I convection depending on the Alfven conductance as simulated by global MHD model with Alfvenic coupling

    NAKAMIZO Aoi, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa, NAKATA Hiroyuki, FUKAZAWA Keiichiro, TANAKA Takashi

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Multiple-event study of substorm electric-field penetration based on simultaneous observation of 630-nm airglow enhancements

    森田早紀, 塩川和夫, 大塚雄一, 西谷望, 新堀淳樹, 惣宇利卓弥, 藤本晶子, 吉川顕正, 西岡未知, PERWITASARI Septi, 山本衛

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Analysis of electromagnetic field structure in the auroral acceleration region using 3D collisional Hall MHD simulation

    川上航典, 吉川顕正, 深沢圭一郎

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Self-Consistent Quantum Calculations of the 6D Boltzmann-Maxwell System in Collisionless Plasmas Using Quantum Computer

    樋口颯人, PEDERSEN Juan William, 吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • The Impact of the Geomagnetic Storm Event of February 2022 on the Inner Radiation Belt by Test Particle Simulations

    GIRGIS Kirolosse, HADA Tohru, MATSUKIYO Shuichi, MATSUKIYO Shuichi, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa, CHIAN Abraham, CHIAN Abraham

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Severe erosion of the plasmasphere caused by the ring current particle injection into the deep inner magnetosphere

    尾花由紀, 吉川顕正, 丸山奈緒美, 新堀淳樹, 中村紗都子, JUN ChaeWoo, 堀智昭, 三好由純, 橋本久美子, 熊本篤志, 土屋史紀, 笠原禎也, 松岡彩子, 風間洋一, WANG Shiang-Yu, 浅村和史, 篠原育, 横田勝一郎, 桂華邦裕, 笠原慧

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • Development of Affine connections to describe 3D evolving magnetic vector fields and its application to space physics

    YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • An Education Program for CubeSat Development Under Collaboration Between Engineering and Science Faculties in Different Universities

    北村健太郎, 増井博一, 魚住禎司, 寺本万里子, 藤本晶子, CHO Meng, 阿部修司, 吉川顕正

    宇宙科学技術連合講演会講演集(CD-ROM)   67th   2023   ISSN:1884-1945

  • Research on the characteristics of equatorial electrojet occurrence with a peculiar decreasing trend

    池末暉, 吉川顕正, 藤本晶子

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   154th   2023

  • シューマン共鳴の経験モデルの作成

    久永, 学実, 池田, 昭大, 藤本, 晶子, 古川, 翔大, 吉川, 顕正, 魚住, 禎司, 阿部, 修司

    E-19   2022.1

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    Language:Japanese  

    type:Conference Paper
    第27回高専シンポジウム, 2022年1月22日, オンライン開催
    source:https://kosen-sympo.org/

    CiNii Research

    researchmap

  • シューマン共鳴の経験モデルの作成

    久永, 学実, 池田, 昭大, 藤本, 晶子, 古川, 翔大, 吉川, 顕正, 魚住, 禎司, 阿部, 修司

    2022.1

     More details

    Language:Japanese  

    type:Conference Paper
    第27回高専シンポジウム, 2022年1月22日, オンライン開催
    source:https://kosen-sympo.org/

  • Recent activities and future plans of MAGDAS project under new organization

    ABE Shuji, FUJIMOTO Akiko, UOZUMI Teiji, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • Control of switching two observation modes on FM-CW ionospheric observation system based on reinforcement learning

    FUJIMOTO Akiko, MIKURIYA Toru, ABE Shuji, IKEDA Akihiro, YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • Modeling of Magnetosphere-Ionosphere-Atmosphere System to Elucidate the Coupling Process in the Space-Earth Transition Region

    YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • Study of coupling processes in the solar-terrestrial system

    山本衛, 小川泰信, 塩川和夫, 吉川顕正, 吉川顕正

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • Study of the response of the Earth’s magnetosphere to a Sun-Earth oriented interplanetary magnetic field

    城戸蓮太郎, 吉川顕正, 吉川顕正, 魚住禎司

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • A Numerical Simulation of the Formation of Poleward Boundary Intensifications of Auroral Emission due to Ionospheric Polarization

    森澤将, 吉川顕正, 大谷晋一

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • Development of Affine Connection for Describing Spatiotemporal Evolving 3D Magnetic Vector Fields

    吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • Eastward Magnetic Variations in the Equatorial Latitude Associated with the IHFAC Observed on the Ground and LEO

    KITAMURA Kentarou, KITAMURA Kentarou, FUJIMOTO Akiko, FUJIMOTO Akiko, TERAMOTO Mariko, TERAMOTO Mariko, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa, ABE Shuji

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • Comparison of Magnetic Variations Associated with the IHFAC Observed on the Ground and in the LEO

    KITAMURA Kentarou, FUJIMOTO Akiko, YOSHIKAWA Akimasa, ABE Shuji

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • Clarifying Horizontal Vectors of Magnetic Fields Using Principal Component Analysis

    高山久美, 吉川顕正, 三好勉信

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • Investigation of the response of magnetic and electric fields in mid-latitude to the development of CW during substorms

    林萌英, 吉川顕正, 吉川顕正, 藤本晶子, OHTANI Shinichi

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • Comparison of general object detection models for Ionogram sporadic E layer echoes detection

    HIROSHIGE Yu, FUJIMOTO Akiko, ABE Shuji, IKEDA Akihiro, YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • Disruption of accumulated northward IMF lines in the dayside magnetosheath due to discontinuous southward turning of IMF

    HASHIMOTO Tsubasa, YOSHIKAWA Akimasa, TANAKA Takashi

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • Analysis of EEJ structure in M-I coupling system using IGRF model and quasi-three-dimensional potential solver

    伊集院拓也, 吉川顕正, 三好勉信, 品川裕之, 藤原均, 陣英克, 中溝葵, 垰千尋, 塩川和夫

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • High available of general object detection models for detection of E/Es layer echo on FM-CW Ionograms

    HIROSHIGE Yu, FUJIMOTO Akiko, ABE Shuji, IKEDA Akihiro, YOSHIKAWA Akimasa

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • Evolution of electrostatic potential in magnetosphere-ionospheric system as simulated by global MHD model with Alfvenic-coupling

    NAKAMIZO Aoi, YOSHIKAWA Akimasa, YOSHIKAWA Akimasa, NAKATA Hiroyuki, FUKAZAWA Keiichiro, TANAKA Takashi

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • Evolution of electrostatic potential in magnetosphere-ionosphere system as simulated by global MHD model with Alfvenic-coupling

    NAKAMIZO Aoi, YOSHIKAWA Akimasa, NAKATA Hiroyuki, FUKAZAWA Keiichiro, TANAKA Takashi

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • On the electron acceleration process as a carrier of field-aligned current and its energy conversion process in the Alfven wavefront

    YOSHIKAWA Akimasa

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • M-I Coupling at High Latitude via Alfven Waves; Combined Effects through Polarization, Induction and Conductance Evolution

    森澤将, 吉川顕正, 吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • 赤道ファウンテン

    山本衛, 津田敏隆, 津田敏隆, 橋口浩之, 横山竜宏, 塩谷雅人, 大村善治, HALIMURRAHMAN, YATINI Clara, 宮岡宏, 小川泰信, 野沢悟徳, 塩川和夫, 吉川顕正

    京都大学生存圏研究所開放型研究推進部・生存圏学際萌芽研究センター活動報告(Web)   2021   2022

  • Development of Quantum Algorithm for Clarifying Auroral Electron Acceleration Mechanism by Collisional Boltzmann-Maxwell Equation

    樋口颯人, 吉川顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • Physics of Magnetosphere-Ionosphere Coupling System from the Collisional Three-Fluid Model.

    樋口颯人, 吉川顕正

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • How is stacked northward IMF removed from the dayside magnetosheath region due to the southward IMF reversal?

    橋本翼, 吉川顕正, 田中高史

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • Schumann resonance parameters at Kuju during intense solar activity

    IKEDA Akihiro, UOZUMI Teiji, YOSHIKAWA Akimasa, FUJIMOTO Akiko, ABE Shuji

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   152nd   2022

  • Characteristics and Causes of Morning side Pc3 Pulsations

    小原隆博, 吉川顕正, 魚住禎司, 阿部修司

    日本地球惑星科学連合大会予稿集(Web)   2022   2022

  • 磁気赤道域における特異的な太陽フレア効果(SFE*)の発生要因の探究—Research on the causes of specific solar flare effects (SFE∗) in the dip equator

    安永, 朗宏, 藤本, 晶子, 吉川, 顕正

    地球電磁気・地球惑星圏学会総会及び講演会(Web)   2021.10

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    Research on the causes of specific solar flare effects (SFE*) in the dip equator

  • バリウム・リチウム発光雲を使ったダイナモ領域大気プラズマ結合過程の可視化実験

    柿並 義宏, 渡部 重十, 阿部 琢美, 羽生 宏人, 白澤 秀剛, 石坂 圭吾, 山本 衛, 斎藤 享, 津川 卓也, 吉川 顕正, 山本 真行

    観測ロケットシンポジウム2019 講演集 = Proceedings of Sounding Rocket Symposium 2019   2019.8

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    Language:Japanese  

    Rocket experiment Visualization of Atmosphere-Plasma Coupling Process in Dynamo Region by using of Chemical Release of Barium and Lithium
    2nd Sounding Rocket Symposium (August 5-6, 2019. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan

  • 観測ロケットによる電離圏プラズマ加熱現象の解明—Study on the ionospheric electron heating by sounding rocket experiment

    阿部, 琢美, 石坂, 圭吾, 熊本, 篤志, 田中, 真, 松下, 拓輝, 吉川, 顕正, Abe, Takumi, Ishisaka, Keigo, Kumamoto, Atsushi, Tanaka, Makoto, Yoshikawa, Akimasa

    大気球シンポジウム: 平成28年度 = Balloon Symposium: 2016   2016.11

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    Language:Japanese  

    大気球シンポジウム 平成28年度(2016年11月1-2日. 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS)), 相模原市, 神奈川県
    Balloon Symposium 2016 (November 1-2, 2016. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan
    資料番号: SA6000057012
    レポート番号: isas16-sbs-012

  • 外傷性頭蓋内出血に対する内視鏡手術の有用性

    内川 裕貴, 山城 重雄, 等 泰之, 吉川 真, 吉田 顯正, 倉津 純一

    神経外傷   2016.8

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    Usefulness of endoscopic surgery for traumatic intracranial hemorrhage
    Background: Standard surgical treatment for traumatic intracranial hemorrhage such as acute subdural hematoma and brain contusion is craniotomy or craniectomy with general anesthesia. However, we offen hesitate surgery for patients who have severe general state or elderly. For these patients, endoscopic surgery is performed in our hospital. In this study, we investigated cases of traumatic intracranial hemorrhage treated with endoscopic surgery and its surgical results retrospectively.

    Methods: Thirteen patients with traumatic intracranial hemorrhage were admitted to our hospital and treated with endoscopic surgery from April 2008 to August 2015. Nine patients with brain contusion and 4 patients with acute subdural hematoma was included. We investigated following factor: age, sex, pre-operative consciousness, hematoma volume and thickness, evacuation rate of hematoma, complication and modified Rankin Scale (mRS) at discharge.

    Results: All cases were treated with endoscopic surgery only without decompressive craniectomy. In cases of brain contusion, mRS at discharge was 0–2: 4 cases (44&#37;), 3–5: 3 cases (33&#37;), 6: 2 cases (22&#37;). In cases of mRS 6, cause of mortality was myocardial infarction and sepsis, respectively, and no case died of brain trauma. In cases of acute subdural hematoma, mRS at discharge was, 3–5: 3 cases (75&#37;), 6: 1 case (25&#37;). Cause of mortality was rebleeding.

    Conclusion: Endoscopic surgery for traumatic intracranial hemorrhage is a treatment option if its indication is considered carefully. While it is not sufficient for hemostasis, endoscopic surgery is less invasive and possible to perform sufficient decrease of intracranial pressure com­pared with craniotomy or craniectomy. The number of endoscopic surgery for traumatic intracranial hemor­rhage is still small, further studies are needed.

    DOI: 10.32187/neurotraumatology.39.1_32

  • S-310-44 号機による電離圏プラズマ過熱現象の観測 ―ロケット実験速報―

    石坂, 圭吾, 安宅, 祐香, 阿部, 琢美, 坂本, 優美花, 熊本, 篤志, 高橋, 隆男, 田中, 真, 澤井, 萌, 吉川, 顕正, 松下, 拓輝, Keigo, Ishisaka, Yuka, Ataka, Takumi, Abe, Yumika, Sakamoto, Atsushi, Kumamoto, Takao, Takahashi, Makoto, Tanaka, Moe, Sawai, Yoshikawa, Akimasa

    第29回大気圏シンポジウム: 講演集録 = Proceedings of the 29th Atmospheric Science Symposium   2016.3

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    Language:Japanese  

    第29回大気圏シンポジウム(2016年3月7日-8日. 宇宙航空研究開発機構宇宙科学研究所(JAXA)(ISAS)), 相模原市, 神奈川県
    29th Atmospheric Science Symposium (March 7-8, 2016. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS)), Sagamihara, Kanagawa Japan
    資料番号: SA6000051048
    レポート番号: VI-4

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Works

  • 宇宙天気概況解析実験マニュアル

    Yoshikawa A., and A. Nakamizo

    2006.4

  • 宇宙天気概況解析実験マニュアル

    Yoshikawa A., and A. Nakamizo

    2006.4

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Professional Memberships

  • Society of Geomagnetism and Earth, Planetary and Space Sciences

  • American Geophysical Union

  • COMMITTEE ON SPACE RESEARCH

  • European Geophysical Union

  • Japan Geoscience Union

  • アメリカ地球物理学連合米国(AMERICAN GEOPRSICAL UNION)

  • COMMITTEE ON SPACE RESEARCH

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  • アメリカ地球物理学連合米国(AMERICAN GEOPRSICAL UNION)

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  • American Geophysical Union

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  • European Geophysical Union

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  • Japan Geoscience Union

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  • Society of Geomagnetism and Earth, Planetary and Space Sciences

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Committee Memberships

  • 九州大学   理学研究院副研究院長(財務・研究担当)  

    2024.4 - 2026.3   

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  • 地球電磁気・地球惑星圏学会   Councilor   Domestic

    2023.5 - 2025.4   

  • 地球電磁気・地球惑星圏学会   評議員  

    2023.5 - 2025.4   

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  • 九州大学   地球惑星科学部門経理委員長  

    2023.4 - 2024.3   

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    Committee type:Other

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  • 九州大学   未来の科学者委員会委員長  

    2022.4 - 2024.3   

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    Committee type:Other

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  • 九州大学   地球惑星科学部門副部門長  

    2022.4 - 2024.3   

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    Committee type:Other

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  • 九州大学   サイエンスへの誘い編集長  

    2022.4 - 2024.3   

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    Committee type:Other

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  • 九州大学   理学部便り編集長  

    2022.4 - 2024.3   

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    Committee type:Other

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  • 九州大学   理学研究院長補佐(国際・社会貢献担当)  

    2022.4 - 2024.3   

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    Committee type:Other

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  • 第25期日本学術会議   地球惑星科学国際連携分科会 SCOSTEP-STPP小委員会(副委員長)  

    2021.4 - 2024.3   

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  • 九州大学   学生支援委員会  

    2021.4 - 2022.3   

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    Committee type:Other

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  • 九州大学   国際化推進室委員  

    2021.4 - 2022.3   

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    Committee type:Other

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  • ネットワーク開催コアメンバー、大会運営特任管理官   ネットワーク開催コアメンバー、大会運営特任管理官   Domestic

    2020.4 - 2020.7   

  • 学生賞小委員会委員   学生賞小委員会委員   Domestic

    2019.4 - 2022.3   

  • 日本地球惑星科学連合   学生賞小委員会委員  

    2019.4 - 2022.3   

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  • 日本地球惑星科学連合   学生賞小委員会   Domestic

    2019.4 - 2021.3   

  • オーロラメダル賞選考委員会(主管)   オーロラメダル賞選考委員会(主管)   Domestic

    2019.2 - 2022.3   

  • 地球電磁気・地球惑星圏学会   オーロラメダル賞選考委員会(主管)  

    2019.2 - 2022.3   

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  • SuperMAG consortium   steering committee member  

    2018.4 - 2022.3   

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  • 九州大学学術情報リポジトリ専門委員会   オープンデータ推進ワーキンググループ委員  

    2018   

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  • 学会将来検討委員会委員   学会将来検討委員会委員   Domestic

    2017.2 - 2022.3   

  • 地球電磁気・地球惑星圏学会   学会将来検討委員会委員  

    2017.2 - 2022.3   

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  • Steering committee member   Steering committee member   Foreign country

    2015.1 - 2022.3   

  • Steering committee member   Scholarship program subcommittee member   Foreign country

    2015.1 - 2022.3   

  • ISC, SVSS program, The Scientific Committee on Solar Terrestrial Physics (SCOSTEP)   Steering committee member  

    2015.1 - 2022.3   

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  • 日本地球惑星科学連合   宇宙惑星科学分野サイエンスボードメンバー  

    2014.4 - 2022.3   

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  • 日本地球惑星科学連合(宇宙惑星科学セクショボードメンバー)   Organizer   Domestic

    2014.4 - 2020.3   

  • 日本地球惑星科学連合(宇宙惑星科学セクショボードメンバー)   宇宙惑星科学セクショボードメンバー幹事   Domestic

    2014.4 - 2020.3   

  • 代議員(宇宙惑星科学セクション選出)   代議員(宇宙惑星科学セクション選出)   Domestic

    2014.4 - 2020.3   

  • 大林奨励賞推薦委員会委員   大林奨励賞推薦委員会委員   Domestic

    2014.4 - 2017.3   

  • 総合解析委員会委員   総合解析委員会委員   Domestic

    2014.4 - 2015.3   

  • 名古屋大学太陽地球環境研究所   総合観測解析部門専門委員会委員  

    2014.4   

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  • Steering committee member   Steering committee member   Foreign country

    2014.1 - 2022.3   

  • Steering committee member   Steering committe menber   Foreign country

    2014.1 - 2022.3   

  • UN/International Space Weather Initiative (ISWI)   Steering committee member  

    2014.1 - 2022.3   

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  • ICUS/SCOSTEP   Scholarship program subcommittee member  

    2014   

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  • ULTIMA consortium   steering committee member  

    2013.4 - 2022.3   

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  • 地球電磁気・地球惑星圏学会   Steering committee member   Domestic

    2013.4 - 2015.3   

  • 地球電磁気・地球惑星圏学会   第27期運営委員   Domestic

    2013.4 - 2015.3   

  • IUGONET運営協議会   運営協議会 構成員   Domestic

    2013.1 - 2019.3   

  • 活動活性化諮問委員会(Plasma 領域) 委員   活動活性化諮問委員会(Plasma 領域) 委員   Domestic

    2012.6 - 2022.3   

  • アジア太平洋物理学連合   活動活性化諮問委員会(Plasma 領域) 委員  

    2012.6 - 2022.3   

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  • 大学間連携事業IUGONETプロジェクト   運営協議会委員  

    2012.4 - 2022.3   

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  • 九州大学   国際宇宙天気科学・教育センター 運営委員  

    2012.4 - 2022.3   

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    Committee type:Other

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  • 総合観測委員会委員   総合観測委員会委員   Domestic

    2012.4 - 2014.3   

  • 地球電磁気・地球惑星圏学会   将来検討委員会委員  

    2012.4   

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  • アジア太平洋物理学連合   活動活性化諮問委員会(Plasma 領域)委員   Foreign country

    2012.2 - 2014.3   

  • 学会将来検討委員会委員   学会将来検討委員会委員   Domestic

    2012.2 - 2013.3   

  • 運営委員   Steering committee member   Domestic

    2011.4 - 2015.3   

  • 日本地球惑星科学連合   環境災害対応委員   Domestic

    2011.4 - 2014.3   

  • 環境災害対策委員   環境災害対策委員   Domestic

    2011.4 - 2014.3   

  • 地球電磁気・地球惑星圏学会   Steering committee member  

    2011.4 - 2013.3   

  • 地球電磁気・地球惑星圏学会   第26期運営委員  

    2011.4 - 2013.3   

  • 地球電磁気・地球惑星圏学会   Steering committee member   Domestic

    2010.4 - 2012.3   

  • 運営委員   Steering committee member   Foreign country

    2009.4 - 2014.3   

  • 運営委員   EISCAT 特別実験観測分科会委員   Foreign country

    2009.4 - 2014.3   

  • 欧州非干渉散乱データ特別実験観測分科会   審査委員  

    2008.4   

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  • 地球電磁気・地球惑星圏学会   オーロラメダル賞選考委員   Domestic

    2005.4 - 2007.3   

▼display all

Academic Activities

  • EISCATレーダー運営委員会/運営委員

    Role(s): Review, evaluation

    国立極地研究所  2024.4 - 2025.3

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    Type:Scientific advice/Review 

  • EISCATレーダー運営委員会/運営委員

    国立極地研究所  2024.4 - 2025.3

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  • コンビナー International contribution

    JpGU−AGU Joint Meeting 2023  ( Japan ) 2023.5

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • JpGU−AGU Joint Meeting 2023 International contribution

    ( 幕張メッセ Japan ) 2023.5

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    Type:Competition, symposium, etc. 

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  • Screening of academic papers

    Role(s): Peer review

    2023

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    Type:Peer review 

    Number of peer-reviewed articles in foreign language journals:3

  • コンビナー International contribution

    JpGU−AGU Joint Meeting 2022  ( Japan ) 2022.5 - 2022.6

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • Screening of academic papers

    Role(s): Peer review

    2022

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    Type:Peer review 

    Number of peer-reviewed articles in foreign language journals:3

  • その他 International contribution

    JpGU−AGU Joint Meeting 2021:Virtual  ( Japan ) 2021.5 - 2021.6

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • EISCAT特別実験観測分科会委員

    Role(s): Review, evaluation

    欧州非干渉散乱科学協会  2021.4 - 2023.3

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    Type:Scientific advice/Review 

  • 第25期学術会議地球惑星科学委員会地球惑星科学国際連携分科会SCOSTEP/STPP小委員会委員(副委員長)として、地球惑星科学に関する国際的なプロジェクトの立案、促進寄与に関する学術活動を行っている。

    第25期学術会議地球惑星科学委員会地球惑星科学国際連携分科会SCOSTEP/STPP小委員会  2021.4 - 2023.3

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  • EISCAT特別実験観測分科会委員

    欧州非干渉散乱科学協会  2021.4 - 2023.3

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  • Screening of academic papers

    Role(s): Peer review

    2021

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    Type:Peer review 

    Number of peer-reviewed articles in foreign language journals:4

  • その他 International contribution

    JpGU−AGU Joint Meeting 2020:Virtual  ( Japan ) 2020.7

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • その他 International contribution

    JpGU−AGU Joint Meeting 2020:Virtual  ( Japan ) 2020.7

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • Screening of academic papers

    Role(s): Peer review

    2020

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    Type:Peer review 

    Number of peer-reviewed articles in foreign language journals:3

  • その他

    日本地球惑星科学連合2019年大会  ( Japan ) 2019.5

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • 学生賞小委員会/委員

    Role(s): Review, evaluation

    日本地球惑星科学連合  2019.4 - 2022.3

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    Type:Scientific advice/Review 

  • 学生賞小委員会/委員

    日本地球惑星科学連合  2019.4 - 2022.3

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  • オーロラメダル賞選考委員会/主査

    Role(s): Review, evaluation

    地球電磁気・地球惑星圏学会  2019.4 - 2021.3

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    Type:Scientific advice/Review 

  • Screening of academic papers

    Role(s): Peer review

    2019

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    Type:Peer review 

    Number of peer-reviewed articles in foreign language journals:3

  • その他

    日本地球惑星科学連合2018年大会  ( Japan ) 2018.5

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • Other

    Japan-Malaysia Joint Seminar on Space and Earth Electromagnetism 2018  ( Ito-campus, Kyushu University Japan Japan ) 2018.3

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    Type:Competition, symposium, etc. 

    Number of participants:20

  • Screening of academic papers

    Role(s): Peer review

    2018

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    Type:Peer review 

    Number of peer-reviewed articles in foreign language journals:4

  • その他

    日本地球惑星科学連合2017年大会  ( Japan ) 2017.5

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • その他

    シンポジウム「太陽地球系科学に於ける地上観測の現状と課題」  ( Japan ) 2017.3

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    Type:Competition, symposium, etc. 

    Number of participants:60

  • Screening of academic papers

    Role(s): Peer review

    2017

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    Type:Peer review 

    Number of peer-reviewed articles in foreign language journals:3

  • その他

    第140回地球電磁気・地球惑星圏学「磁気圏電離圏結合セッション座長」  ( Japan ) 2016.11

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    Type:Competition, symposium, etc. 

    Number of participants:400

  • Other International contribution

    AOSG2016  ( Beijing China China ) 2016.8

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • Other International contribution

    AGU Chapman Conference on Current in Geospace and Beyond  ( Dubrobunik Croatia Croatia ) 2016.5

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    Type:Competition, symposium, etc. 

    Number of participants:300

  • その他

    日本地球惑星科学連合2016年大会  ( Japan ) 2016.5

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • その他

    日本地球惑星科学連合2016年大会  ( Japan ) 2016.5

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • 科研費審査委員

    Role(s): Review, evaluation

    学術振興会  2016.4 - 2017.3

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    Type:Scientific advice/Review 

  • SVSS-SCHOLARSHIP選考委員会/委員

    Role(s): Review, evaluation

    ISC/SCOSTEP  2016.1 - 2021.12

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    Type:Scientific advice/Review 

  • Screening of academic papers

    Role(s): Peer review

    2016

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    Type:Peer review 

    Number of peer-reviewed articles in foreign language journals:4

  • Other International contribution

    14-th International Symposium on Equatorial Aeronomy (ISEA)  ( Bahir Dar University, Bair Dar Ethiopia Ethiopia ) 2015.10 - 2016.10

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    Type:Competition, symposium, etc. 

    Number of participants:400

  • その他

    日本地球惑星科学連合2015年大会  ( Japan ) 2015.5

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • その他

    日本地球惑星科学連合2015年大会  ( Japan ) 2015.5

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    Type:Competition, symposium, etc. 

    Number of participants:4,000

  • その他 International contribution

    UN/JAPAN Workshop on Space Weather Science 2015  ( Japan ) 2015.3

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    Type:Competition, symposium, etc. 

    Number of participants:120

  • その他 International contribution

    United nations/Japan Workshop on Space Weather Science  ( Japan ) 2015.3

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    Type:Competition, symposium, etc. 

    Number of participants:400

  • その他 International contribution

    United nations/Japan Workshop on Space Weather Science  ( Japan ) 2015.3

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    Type:Competition, symposium, etc. 

  • Screening of academic papers

    Role(s): Peer review

    2015

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    Type:Peer review 

    Number of peer-reviewed articles in foreign language journals:4

  • その他 International contribution

    AGU General Assembly 2014,” Causes of large-scale geomagnetic disturbances”  ( Sanfransisco, USA UnitedStatesofAmerica UnitedStatesofAmerica ) 2014.12

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    Type:Competition, symposium, etc. 

  • Convener International contribution

    AGU General Assembly 2014,” Causes of large-scale geomagnetic disturbances  ( UnitedStatesofAmerica ) 2014.12 - 2013.12

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    Type:Competition, symposium, etc. 

    Number of participants:120

  • Science Program Committee International contribution

    UN/Austria Symposium on “Space Science and the United Nations”  ( Austria ) 2014.9 - 2013.9

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    Type:Competition, symposium, etc. 

    Number of participants:60

  • Other International contribution

    AGU Chapman Conference on Low frequency Waves in Space Plasma  ( Chez-island, Korea Korea Korea ) 2014.8 - 2014.9

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  • 国際連合宇宙部(UN/OOSA)と連携して、国際宇宙天気イニシアチブプロジェクト(ISWI: International Space Weather Initiative)のexcecutive commiteeメンバーとして、国際的なキャパシティビルディング活動や学術振興活動を行っている。

    International Space Weather Initiative Project Steering committee (http://www.iswi-secretariat.org)  2014.4 - 2022.3

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    International Space Weather Initiative (ISWI) is a program of international cooperation to advance the space weather science by a combination of instrument deployment, analysis and interpretation of space weather data from the deployed instruments in conjunction with space data, and communicate the results to the public and students.
    ISWI is a follow-up activity to the successful IHY 2007, but focusing exclusively on space weather.
    The goal of the ISWI is to develop the scientific insight necessary to understand the science, and to reconstruct and forecast near-Earth space weather. This includes instrumentation, data analysis, modeling, education, training, and public outreach.

    researchmap

  • 代議員(宇宙惑星科学選出)

    Role(s): Review, evaluation

    日本地球惑星科学連合  2014.4 - 2019.3

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    Type:Scientific advice/Review 

  • 大林奨励賞推薦委員会/委員

    Role(s): Review, evaluation

    地球電磁気・地球惑星圏学会  2014.1 - 2017.3

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    Type:Scientific advice/Review 

  • その他 International contribution

    International Workshop on global ionospheric dynamics II  ( Japan ) 2013.11

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    Type:Competition, symposium, etc. 

    Number of participants:20

  • その他 International contribution

    UN-ISWI/MAGDAS AFRICA School  ( ココディ大学・アブジャ・コートジボワール その他 その他 ) 2013.9

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    Type:Competition, symposium, etc. 

    Number of participants:70

  • その他 International contribution

    UN/Austria Symposium on “Space Weather Data, Instruments and Models: Looking Beyond the International Space Weather Initiative  ( Austria ) 2013.9

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    Type:Competition, symposium, etc. 

    Number of participants:60

  • Earth, Planet and Space International contribution

    2013.9 - 2017.12

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    Type:Academic society, research group, etc. 

  • 地球電磁気・地球惑星圏科学学会会報誌

    2013.4 - 2015.3

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    Type:Academic society, research group, etc. 

  • その他 International contribution

    International Workshop on global ionospheric dynamics I  ( Japan ) 2013.1

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    Type:Competition, symposium, etc. 

    Number of participants:20

  • その他 International contribution

    UN-ISWI/MAGDAS INDONESIA School  ( Indonesia ) 2012.9

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    Type:Competition, symposium, etc. 

    Number of participants:60

  • EISCAT特別実験観測分科会委員

    Role(s): Review, evaluation

    欧州非干渉散乱科学協会  2012.4 - 2014.3

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    Type:Scientific advice/Review 

  • その他

    国立極地研究所研究集会:極域における電離圏パラメータの非線形発展:モデル化と検証II  ( Japan ) 2011.12

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    Type:Competition, symposium, etc. 

    Number of participants:30

  • その他

    極域における電離圏パラメータの非線形発展:モデル化と検証II  ( Japan ) 2011.12

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    Type:Competition, symposium, etc. 

  • その他 International contribution

    Workshop on Physical Processes in Non-Uniform Finite Magnetospheric Systems-50 Years of Tamao's Resonant Mode Coupling Theory  ( Japan ) 2011.9

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    Type:Competition, symposium, etc. 

    Number of participants:90

  • その他 International contribution

    Workshop on Physical Processes in Non-Uniform Finite Magnetospheric Systems-50 Years of Tamao's Resonant Mode Coupling Theory  ( Japan ) 2011.9

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    Type:Competition, symposium, etc. 

  • その他 International contribution

    UN-ISWI/MAGDAS School on Litho-Space Weather  ( Redeemers 大学、ラゴス、ナイジェリア その他 その他 ) 2011.8

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    Type:Competition, symposium, etc. 

    Number of participants:60

  • Earth, Planet and Space International contribution

    2011.4 - 2013.3

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    Type:Academic society, research group, etc. 

  • EISCAT特別実験観測分科会委員

    Role(s): Review, evaluation

    欧州非干渉散乱科学協会  2011.4 - 2012.3

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    Type:Scientific advice/Review 

  • その他

    国立極地研究所研究集会:極域における電離圏パラメータの非線形発展:モデル化と検証  ( Japan ) 2010.12

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    Type:Competition, symposium, etc. 

    Number of participants:30

  • 座長(Chairmanship)

    極域における電離圏パラメータの非線形発展:モデル化と検証  ( Japan ) 2010.12

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    Type:Competition, symposium, etc. 

  • その他

    地球惑星科学関連合同大会2010年度大会  ( Japan ) 2010.5

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    Type:Competition, symposium, etc. 

    Number of participants:140

  • EISCAT特別実験観測分科会委員

    Role(s): Review, evaluation

    欧州非干渉散乱科学協会  2010.4 - 2011.3

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    Type:Scientific advice/Review 

  • 座長(Chairmanship)

    第6回ジオスペース研究会  ( Japan ) 2010.3 - 2009.3

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    Type:Competition, symposium, etc. 

  • その他

    名古屋大学太陽地球環境研究所: 太陽地球/惑星系統合型モデル・シミュレータ構築に向けた研究集会  ( Japan ) 2009.8

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    Type:Competition, symposium, etc. 

  • コンビーナ

    名古屋大学太陽地球環境研究所:太陽地球/惑星系統合型モデル・シミュレータ構築に向けた研究集会  ( Japan ) 2009.8 - 2008.8

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    地球惑星科学関連合同大会2009年度大会  ( Japan ) 2009.5

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    Number of participants:140

  • 地球惑星科学関連合同大会2009年度大会

    ( 千葉・幕張メッセ 国名:Japan Japan ) 2009.5

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  • EISCAT特別実験観測分科会委員

    Role(s): Review, evaluation

    欧州非干渉散乱科学協会  2009.4 - 2010.3

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    第5回ジオスペース研究会  ( Japan ) 2009.3

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    名古屋大学太陽地球環境研究所: 太陽地球/惑星系統合型モデル・シミュレータ構築に向けた研究集集会  ( Japan ) 2008.8 - 2009.8

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    名古屋大学太陽地球環境研究所:太陽地球/惑星系統合型モデル・シミュレータ構築に向けた研究集会  ( Japan ) 2008.8

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    地球惑星科学関連合同大会2008年度大会  ( Japan ) 2008.5

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  • 地球惑星科学関連合同大会2008年度大会

    ( 千葉・幕張メッセ 国名:Japan Japan ) 2008.5

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    第4回ジオスペース研究会  ( Japan ) 2008.3

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    ( 福岡 Japan ) 2008.3

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    ISSI team meeting  ( International Space Science Institute, Bern Switzerland Switzerland ) 2007.11

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    ( International Space Science Institute, Bern Switzerland ) 2007.11

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    名古屋大学太陽地球環境研究所:磁気嵐シミュレータ検討会  ( Japan ) 2007.9

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    磁気嵐シミュレータ検討会  ( Japan ) 2007.9

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  • 磁気嵐シミュレータ検討会

    ( 名古屋大学太陽地球環境研究所 Japan ) 2007.9

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    地球惑星科学関連合同大会2007年度大会  ( Japan ) 2007.5

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  • 地球惑星科学関連合同大会2007年度大会

    ( 千葉・幕張メッセ 国名:Japan Japan ) 2007.5

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    名古屋大学太陽地球環境研究所:磁気嵐シミュレータ検討会  ( Japan ) 2007.2 - Present

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    磁気嵐シミュレータ検討会  ( Japan ) 2007.2

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  • 磁気嵐シミュレータ検討会

    ( 名古屋大学太陽地球環境研究所 Japan ) 2007.2

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  • 名古屋大学太陽地球環境研究所:磁気嵐シミュレータ検討会

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    名古屋大学太陽地球環境研究所:磁気嵐シミュレータ検討会  ( Japan ) 2006.8

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  • 名古屋大学太陽地球環境研究所:磁気嵐シミュレータ検討会

    ( 名古屋大学太陽地球環境研究所 Japan ) 2006.8

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    地球惑星科学関連合同大会2006年度大会  ( Japan ) 2006.5

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  • 地球惑星科学関連合同大会2006年度大会

    ( 千葉・幕張メッセ 国名:Japan Japan ) 2006.5

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    磁気嵐シミュレータ検討会  ( Japan ) 2006.3

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  • 磁気嵐シミュレータ検討会

    ( 名古屋大学太陽地球環境研究所 Japan ) 2006.3

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    宇宙プラズマ/太陽系環境研究の将来構想座談会(SSF)4  ( Japan ) 2005.12

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  • 宇宙プラズマ/太陽系環境研究の将来構想座談会(SSF)4

    ( 名古屋 Japan ) 2005.12

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    ISSI team meeting  ( Bern Switzerland Switzerland ) 2005.10

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    ( Bern Switzerland ) 2005.10

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    The IAGA Scientific Assembly in Toulouse  ( France ) 2005.7

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    Number of participants:300

  • The IAGA Scientific Assembly in Toulouse International contribution

    ( ツールース France ) 2005.7

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    地球惑星科学関連合同大会2004年度大会  ( Japan ) 2005.5 - Present

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    地球惑星科学関連合同大会2005年度大会  ( Japan ) 2005.5

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    Number of participants:140

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    地球惑星科学合同大会2005年大会  ( Japan ) 2005.5

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  • 地球惑星科学合同大会2005年大会

    ( 東京 Japan ) 2005.5

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  • 地球惑星科学関連合同大会2005年度大会

    ( 千葉・幕張メッセ 国名:Japan Japan ) 2005.5

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  • 地球惑星科学関連合同大会2004年度大会

    ( 千葉・幕張メッセ 国名:Japan Japan ) 2005.5

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    Chapman conference on magnetospheric ULF waves  ( UnitedStatesofAmerica ) 2005.3

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    Chapman conference on magnetospheric ULF waves-Magnetospheric diagonosis session  ( San Diego UnitedStatesofAmerica UnitedStatesofAmerica ) 2005.3

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    Chapman conference on magnetospheric ULF waves-Magnetosphere-ionosphere coupling session  ( San Diego UnitedStatesofAmerica UnitedStatesofAmerica ) 2005.3

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    ( カルフォルニア、サンディエゴ UnitedStatesofAmerica ) 2005.3

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  • Chapman conference on magnetospheric ULF waves-Magnetospheric diagonosis session International contribution

    ( San Diego UnitedStatesofAmerica ) 2005.3

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    ( San Diego UnitedStatesofAmerica ) 2005.3

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    地球惑星科学関連合同大会2004年度大会  ( Japan ) 2004.5

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    地球惑星科学合同大会2004年大会  ( Japan ) 2004.5

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    ( 東京 Japan ) 2004.5

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  • 地球惑星科学関連合同大会2004年度大会

    ( 千葉・幕張メッセ Japan ) 2004.5

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    CAWSES宇宙天気シンポジウム  ( Japan ) 2004.3

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    ( 九州大学 Japan ) 2004.3

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    地球惑星科学関連合同大会2003年度大会  ( Japan ) 2003.5

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    地球惑星科学合同大会2003年大会  ( Japan ) 2003.5

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    ( 東京 Japan ) 2003.5

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    ( 千葉・幕張メッセ Japan ) 2003.5

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    地球惑星科学関連合同大会2002年度大会  ( Japan ) 2002.5

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    地球惑星科学合同大会2002年大会  ( Japan ) 2002.5

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    ( 東京 Japan ) 2002.5

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    ( 千葉・幕張メッセ Japan ) 2002.5

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  • 第24期日本学術会議マスタープラン2020に於いて、京都大学、名古屋大学、国立極地研究所と共同提案した「太陽地球結合系の研究基盤形成」が、重点大型研究計画として採択された。

    2020.1

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    太陽から地球へのエネルギーとプラズマの流れ、太陽活動に対する地 球大気圏・電離圏・磁気圏の応答過程を知り、太陽地球系の結合過程を 統一したシステムとして定量的理解を深める。太陽から放射エネルギー と太陽風(高エネルギー粒子の流れ)が地球に来る。前者は定常的で赤 道域で最大、後者は小さいが間欠的かつ極域に集中するため放射エネル ギーに匹敵する(右図)。赤道と極域の2つの特異点に大型大気レーダ ーを建設するとともに、全球に広域地上観測網を整備し、衛星観測・モ デル研究と連携しつつ研究を推進する。
    1)赤道ファウンテン:赤道域で大気擾乱が最大であるインドネシアに赤道 MU レーダーを設置して総合観測拠点とし、地表付近の対流圏、 中層大気、超高層大気に至る高度領域に共通するエネルギー・物質の 噴流・循環過程(赤道ファウンテン)を解明する。
    2)極域エネルギー流入過程:スカンジナビア半島北部の EISCAT_3D レ ーダー(6ヶ国共同、国際的には建設中)を完成させる。太陽風エネ ルギー流入により激しく変動する極域の電離圏・磁気圏を高解像度で 3次元観測し、電離圏・中層大気へのエネルギー流入と応答過程を解 明する。
    3)グローバル結合過程:中層・超高層大気の広域地上観測網を赤道から極域に展開する。大学間連携「超高層大気長期変動 の全球地上ネットワーク観測・研究(IUGONET)」による大量・多様な観測データの統合メタデータデータベース・解析シス テムを活用して総合解析する。観測衛星と連携、数値モデル研究(全大気圏モデル GAIA 等)と共同でエネルギーと物質のグ ローバル結合過程を研究する。

  • 第24期日本学術会議マスタープラン2020に於いて、京都大学、名古屋大学、国立極地研究所と共同提案した「太陽地球結合系の研究基盤形成」が、重点大型研究計画として採択された。

    2020.1

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    太陽から地球へのエネルギーとプラズマの流れ、太陽活動に対する地 球大気圏・電離圏・磁気圏の応答過程を知り、太陽地球系の結合過程を 統一したシステムとして定量的理解を深める。太陽から放射エネルギー と太陽風(高エネルギー粒子の流れ)が地球に来る。前者は定常的で赤 道域で最大、後者は小さいが間欠的かつ極域に集中するため放射エネル ギーに匹敵する(右図)。赤道と極域の2つの特異点に大型大気レーダ ーを建設するとともに、全球に広域地上観測網を整備し、衛星観測・モ デル研究と連携しつつ研究を推進する。
    1)赤道ファウンテン:赤道域で大気擾乱が最大であるインドネシアに赤道 MU レーダーを設置して総合観測拠点とし、地表付近の対流圏、 中層大気、超高層大気に至る高度領域に共通するエネルギー・物質の 噴流・循環過程(赤道ファウンテン)を解明する。
    2)極域エネルギー流入過程:スカンジナビア半島北部の EISCAT_3D レ ーダー(6ヶ国共同、国際的には建設中)を完成させる。太陽風エネ ルギー流入により激しく変動する極域の電離圏・磁気圏を高解像度で 3次元観測し、電離圏・中層大気へのエネルギー流入と応答過程を解 明する。
    3)グローバル結合過程:中層・超高層大気の広域地上観測網を赤道から極域に展開する。大学間連携「超高層大気長期変動 の全球地上ネットワーク観測・研究(IUGONET)」による大量・多様な観測データの統合メタデータデータベース・解析シス テムを活用して総合解析する。観測衛星と連携、数値モデル研究(全大気圏モデル GAIA 等)と共同でエネルギーと物質のグ ローバル結合過程を研究する。

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  • 最新磁気圏電離圏結合の教科書執筆 「Earth’s Ionosphere: Theory and Phenomenology of Cowling Channels」, in Electric Currents in Geospace and Beyond (eds A. Keiling, O. Marghitu, and M. Wheatland), John Wiley & Sons, Inc, Hoboken, N.J., doi: 10.1002/9781119324522.ch25

    2018.1

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    The Cowling channel is a generic name of a current system forming inside a high conductivity band, in which a secondary polarization electric field modifies the current flow. The polarization field is excited when a divergent part of Hall current driven by the primary electric field is prevented from flowing out to the magnetosphere as the field-aligned current (FAC).
    The Cowling effect is now well known as enhancement of current flow in the direction of the primary electric field by the secondary Hall current [Chapman, 1956]. The Cowling effect was first investigated by Cowling [1932] in connection with the solar atmosphere. The generation mechanism [Cowling and Boreger, 1948] was adopted to account for equatorial electrojet [Hirono, 1950, Untied, 1967] and auroral electrojet [Boström, 1964]. The Cowling effect has been investigated theoretically and observationally [e.g., Baujohann, 1983; Yasuhara et al., 1985; Haerendel, 2008, Amm et al., [2008]; Amm and Fujii, 2008; Marghitu et al., 2011].
    Figure 1 shows traditional picture of two-dimensional Cowling channel model elongated along east-west direction [e.g., Baumjohann, 1983], in which ionospheric Hall and Pedersen conductivity are height-integrated. The primary westward electric field (E1) drives northward Hall current and westward Pedersen current. The southward secondary field (E2) is generated so that the Pedersen current closes the primary Hall current between the conductivity gradients. The secondary Hall current flows in the same direction as the primary Pedersen current and forms the electrojet system.
    Generally, it is difficult to specify polarization effects in the ionosphere from ground-based data alone. These data only allow to infer the resultant total electrodynamic fields, but cannot track back the chain of cause and consequence that led to the physical situation which then causes these observed total fields. Thus, using ground-based data alone in most cases we can only state whether an observed situation is consistent or not with the expectations from an “active” polarization effect.
    To quantify the Cowling effect, we need to know the relative strength of the polarization electric field to total electric field and to what extent it cancels (closes) the primary Hall current. This problem is complementary to the question: How much curl-free Hall current flows out to the magnetosphere as FAC?
    In order to reply to this problem provided by Amm et al., [2008], modeling of Cowling channel has been further developed.
    To describe the Cowling channel, Amm et al., [2011] and Fujii et al., [2011] introduce a parameter called the Cowling efficiency. It is defined as a ratio how much of Hall current is confined inside the ionosphere by the secondary Pedersen current excited by the polarization electric field. Definition of Cowling efficiency is practically important. It provides a general way to calculate quantitatively the polarization electric field, if the Cowling efficiency, the conductance, and either primary or the total electric fields are known [Amm et al., 2013].
    It has been suggested that to identify the Cowling efficiency for specific phenomenon, one needs to know the impedance of the magnetospheric circuit, which completes the current circuit in the M-I system via FAC [e.g., Fujii et al., 2011]. However, it is questionable to assign a magnetospheric impedance for steady state because the M-I system is always changing dynamically.
    The M-I coupling process via shear Alfven waves has been used to investigate the nonstationary FAC closure by ionospheric conducting current [e.g., Scholer, 1970]. Assuming specific electric field configurations of an incident wave, Glaβmeier [1983] and Itonaga and Kitamura [1988] have shown that a secondary polarization field due to gradients of Hall conductance can appear in the reflected wave. Actually, the Alfven wave approach can be used to describe not only local and dynamical phenomena but also more generally global quasi-static M-I coupling processes [Yoshikawa et al., 2010]. Therefore it is very important to understand the how the shear Alfven wave interacts with the Cowling channel.
    Yoshikawa et al., [2011a] give a general theory about M-I coupling, independent of specific geometries or specific situations. This theory, based on the Alfven waves used in a way of a basis function for the M-I coupling process, is later applied in Yoshikawa et al., [2013a] and Yoshikawa et al., [2013b] specifically to a Cowling channel situation, but can be applied for any general case.
    Most of Cowling channel models introduced so far rely on a thin-sheet ionosphere [e.g., Baujohann, 1983]. However, in a realistic ionospheric E-layer, a vertical distribution of the Pedersen conductivity and Hall conductivity has maximum peak around 125 km altitude and around 110 km altitude, respectively [e.g., Richmond and Thayer, 2000]. In order properly consider the ionospheric current closure, one also takes into account the ionospheric thickness [Amm et al., 2008]. One step in this direction is to assume that the Pedersen and Hall current flow thin layers at different altitudes [Fujii et al., 2011; Amm et al., 2011; Yoshikawa et al., 2011].
    The classical picture illustrated in Figure 1 describes divergence-free approximation of auroral electrojet. However, a longitudinal boarder of Cowling channel is also important for considering finite aurora arc formation and Harang reversal region [Harang, 1947; Heppner, 1972; Marghitu et al., 2011], where the auroral electrojet is diverging.
    Amm et al., [2008] give a review of the work available in the literature until 2008 regarding following aspects of ionospheric electrodynamics and Magnetosphere-Ionosphere (M-I) coupling:
    -Polarization effect in the ionosphere (often referred to as “Cowling effect)”
    -Inductive effect in the ionosphere
    -The effect of the three-dimensional (3D) nature of the ionosphere for ionospheric electrodynamics
    -The consequences of the above mentioned aspects to M-I coupling.
    Marghitu, [2012] provides an excellent review for auroral arc electrodynamics, by considering the 1D thin uniform arc, the 2D thick uniform arc, and the non-uniform arc. The various arc features are assembled together in a tentative 3D arc model.
    The purpose of this chapter is to review the recent development of Cowling channel model after Amm et al., [2008] and Marghitu, [2012]. Recent work provide an extension of theoretical description of the classical Cowling channel with respect to the following aspects: 1) Taking into account the 3D nature of ionosphere by introducing two current layers at different altitudes, and 2) considering finite length of the Cowling channel by introducing a conductance boundary not only at the meridional borders of Cowling channel, but also at its zonal boundaries. Using this improved model, schematically illustrated in Figure 2 with Cowling efficiency description, we discuss current closure and their energy principle for evolution of Cowling channel. Energy flow inside the Cowling channel and impact of polarization effect on Joule dissipation in more general M-I coupling scheme are also provided. In addition, we also clarify how shear Alfven wave interacts to the Cowling channel and their application to the global magnetosphere-ionosphere coupling simulations.

  • 最新磁気圏電離圏結合の教科書執筆 「Earth’s Ionosphere: Theory and Phenomenology of Cowling Channels」, in Electric Currents in Geospace and Beyond (eds A. Keiling, O. Marghitu, and M. Wheatland), John Wiley & Sons, Inc, Hoboken, N.J., doi: 10.1002/9781119324522.ch25

    2018.1

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    The Cowling channel is a generic name of a current system forming inside a high conductivity band, in which a secondary polarization electric field modifies the current flow. The polarization field is excited when a divergent part of Hall current driven by the primary electric field is prevented from flowing out to the magnetosphere as the field-aligned current (FAC).
    The Cowling effect is now well known as enhancement of current flow in the direction of the primary electric field by the secondary Hall current [Chapman, 1956]. The Cowling effect was first investigated by Cowling [1932] in connection with the solar atmosphere. The generation mechanism [Cowling and Boreger, 1948] was adopted to account for equatorial electrojet [Hirono, 1950, Untied, 1967] and auroral electrojet [Boström, 1964]. The Cowling effect has been investigated theoretically and observationally [e.g., Baujohann, 1983; Yasuhara et al., 1985; Haerendel, 2008, Amm et al., [2008]; Amm and Fujii, 2008; Marghitu et al., 2011].
    Figure 1 shows traditional picture of two-dimensional Cowling channel model elongated along east-west direction [e.g., Baumjohann, 1983], in which ionospheric Hall and Pedersen conductivity are height-integrated. The primary westward electric field (E1) drives northward Hall current and westward Pedersen current. The southward secondary field (E2) is generated so that the Pedersen current closes the primary Hall current between the conductivity gradients. The secondary Hall current flows in the same direction as the primary Pedersen current and forms the electrojet system.
    Generally, it is difficult to specify polarization effects in the ionosphere from ground-based data alone. These data only allow to infer the resultant total electrodynamic fields, but cannot track back the chain of cause and consequence that led to the physical situation which then causes these observed total fields. Thus, using ground-based data alone in most cases we can only state whether an observed situation is consistent or not with the expectations from an “active” polarization effect.
    To quantify the Cowling effect, we need to know the relative strength of the polarization electric field to total electric field and to what extent it cancels (closes) the primary Hall current. This problem is complementary to the question: How much curl-free Hall current flows out to the magnetosphere as FAC?
    In order to reply to this problem provided by Amm et al., [2008], modeling of Cowling channel has been further developed.
    To describe the Cowling channel, Amm et al., [2011] and Fujii et al., [2011] introduce a parameter called the Cowling efficiency. It is defined as a ratio how much of Hall current is confined inside the ionosphere by the secondary Pedersen current excited by the polarization electric field. Definition of Cowling efficiency is practically important. It provides a general way to calculate quantitatively the polarization electric field, if the Cowling efficiency, the conductance, and either primary or the total electric fields are known [Amm et al., 2013].
    It has been suggested that to identify the Cowling efficiency for specific phenomenon, one needs to know the impedance of the magnetospheric circuit, which completes the current circuit in the M-I system via FAC [e.g., Fujii et al., 2011]. However, it is questionable to assign a magnetospheric impedance for steady state because the M-I system is always changing dynamically.
    The M-I coupling process via shear Alfven waves has been used to investigate the nonstationary FAC closure by ionospheric conducting current [e.g., Scholer, 1970]. Assuming specific electric field configurations of an incident wave, Glaβmeier [1983] and Itonaga and Kitamura [1988] have shown that a secondary polarization field due to gradients of Hall conductance can appear in the reflected wave. Actually, the Alfven wave approach can be used to describe not only local and dynamical phenomena but also more generally global quasi-static M-I coupling processes [Yoshikawa et al., 2010]. Therefore it is very important to understand the how the shear Alfven wave interacts with the Cowling channel.
    Yoshikawa et al., [2011a] give a general theory about M-I coupling, independent of specific geometries or specific situations. This theory, based on the Alfven waves used in a way of a basis function for the M-I coupling process, is later applied in Yoshikawa et al., [2013a] and Yoshikawa et al., [2013b] specifically to a Cowling channel situation, but can be applied for any general case.
    Most of Cowling channel models introduced so far rely on a thin-sheet ionosphere [e.g., Baujohann, 1983]. However, in a realistic ionospheric E-layer, a vertical distribution of the Pedersen conductivity and Hall conductivity has maximum peak around 125 km altitude and around 110 km altitude, respectively [e.g., Richmond and Thayer, 2000]. In order properly consider the ionospheric current closure, one also takes into account the ionospheric thickness [Amm et al., 2008]. One step in this direction is to assume that the Pedersen and Hall current flow thin layers at different altitudes [Fujii et al., 2011; Amm et al., 2011; Yoshikawa et al., 2011].
    The classical picture illustrated in Figure 1 describes divergence-free approximation of auroral electrojet. However, a longitudinal boarder of Cowling channel is also important for considering finite aurora arc formation and Harang reversal region [Harang, 1947; Heppner, 1972; Marghitu et al., 2011], where the auroral electrojet is diverging.
    Amm et al., [2008] give a review of the work available in the literature until 2008 regarding following aspects of ionospheric electrodynamics and Magnetosphere-Ionosphere (M-I) coupling:
    -Polarization effect in the ionosphere (often referred to as “Cowling effect)”
    -Inductive effect in the ionosphere
    -The effect of the three-dimensional (3D) nature of the ionosphere for ionospheric electrodynamics
    -The consequences of the above mentioned aspects to M-I coupling.
    Marghitu, [2012] provides an excellent review for auroral arc electrodynamics, by considering the 1D thin uniform arc, the 2D thick uniform arc, and the non-uniform arc. The various arc features are assembled together in a tentative 3D arc model.
    The purpose of this chapter is to review the recent development of Cowling channel model after Amm et al., [2008] and Marghitu, [2012]. Recent work provide an extension of theoretical description of the classical Cowling channel with respect to the following aspects: 1) Taking into account the 3D nature of ionosphere by introducing two current layers at different altitudes, and 2) considering finite length of the Cowling channel by introducing a conductance boundary not only at the meridional borders of Cowling channel, but also at its zonal boundaries. Using this improved model, schematically illustrated in Figure 2 with Cowling efficiency description, we discuss current closure and their energy principle for evolution of Cowling channel. Energy flow inside the Cowling channel and impact of polarization effect on Joule dissipation in more general M-I coupling scheme are also provided. In addition, we also clarify how shear Alfven wave interacts to the Cowling channel and their application to the global magnetosphere-ionosphere coupling simulations.

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  • 論文名「The initiation of the poleward boundary intensification of auroral emission by fast polar cap flows: A new interpretation based on ionospheric polarization」のJGR Space Physicsへの出版

    2016.12

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    The auroral intensification at the poleward boundary of the auroral oval is often considered to be the ionospheric manifestation of the distant reconnection. In the present study, however, we propose that the poleward boundary intensifications (PBIs) are initiated by ionospheric polarization due to fast polar cap flows, which are known to be well correlated with PBIs. The current continuity at the ionosphere can be described in two different ways, that is, the reflection of an Alfv�n wave and the closure of Pedersen and Hall currents with field-aligned currents (FACs). The required consistency between the two approaches sets a framework for modeling the ionospheric polarization, and we numerically test the aforementioned idea focusing on an induced upward FAC as indicative of PBIs. The results show that in case the polar cap flow channel approaches the auroral oval perpendicularly from poleward, (i) upward and downward FACs are induced at the poleward boundary to the west and east of the longitudinal center of the flow channel, respectively; (ii) those induced FACs extend much wider in longitude than the flow channel; (iii) the peak densities of those induced FACs are significantly larger than those of the incident FACs; (iv) those induced FACs are distributed almost symmetrically in longitude, indicating that the Pedersen polarization dominates the Hall polarization; and (v) if the polar cap flow inclined dawnward (duskward), an upward (downward) FAC is induced first. These results are consistent with the reported characteristics of PBIs, which are rather difficult to explain otherwise.

  • 論文名「The initiation of the poleward boundary intensification of auroral emission by fast polar cap flows: A new interpretation based on ionospheric polarization」のJGR Space Physicsへの出版

    2016.12

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    The auroral intensification at the poleward boundary of the auroral oval is often considered to be the ionospheric manifestation of the distant reconnection. In the present study, however, we propose that the poleward boundary intensifications (PBIs) are initiated by ionospheric polarization due to fast polar cap flows, which are known to be well correlated with PBIs. The current continuity at the ionosphere can be described in two different ways, that is, the reflection of an Alfv�n wave and the closure of Pedersen and Hall currents with field-aligned currents (FACs). The required consistency between the two approaches sets a framework for modeling the ionospheric polarization, and we numerically test the aforementioned idea focusing on an induced upward FAC as indicative of PBIs. The results show that in case the polar cap flow channel approaches the auroral oval perpendicularly from poleward, (i) upward and downward FACs are induced at the poleward boundary to the west and east of the longitudinal center of the flow channel, respectively; (ii) those induced FACs extend much wider in longitude than the flow channel; (iii) the peak densities of those induced FACs are significantly larger than those of the incident FACs; (iv) those induced FACs are distributed almost symmetrically in longitude, indicating that the Pedersen polarization dominates the Hall polarization; and (v) if the polar cap flow inclined dawnward (duskward), an upward (downward) FAC is induced first. These results are consistent with the reported characteristics of PBIs, which are rather difficult to explain otherwise.

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Research Projects

  • 多様なデータにメタデータを付与できるシステムの開発と複数実データセットへの適用

    2023.4 - 2024.3

    Research commissions

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  • IUGONETメタデータデータベースの保守・更新、及び、システムの改良

    2023.4 - 2024.3

    Research commissions

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  • MAGDAS/CPMNプロジェクト

    2023

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  • IUGONETメタデータデータベースの保守・更新、及び、システムの改良

    2022.4 - 2023.3

    Research commissions

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  • 多様なデータにメタデータを付与できるシステムの開発と複数実データセットへの適用

    2022.4 - 2023.3

    Research commissions

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  • 国際地上観測網と人工衛星観測・モデリングに基づくジオスペース変動の国際共同研究

    Grant number:22K21345  2022 - 2029

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  International Leading Research

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  • 国際地上観測網と人工衛星観測・モデリングに基づくジオスペース変動の国際共同研究

    Grant number:22K21345  2022 - 2028

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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  • オーロラ嵐時の電離圏全球電場構造・電流クロージャー形成の解明

    Grant number:22K03707  2022 - 2025

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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  • オーロラ嵐時の電離圏全球電場構造・電流クロージャー形成の解明

    Grant number:22K03707  2022 - 2024

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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  • MAGDAS/CPMNプロジェクト

    2022

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  • 大学間連携による理学工学融合実践的宇宙ミッション早期教育プログラム

    2021.4 - 2024.3

    Research commissions

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    Authorship:Collaborating Investigator(s) (not designated on Grant-in-Aid)  Grant type:Other funds from industry-academia collaboration

  • IUGONETメタデータデータベースの保守・更新、及び、システムの改良

    2021.4 - 2022.3

    Research commissions

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  • 多様なデータにメタデータを付与できるシステムの開発と複数実データセットへの適用

    2021.4 - 2022.3

    Research commissions

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  • 地上多点ネットワークに基づく超高層大気変動の緯度間結合の観測的研究

    Grant number:21H04518  2021 - 2026

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (A)

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  • 地上多点ネットワークに基づく超高層大気変動の緯度間結合の観測的研究

    Grant number:21H04518  2021 - 2025

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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  • 自律型電離圏観測による赤道ジェット電流-プラズマバブル発生/抑制モデルの実証

    Grant number:21K03646  2021 - 2025

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

    藤本 晶子, 阿部 修司, 吉川 顕正

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    電離圏電子密度の乱れ「プラズマバブル」は、衛星測位や衛星通信等に影響を与え、GPS測位精度の低下や、車輛、船舶、航空機の安全運航に支障をきたす。本研究では、機械学習/強化学習による自律的な電離圏観測機器制御システムを設計・作成し、既存手法では困難なプラズマバブル形成・抑制過程の「電離圏E領域―F領域上下結合」を捉えるシームレス・マルチ電離圏観測を実施する。これに、プラズマバブル形成・抑制の環境場をコントロールする赤道域地磁気変動観測、大気圏電離圏モデルGAIA数値シミュレーションを組み合わせて、グローバルな形成過程の観点からプラズマバブル発生・抑制モデルを包括的に明らかにする。

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  • 大学間連携による理学工学融合実践的宇宙ミッション早期教育プログラム

    2021 - 2023

    令和3年度宇宙航空科学技術推進委託費(プログラム名:宇宙航空人材育成プログラム)

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    Authorship:Principal investigator  Grant type:Contract research

  • 多様なデータにメタデータを付与できるシステムの開発と複数実データセットへの適用

    2020.4 - 2021.3

    Research commissions

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  • Exploring the Magnetosphere-Ionosphere coupling process: emergence of magnetospheric dynamics

    Grant number:20H01961  2020 - 2022

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (B)

    吉川 顕正, Ohtani Shinichi, 中溝 葵

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    地球電離圏はその強磁場弱電離気体系としての特有のダイナミクスを有し、磁気圏ダイナミクスに大きく影響を及ぼす能動的役割を持つ」と提案、この新概念を実証するために、
    (A) 数値実験による電離圏対流変調効果など、 MI結合の結果電離圏に発現する現象の磁気圏構造/ダイナミクスへの影響の抽出
    (B) データ解析によるオーロラ間近接相互作用をもたらす電離圏独自の局所ダイナミクスの解明を目的とした研究を遂行し、MI系ダイナミクスの理解深化へ向け、旧来の固定観念を刷新、
    (C)それらを包括的に記述する多圏間結合系プラズマ力学の一般化と結合理論の構築をつうじて、宇宙惑星科学の基盤となる学術の進展に貢献する。

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  • MAGDAS/CPMNプロジェクト

    2020

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  • 地磁気観測記録装置の導入

    2020

    九州大学研究環境整備事業(キャンパス整備事業等経費)

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  • 多様なデータにメタデータを付与できるシステムの開発と複数実データセットへの適用

    2019.4 - 2020.3

    Research commissions

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  • IUGONETメタデータデータベースの保守・更新、及び、システムの改良

    2019.4 - 2020.3

    Research commissions

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  • Schumann Resonance for monitoring of ionosphere

    Grant number:19K03956  2019 - 2022

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

    Ikeda Akihiro

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    We examined Schumann Resonance (SR) measured by an induction magnetometer at Kuju, Japan. The periodicity of SR parameters is dominant at about 360 and 180 days. The 27-days period, which corresponds to the solar rotational period, also can be seen. The daily variation of SR amplitudes corresponded with the thunderstorm activity in Africa, Asia, North America, and South America. We further found the SR frequency well correlated with EUV flux for long period.
    Variations of SR frequency often associated with solar flares. Since X-ray and EUV of flares enhance the ionization of Earth's ionosphere, the variation of the SR frequency seems to reflect the electron density in the ionospheric D-region. For SPEs (solar proton events), the variation of the SR frequency in eastward component corresponded with enhancement of the Proton flux. We conclude that SR reflects conditions of the lower ionosphere during the intense solar activity.

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  • MAGDAS/CPMNプロジェクト

    2019

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  • IUGONETメタデータデータベースの保守・更新、及び、システムの改良

    2018.4 - 2019.3

    Research commissions

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 磁気赤道多点稠密観測に基づく電離圏赤道ジェット電流の面的時空間構造発展の研究

    2018 - 2020

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • PBIの理論構築

    2017.4 - 2019.3

    Joint research

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  • IUGONETメタデータデータベースの保守・更新、及び、システムの改良

    2017.4 - 2018.3

    Research commissions

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  • 赤道域地磁気変動の稠密観測に基づく太陽地球環境変動モニタリングシステムの開発

    2017 - 2019

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • 理論・数値実験・データ解析に基づく全球カウリングチャンネルの演繹的・実証的解明

    2017 - 2019

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • Composite study on Magnetosphere-Ionosphere Coupling by using MAGDAS and SWARM satellite

    2017 - 2018

    大学・部局間国際交流協定等推進事業:外国人教員招聘

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • MAGDAS/CPMNプロジェクト

    2017

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  • 磁気赤道稠密観測網の 構築によるEEJ研究

    2016.4 - 2019.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 赤道域地磁気変動の稠密観測に基づく太陽地球環境変動モニタリングシステムの開発

    2016 - 2018

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • 極域から磁気赤道域を連結する全球Cowlingチャンネルの実証的研究

    2016 - 2018

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • Seismoelectromagnetics of the Moro Gulf Quake project

    2016 - 2017

    大学・部局間国際交流協定等推進事業:外国人教員招聘

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  • MAGDASデータを用いた太陽活動と地殻変動現象の関連性について

    2016

    Japan Society for the Promotion of Science  JASSO帰国外国人留学生短期研究制度

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    Authorship:Principal investigator  Grant type:Joint research

  • MAGDAS/CPMNプロジェクト

    2016

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  • 留学生獲得のための海外プロモーション

    2016

    スーパーグローバル創成大学支援事業

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  • 超多点地上ネットワーク観測データ解析による電離圏極域-磁気赤道域電磁結合メカニズムの解明

    2015.4 - 2016.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 地球電磁気圏擾乱現象の発生機構の解明と予測

    Grant number:15H05815  2015 - 2020

    Japan Society for the Promotion of Science・Ministry of Education, Culture, Sports, Science and Technology  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research on Innovative Areas (Research in a proposed research area)

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    Authorship:Coinvestigator(s)  Grant type:Scientific research funding

  • 地球電磁気圏擾乱現象の発生機構の解明と予測

    Grant number:15H05815  2015 - 2019

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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  • PBI研究の新展開

    2015 - 2018

    国際宇宙天気科学・教育センター共同利用研究研究費

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  • 衝突系プラズマダイナミクスに基づく全球Cowlingチャンネルの実証的研究

    2015 - 2017

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • Studies on global aspects of Storm Sudden Commencement

    2015 - 2016

    大学・部局間国際交流協定等推進事業:外国人教員招聘

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  • 太陽地球結合系解明の研究基盤形成(マスタープラン重点課題採択)

    2014.4 - 2024.3

    京都大学・生存圏研究所(日本) 

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    極域、赤道域に大型レーダを配備し、地球規模の磁場・電場多点観測網を整備する事により、極域から赤道域にわたるエネルギー・物質輸送のプロセスを理解する。

  • 極域3次元磁気圏電離圏結合系の再定式

    2014.4 - 2017.3

    Joint research

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  • 宇宙災害予報のためのマグダスインデックス

    2014 - 2018

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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  • 地上衛星融合観測研究による磁気嵐時の放射線増加と大気膨張の更なる解明と予測

    2014 - 2018

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Coinvestigator(s)  Grant type:Scientific research funding

  • 極域から磁気赤道域までを結合する全球Cowlingチャンネルの実証的研究

    2014 - 2017

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • 衛星地上融合観測研究による磁気嵐時の放射線増加の更なる解明と予測

    2014 - 2016

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Coinvestigator(s)  Grant type:Scientific research funding

  • FM-CWレーダを用いた赤道域電場変動の全球的研究

    2014 - 2016

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Coinvestigator(s)  Grant type:Scientific research funding

  • 宙空・気象現象と結合した電離圏電磁擾乱の水平・鉛直伝播機構の解明

    2014 - 2016

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • 極冠オーロラ発生機構に関する理論・観測融合研究

    2014 - 2016

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Coinvestigator(s)  Grant type:Scientific research funding

  • 3次元電離圏に於けるCowling チャンネル生成機構の解明

    2014

    情報システム研究機構国際交流プログラム“研究者交流”

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    Authorship:Principal investigator  Grant type:Contract research

  • MAGDAS/CPMN多点ネットワーク観測による全球結合系に於けるエネルギー・物質輸送の解明 International coauthorship

    2013.6 - 2022.3

    九州大学(日本) 

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    Authorship:Principal investigator 

    地球規模の磁場・電場多点観測網を整備する事により、ジオスペースにおける様々な擾乱現象の解明を行う

  • 超多点地上ネットワークデータ解析による電離圏極域−磁気赤道域電磁結合メカニズムの解明

    2013.4 - 2015.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 国際連合・日本合同宇宙天気ワークショップ2015の開催

    2013 - 2014

    情報システム研究機構国際交流プログラム“国際研究集会開催支援”

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    Authorship:Principal investigator  Grant type:Contract research

  • 全球結合系に関する論文執筆

    2013

    九州大学研究者招聘・派遣プログラム

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • 全球Cowlingチャンネルの実証的研究 International coauthorship

    2012.4 - 2022.3

    九州大学(日本) 

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    Authorship:Principal investigator 

    太陽活動現象と同期して発現する、極域から磁気赤道域を連結する全球Cowling電流系の存在を理論・数値実験・データ解析のそれぞれの立場から実証的に検証するプロジェクトである。
    吉川は理論研究と観測ネットワークのコーディネーションを主担として、本プロジェクトを統括する。

  • EISCAT/SuperDARNレーダーを用いたCowlingチャンネル検出手法の検討

    2012.4 - 2014.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 放射線帯形成を促す内部磁気圏複雑系の創発的特性

    Grant number:2340019  2012 - 2014

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (B)

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    Authorship:Coinvestigator(s)  Grant type:Scientific research funding

  • 電磁流体・粒子連結シミュレーションによる地球放射線帯ダイナミクスの研究

    Grant number:24340119  2012 - 2014

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • 国際宇宙天気キャパシティビルディングの形成

    2012 - 2014

    Japan Society for the Promotion of Science  Multilateral program

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    Authorship:Principal investigator  Grant type:Joint research

  • International workshop on global ionospheric dynamics

    2012 - 2014

    国際宇宙天気科学・教育センター共同利用研究研究費

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • 極域における電離圏パラメータの非線形発展:モデル化と検証II

    2011.4 - 2012.3

    Joint research

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    Authorship:Coinvestigator(s)  Grant type:Other funds from industry-academia collaboration

  • 大気大循環モデルと超多点磁場観測データによる大気圏電離圏協調現象の解明

    Grant number:23540513  2011 - 2013

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • 磁気圏MHDシミュレータの為の電離圏・大気圏・固体地球系融合結合ソルバーの開発

    2011 - 2012

    Japan Society for the Promotion of Science  Postdoctoral Fellowships for Research Abroad

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    Authorship:Principal investigator  Grant type:Joint research

  • 3次元電離圏に於けるCowling Channel形成過程の解明

    2011

    宙空環境研究センター平成23年度共同利用研究研究費

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • 極域における電離圏パラメータの非線形発展:モデル化と検証

    2010.4 - 2011.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 大規模電離圏電流の観測に基づく太陽圏ー磁気圏ー電離圏ー大気圏結合過程の研究

    Grant number:22253007  2010 - 2012

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • EMF駆動型磁気圏電離圏結合シミュレータによる全球Cowlingチャンネルの解明

    Grant number:22540460  2010 - 2012

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • 超高層大気長期変動の全球地上ネットワーク観測・研究(IUGONET)

    2009.4 - 2022.3

    東北大学(日本) 国立極研究所(日本) 名古屋大学(日本) 京都大学(日本) 九州大学(日本) 

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    Authorship:Collaborating Investigator(s) (not designated on Grant-in-Aid) 

    IUGONETは超高層大気を取得している5研究機関が連携して、観測データからメタデータを抽出するための、システム、ソフトウエアを開発しするとともに、全球規模で起こる超高層大気諸現象の解明に貢献する研究推進基盤の構築と共に、分野横断的な研究の促進を目指します。

  • Hall共役電流を用いたCowling効果解析手法の開発

    2009.4 - 2011.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 太陽地球/惑星系統合型モデル・シミュレータ構築に向けた研究集会

    2009.4 - 2010.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 3次元電離圏に於けるCowling Channel形成過程の解明

    2009 - 2010

    宙空環境研究センター平成21-22年度共同利用研究研究費

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • 木星探査プロジェクト International coauthorship

    2008.5 - 2013.5

    JAXA/ISAS(日本) 

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    Authorship:Coinvestigator(s) 

    JAXA/ESA共同で打ち上げる予定の木星探査衛星に於ける科学的探査についてのプロジェクトチームである。

  • 太陽地球/惑星系統合型モデル・シミュレータ構築に向けた研究集会

    2008.4 - 2009.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • マグダス環太平洋地磁気ネットワークデータベース

    2008

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Coinvestigator(s)  Grant type:Scientific research funding

  • 3次元電離圏に於けるCowling Channel形成過程の解明

    2008

    宙空環境研究センター平成20年度共同利用研究研究費

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • 3次元電離圏に於けるCowling Channel形成過程の解明

    2007.4 - 2009.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • スイス国際宇宙科学研究所「国際科学者チーム」:Study for Inductive-3D Ionosphere International coauthorship

    2007.4 - 2008.3

    Switzerland 

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    Authorship:Coinvestigator(s) 

    宇宙科学に携わる、新進気鋭の研究者10名が、2005-2006年度にかけて、スイス宇宙科学研究所に終結し、各年度2週間ずつの集中meetingを行い、未だ未知領域である電離圏三次元構造の誘導的な振る舞いを調べる為の研究方策を策定し、その成果を文献としてまとめ将来の方向性を世に問う為のプロジェクトである。2007年度はこの成果報告作成の為の編集会議を行った。

  • ULFレンジで駆動される磁気圏ー電離圏ー熱圏結合シミュレータの開発

    2007 - 2008

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • マグダス環太平洋地磁気ネットワークデータベース

    2007

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Publication of Scientific Research Results

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    Authorship:Coinvestigator(s)  Grant type:Scientific research funding

  • 統合型多圏間シミュレータの開発

    2007

    宙空環境研究センター平成19年度共同利用研究研究費

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • 磁気嵐シミュレータ実現に向けた検討会

    2006.4 - 2007.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 組織化された地上磁場ネットワークデータと統合されたジオスペースシミュレータの開発

    2006 - 2008

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (B)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • 環太平洋ネットワーク観測による宙空領域へのエネルギー・物質流入過程の研究

    Grant number:18253005  2006 - 2008

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • マグダス環太平洋地磁気ネットワークデータベース

    2006

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Publication of Scientific Research Results

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    Authorship:Coinvestigator(s)  Grant type:Scientific research funding

  • 統合型多圏間シミュレータの開発

    2006

    宙空環境研究センター平成18年度共同利用研究研究費

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • 磁気嵐シミュレータ実現に向けた検討会

    2005.4 - 2006.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 地上磁場による三次元電流系推定アルゴリズムの開発

    2005.3 - 2006.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • サブストーム電流系形成メカニズムの評価

    2005

    宙空環境研究センター平成17年度共同利用研究研究費

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • リアルタイム宇宙天気シミュレータの開発

    2004.4 - 2010.3

    九州大学(日本) 

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    Authorship:Coinvestigator(s) 

    太陽監視衛星によって取得された、太陽風データを入力値として、地球磁気圏の擾乱現象をリアルタイムで再現する宇宙天気シミュレータを開発する

  • サブストーム電流系形成メカニズムの研究

    2004.3 - 2005.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • リアルタイム宇宙天気シミュレーション

    2004 - 2009

    Special Coordination Fund for Promoting Science and Technology (Ministry of Education, Culture, Sports, Science and Technology)

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    Authorship:Coinvestigator(s)  Grant type:Contract research

  • 松本研究奨励資金(若手研究者招聘)

    2004

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    Grant type:Donation

  • 米国地球物理学連合、Chapman conference(サンディエゴ、カルフォルニア)への出席補助(議長、招待講演)

    2004

    財団法人九州大学後援会国際研究集会派遣助成

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • サブストーム電流系形成メカニズムの評価

    2004

    宙空環境研究センター平成16年度共同利用研究研究費

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • 沿磁力線電流、Sqダイナモ効果を繰り込りだ電離層電流の全球過渡応答モデルの開発

    Grant number:15740298  2003 - 2005

    Grants-in-Aid for Scientific Research  Grant-in-Aid for Young Scientists (B)

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    Grant type:Scientific research funding

  • 太陽風から磁気赤道領域までのエネルギー・物質流入過程に伴う宙空環境変動の研究

    Grant number:15253005  2003 - 2005

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • 水星探査プロジェクト共同研究 International coauthorship

    2002.5 - 2013.5

    JAXA/ISAS(日本) 

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    Authorship:Coinvestigator(s) 

    JAXA/ESA共同で打ち上げる予定の水星探査衛星「BeppiColombo」に於ける科学的探査についてのプロジェクトチームである。

  • オーロラ形成に於ける発散性ホール電流の役割に関する研究

    2002.4 - 2004.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • グローバルな宙空環境変動観測記録システムの開発

    Grant number:13554016  2001 - 2003

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • The nature of reflection and mode conversion of MHD waves at the inductive ionosphere: Multistep mode conversion between divergent and rotational electric fields

    2001

    第一回 九州大学総長賞(研究奨励金):

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    Authorship:Principal investigator  Grant type:Contract research

  • 極域・磁気赤道域を含む磁気圏-電離圏結合の理論的研究

    2000.4 - 2002.3

    Joint research

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    Authorship:Principal investigator  Grant type:Other funds from industry-academia collaboration

  • 太陽風-地球磁気圏相互作用によるエネルギーの侵入・結合・変換過程の研究

    Grant number:12373003  2000 - 2002

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • 磁気圏-電離圏-中性大気-固体地球 電磁気的結合系の理論的研究

    2000 - 2001

    Grants-in-Aid for Scientific Research  Grant-in-Aid for Encouragement of Scientists (B)

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    Authorship:Principal investigator  Grant type:Scientific research funding

  • 大規模電磁場擾乱の極冠域から赤道域への侵入・伝播過程

    Grant number:10440137  1998 - 2001

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • 磁気圏―電離圏―中性大気層―固体地球電磁結合系での地磁気脈動

    Grant number:10740233  1998 - 1999

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • 南大西洋域磁気異常帯での超高層現象の研究

    Grant number:09874094  1997 - 1999

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

  • インターネットを通じた大学研究情報公開のあり方に関する研究

    1997

    九州大学総長特別経費

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    Authorship:Principal investigator  Grant type:On-campus funds, funds, etc.

  • MAGDAS/CPMN多点ネットワーク観測による地球磁気圏の研究

    1996.4 - 2022.5

    九州大学(日本) 

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    Authorship:Coinvestigator(s) 

    地球規模の磁場・電場多点観測網を整備する事により、ジオスペースにおける様々な擾乱現象の解明を行う

  • 太陽風変動に伴う擾乱の極域から赤道域への侵入・輸送過程の研究

    Grant number:08041105  1996 - 1997

    Japan Society for the Promotion of Science  Grants-in-Aid for Scientific Research  Grant-in-Aid for Scientific Research (C)

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    Grant type:Scientific research funding

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Educational Activities

  • 現在、地球惑星科学部門に於いて、物理学実験、数理科学関係の演習、宇宙空間科学に関する講義を担当している。所属研究室においては、4年生、大学院生の研究活動を支援し、共同研究を行っている。大学院教育においては、博士課程の学生8名、修士課程学生13名を主指導している。
    また国際宇宙惑星環境研究センター(センタ−長)に於いて宇宙天気科学に関する部局間を跨いだ教育研究活動を行っている。センターでの学術活動を学府の大学院教育に活用するとともに、海外からの若手研究者の短期受け入れを積極的に行い、九大の学生との交流活動にも活用している。当センターに於いては、大学の制度を活用し、過去3年連続で、海外からの准教授を雇用、センタープロジェクトの遂行、学生の教育に活用している。
    また、2011年からは国連と共同で世界中の若手研究者を対象とした、国際的なキャパシティ・ビルディング活動を開始しており、2012年からはJSPS学術基盤形成のPIとして本活動を推進しており、各種国際学校の主催、共催、講師参加などにも積極的に取り組んでいる。

Class subject

  • 太陽惑星系物理学

    2024.10 - 2025.3   Second semester

  • Solar Planetary System Physics

    2024.10 - 2025.3   Second semester

  • 基幹教育セミナー

    2024.6 - 2024.8   Summer quarter

  • 宙空物理学

    2024.4 - 2024.9   First semester

  • 宇宙科学概論

    2024.4 - 2024.9   First semester

  • 地学通論

    2024.4 - 2024.9   First semester

  • Solar Planetary System Physics

    2023.10 - 2024.3   Second semester

  • 地球惑星科学特別講義Ⅰ

    2023.10 - 2024.3   Second semester

  • 太陽惑星系物理学

    2023.10 - 2024.3   Second semester

  • 電磁気学基礎演習

    2023.10 - 2023.12   Fall quarter

  • 宙空物理学

    2023.4 - 2023.9   First semester

  • 宇宙科学概論

    2023.4 - 2023.9   First semester

  • 地学通論

    2023.4 - 2023.9   First semester

  • 太陽惑星系物理学

    2022.10 - 2023.3   Second semester

  • 電磁気学基礎演習

    2022.10 - 2022.12   Fall quarter

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2022.4 - 2022.9   First semester

  • 宇宙科学概論

    2022.4 - 2022.9   First semester

  • 宙空物理学

    2022.4 - 2022.9   First semester

  • 地学通論

    2022.4 - 2022.9   First semester

  • 地球惑星科学基礎実験

    2022.4 - 2022.9   First semester

  • 九州大学で学ぶ宇宙科学技術

    2022.4 - 2022.9   First semester

  • 太陽惑星系物理学

    2021.10 - 2022.3   Second semester

  • 基幹教育セミナー

    2021.6 - 2021.8   Summer quarter

  • 基幹教育セミナー

    2021.6 - 2021.8   Summer quarter

  • 宙空物理学

    2021.4 - 2021.9   First semester

  • 地球惑星科学基礎実験

    2021.4 - 2021.9   First semester

  • 宇宙科学概論

    2021.4 - 2021.9   First semester

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2021.4 - 2021.9   First semester

  • 宇宙科学概論

    2021.4 - 2021.9   First semester

  • 宙空物理学

    2021.4 - 2021.9   First semester

  • 地球惑星科学基礎実験

    2021.4 - 2021.9   First semester

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2021.4 - 2021.9   First semester

  • 九州大学で学ぶ宇宙科学技術

    2021.4 - 2021.9   First semester

  • 太陽惑星系物理学

    2020.10 - 2021.3   Second semester

  • 基幹教育セミナー

    2020.6 - 2020.8   Summer quarter

  • 基幹教育セミナー

    2020.6 - 2020.8   Summer quarter

  • 宙空物理学

    2020.4 - 2020.9   First semester

  • 宇宙科学概論

    2020.4 - 2020.9   First semester

  • 宙空物理学

    2020.4 - 2020.9   First semester

  • 地球惑星科学基礎実験

    2020.4 - 2020.9   First semester

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2020.4 - 2020.9   First semester

  • 九州大学で学ぶ宇宙科学技術

    2020.4 - 2020.9   First semester

  • 地球惑星科学基礎実験

    2020.4 - 2020.9   First semester

  • 基幹教育セミナー

    2020.4 - 2020.9   First semester

  • 太陽惑星系物理学

    2020.4 - 2020.9   First semester

  • 基幹物理学ⅠB演習

    2019.10 - 2020.3   Second semester

  • 太陽惑星系物理学

    2019.10 - 2020.3   Second semester

  • 地球惑星科学特別講義Ⅲ

    2019.4 - 2019.9   First semester

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2019.4 - 2019.9   First semester

  • 九州大学で学ぶ宇宙科学技術

    2019.4 - 2019.9   First semester

  • 地球惑星物理学実験

    2019.4 - 2019.9   First semester

  • 地球惑星科学Ⅰ

    2019.4 - 2019.9   First semester

  • 宙空物理学

    2019.4 - 2019.9   First semester

  • 基幹物理学ⅠB演習

    2018.10 - 2019.3   Second semester

  • 太陽惑星系物理学

    2018.10 - 2019.3   Second semester

  • 宇宙科学概論

    2018.4 - 2018.9   First semester

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2018.4 - 2018.9   First semester

  • 九州大学で学ぶ宇宙科学技術

    2018.4 - 2018.9   First semester

  • 宙空物理学

    2018.4 - 2018.9   First semester

  • 地球惑星物理学実験

    2018.4 - 2018.9   First semester

  • 太陽惑星系物理学

    2017.10 - 2018.3   Second semester

  • 地球惑星科学演習V

    2017.10 - 2018.3   Second semester

  • 地球惑星科学演習II

    2017.10 - 2018.3   Second semester

  • 基幹物理学ⅠB演習

    2017.10 - 2018.3   Second semester

  • 地球惑星科学特別研究I

    2017.4 - 2018.3   Full year

  • 地球惑星科学特別講究

    2017.4 - 2018.3   Full year

  • 地球惑星科学特別研究

    2017.4 - 2018.3   Full year

  • 地球惑星物理学実験

    2017.4 - 2017.9   First semester

  • 地球惑星科学演習III

    2017.4 - 2017.9   First semester

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2017.4 - 2017.9   First semester

  • 地球惑星科学I

    2017.4 - 2017.9   First semester

  • 宇宙科学概論

    2017.4 - 2017.9   First semester

  • 宙空物理学

    2017.4 - 2017.9   First semester

  • 地球惑星科学演習V

    2016.10 - 2017.3   Second semester

  • 地球惑星科学演習II

    2016.10 - 2017.3   Second semester

  • 地球惑星科学特別講究

    2016.4 - 2017.3   Full year

  • 地球惑星科学特別研究I

    2016.4 - 2017.3   Full year

  • 地球惑星科学特別研究

    2016.4 - 2017.3   Full year

  • 地球惑星科学演習III

    2016.4 - 2016.9   First semester

  • 宇宙科学概論

    2016.4 - 2016.9   First semester

  • 地球惑星物理学実験(電磁気学実験)

    2016.4 - 2016.9   First semester

  • 地球惑星科学I

    2016.4 - 2016.9   First semester

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2016.4 - 2016.9   First semester

  • 宙空物理学

    2016.4 - 2016.9   First semester

  • 太陽惑星系物理学

    2016.4 - 2016.9   First semester

  • 地球惑星科学演習II

    2015.10 - 2016.3   Second semester

  • 地球惑星科学演習V

    2015.10 - 2016.3   Second semester

  • 地球惑星科学特別研究

    2015.4 - 2016.3   Full year

  • 地球惑星科学特別講究

    2015.4 - 2016.3   Full year

  • 地球惑星科学特別研究I

    2015.4 - 2016.3   Full year

  • 地球惑星科学演習III

    2015.4 - 2015.9   First semester

  • 宇宙科学概論

    2015.4 - 2015.9   First semester

  • 地球惑星科学I

    2015.4 - 2015.9   First semester

  • 太陽惑星系物理学

    2015.4 - 2015.9   First semester

  • 宙空物理学

    2015.4 - 2015.9   First semester

  • 地球惑星物理学実験(電磁気学実験)

    2015.4 - 2015.9   First semester

  • 宇宙電磁力学

    2015.4 - 2015.9   First semester

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2015.4 - 2015.9   First semester

  • 地球惑星科学演習II

    2014.10 - 2015.3   Second semester

  • 地球惑星科学演習V

    2014.10 - 2015.3   Second semester

  • 地球惑星科学特別講究

    2014.4 - 2015.3   Full year

  • 地球惑星科学特別研究I

    2014.4 - 2015.3   Full year

  • 地球惑星科学特別研究

    2014.4 - 2015.3   Full year

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2014.4 - 2014.9   First semester

  • 宇宙科学概論

    2014.4 - 2014.9   First semester

  • 地球惑星科学I

    2014.4 - 2014.9   First semester

  • 太陽惑星系物理学

    2014.4 - 2014.9   First semester

  • 地球惑星物理学実験(電磁気学実験)

    2014.4 - 2014.9   First semester

  • 宙空物理学

    2014.4 - 2014.9   First semester

  • 地球惑星科学演習III

    2014.4 - 2014.9   First semester

  • 宇宙電磁力学

    2014.4 - 2014.9   First semester

  • 地球惑星科学演習II

    2013.10 - 2014.3   Second semester

  • 地球惑星科学演習V

    2013.10 - 2014.3   Second semester

  • 地球惑星特別研究

    2013.4 - 2014.3   Full year

  • 地球惑星科学特別講究

    2013.4 - 2014.3   Full year

  • 地球惑星科学特別研究

    2013.4 - 2014.3   Full year

  • 地球惑星科学特別研究I

    2013.4 - 2014.3   Full year

  • 地球惑星物理学実験(電磁気学実験)

    2013.4 - 2013.9   First semester

  • 地球惑星数理解析演習(球面調和関数解析担当)

    2013.4 - 2013.9   First semester

  • 宇宙電磁力学

    2013.4 - 2013.9   First semester

  • 地球惑星科学演習III

    2013.4 - 2013.9   First semester

  • 宇宙科学概論

    2013.4 - 2013.9   First semester

  • 宙空物理学

    2013.4 - 2013.9   First semester

  • 地球惑星科学演習II

    2012.10 - 2013.3   Second semester

  • 地球惑星科学演習V

    2012.10 - 2013.3   Second semester

  • 地球惑星特別研究

    2012.4 - 2013.3   Full year

  • 地球惑星科学特別講究

    2012.4 - 2013.3   Full year

  • 地球惑星科学特別研究

    2012.4 - 2013.3   Full year

  • 地球惑星科学特別研究I

    2012.4 - 2013.3   Full year

  • コアセミナー(太陽について調べよう)

    2012.4 - 2012.9   First semester

  • 宇宙電磁力学

    2012.4 - 2012.9   First semester

  • 地球惑星科学演習III

    2012.4 - 2012.9   First semester

  • 宇宙科学概論

    2012.4 - 2012.9   First semester

  • 宙空物理学

    2012.4 - 2012.9   First semester

  • 地球惑星物理学実験(電磁気学実験)

    2012.4 - 2012.9   First semester

  • 地球惑星数理解析演習(Fourier解析、球面調和関数解析担当)

    2012.4 - 2012.9   First semester

  • 地球惑星科学演習II

    2011.10 - 2012.3   Second semester

  • 地球惑星科学演習V

    2011.10 - 2012.3   Second semester

  • 地球惑星特別研究

    2011.4 - 2012.3   Full year

  • 地球惑星科学特別講究

    2011.4 - 2012.3   Full year

  • 地球惑星科学特別研究

    2011.4 - 2012.3   Full year

  • 地球惑星科学特別研究I

    2011.4 - 2012.3   Full year

  • 地球惑星物理学実験(電磁気学実験)

    2011.4 - 2011.9   First semester

  • 太陽惑星系物理学

    2011.4 - 2011.9   First semester

  • 宇宙電磁力学

    2011.4 - 2011.9   First semester

  • 地球惑星数理解析演習(ベクトル・テンソル解析担当)

    2011.4 - 2011.9   First semester

  • 地球惑星科学演習III

    2011.4 - 2011.9   First semester

  • 電磁流体力学

    2011.4 - 2011.9   First semester

  • 地球惑星科学演習II

    2010.10 - 2011.3   Second semester

  • 地球惑星科学演習V

    2010.10 - 2011.3   Second semester

  • 地球惑星特別研究

    2010.4 - 2011.3   Full year

  • 地球惑星科学特別講究

    2010.4 - 2011.3   Full year

  • 地球惑星科学特別研究

    2010.4 - 2011.3   Full year

  • 地球惑星科学特別演習I

    2010.4 - 2011.3   Full year

  • 地球惑星科学特別研究I

    2010.4 - 2011.3   Full year

  • 宇宙電磁力学

    2010.4 - 2010.9   First semester

  • 太陽惑星系物理学

    2010.4 - 2010.9   First semester

  • 地球惑星科学演習III

    2010.4 - 2010.9   First semester

  • 電磁流体力学

    2010.4 - 2010.9   First semester

  • コアセミナー(オーロラの動態を探る)

    2010.4 - 2010.9   First semester

  • 地球惑星物理学実験(電磁気学実験)

    2010.4 - 2010.9   First semester

  • 地球惑星数理解析演習(ベクトル・テンソル解析担当)

    2010.4 - 2010.9   First semester

  • 地球惑星科学演習V

    2009.10 - 2010.3   Second semester

  • 地球惑星物理学演習I(熱力学担当)

    2009.10 - 2010.3   Second semester

  • 宇宙電磁力学

    2009.10 - 2010.3   Second semester

  • 地球惑星科学演習II

    2009.10 - 2010.3   Second semester

  • 地球惑星科学特別講究

    2009.4 - 2010.3   Full year

  • 地球惑星特別研究

    2009.4 - 2010.3   Full year

  • 地球惑星科学特別研究I

    2009.4 - 2010.3   Full year

  • 地球惑星科学特別演習I

    2009.4 - 2010.3   Full year

  • 地球惑星科学特別研究

    2009.4 - 2010.3   Full year

  • 地球惑星科学演習III

    2009.4 - 2009.9   First semester

  • 電磁流体力学

    2009.4 - 2009.9   First semester

  • 地球惑星物理学実験(電磁気学実験)

    2009.4 - 2009.9   First semester

  • 地球惑星科学演習V

    2008.10 - 2009.3   Second semester

  • 地球惑星科学演習I (数理解析演習)

    2008.10 - 2009.3   Second semester

  • 地球惑星科学演習II

    2008.10 - 2009.3   Second semester

  • 地球惑星科学特別講究

    2008.4 - 2009.3   Full year

  • 地球惑星特別研究

    2008.4 - 2009.3   Full year

  • 地球惑星科学特別研究I

    2008.4 - 2009.3   Full year

  • 地球惑星科学特別演習I

    2008.4 - 2009.3   Full year

  • 地球惑星科学特別研究

    2008.4 - 2009.3   Full year

  • 地球惑星数理演習

    2008.4 - 2008.9   First semester

  • 地球惑星科学実験 マイコン制御実験

    2008.4 - 2008.9   First semester

  • 地球惑星科学実習I・II 宇宙空間観測所実習

    2008.4 - 2008.9   First semester

  • 地球惑星科学演習III

    2008.4 - 2008.9   First semester

  • 宇宙空間物理学

    2008.4 - 2008.9   First semester

  • 宇宙電磁力学

    2008.4 - 2008.9   First semester

  • 地球惑星物理学実験(宇宙天気概況解析実験)

    2007.10 - 2008.3   Second semester

  • 地球惑星科学演習V

    2007.10 - 2008.3   Second semester

  • 地球惑星科学演習II

    2007.10 - 2008.3   Second semester

  • 地球惑星科学演習I (数理解析演習)

    2007.10 - 2008.3   Second semester

  • 地球惑星特別研究

    2007.4 - 2008.3   Full year

  • 地球惑星科学特別講究

    2007.4 - 2008.3   Full year

  • 地球惑星科学特別研究

    2007.4 - 2008.3   Full year

  • 地球惑星科学特別演習I

    2007.4 - 2008.3   Full year

  • 地球惑星科学特別研究I

    2007.4 - 2008.3   Full year

  • 地球惑星科学実験 マイコン制御実験

    2007.4 - 2007.9   First semester

  • 地球惑星数理演習

    2007.4 - 2007.9   First semester

  • 地球惑星科学演習III

    2007.4 - 2007.9   First semester

  • 地球惑星科学実習I・II 宇宙空間観測所実習

    2007.4 - 2007.9   First semester

  • 地球惑星科学演習V

    2006.10 - 2007.3   Second semester

  • 地球惑星物理学実験(宇宙天気概況解析実験)

    2006.10 - 2007.3   Second semester

  • 地球惑星科学演習I (数理解析演習)

    2006.10 - 2007.3   Second semester

  • 地球惑星科学演習II

    2006.10 - 2007.3   Second semester

  • 地球惑星科学特別講究

    2006.4 - 2007.3   Full year

  • 地球惑星特別研究

    2006.4 - 2007.3   Full year

  • 地球惑星科学特別研究I

    2006.4 - 2007.3   Full year

  • 地球惑星科学特別演習I

    2006.4 - 2007.3   Full year

  • 地球惑星科学特別研究

    2006.4 - 2007.3   Full year

  • 地球惑星数理演習

    2006.4 - 2006.9   First semester

  • 地球惑星科学実験 マイコン制御実験

    2006.4 - 2006.9   First semester

  • 地球惑星科学実習I・II 宇宙空間観測所実習

    2006.4 - 2006.9   First semester

  • 地球惑星科学演習III

    2006.4 - 2006.9   First semester

  • 地球惑星科学演習 数理解析演習

    2005.10 - 2006.3   Second semester

  • 地球惑星物理学実験I (宇宙天気概況解析実験)

    2005.4 - 2005.9   First semester

  • 地球惑星科学実習I(宇宙空間観測所実習)

    2005.4 - 2005.9   First semester

  • 地球惑星物理学実験II(マイコン制御実験)

    2005.4 - 2005.9   First semester

  • 地球惑星科学演習 数理解析演習

    2004.10 - 2005.3   Second semester

  • 地球惑星物理学実験I (電磁気回路実験)

    2004.10 - 2005.3   Second semester

  • 地球惑星物理学実験II(マイコン制御実験)

    2004.4 - 2004.9   First semester

  • 地球惑星科学実習I(宇宙空間観測所実習)

    2004.4 - 2004.9   First semester

  • 地球惑星物理学実験II(マイコン制御実験)

    2003.10 - 2004.3   Second semester

  • 地球惑星科学実習I(宇宙空間観測所実習)

    2003.4 - 2003.9   First semester

  • 地球惑星物理学実験I (電磁気回路実験)

    2003.4 - 2003.9   First semester

  • 地球惑星物理学実験II(マイコン制御実験)

    2002.10 - 2003.3   Second semester

  • 地球惑星科学実習I(宇宙空間観測所実習)

    2002.4 - 2002.9   First semester

  • 地球惑星物理学実験I (電磁気回路実験)

    2002.4 - 2002.9   First semester

  • 太陽惑星系物理学

    2024.10 - 2025.3   Second semester

  • 地球惑星科学演習Ⅴ

    2024.10 - 2025.3   Second semester

  • Solar Planetary System Physics

    2024.10 - 2025.3   Second semester

  • Research Seminar Ⅱ

    2024.10 - 2025.3   Second semester

  • 基幹教育セミナー

    2024.6 - 2024.8   Summer quarter

  • 地球惑星科学特別研究Ⅱ(2年)(9月卒業)

    2024.4 - 2025.3   Full year

  • 地球惑星科学特別研究Ⅱ(2年)

    2024.4 - 2025.3   Full year

  • 地球惑星科学特別研究Ⅰ(1年)

    2024.4 - 2025.3   Full year

  • 地球惑星科学特別研究

    2024.4 - 2025.3   Full year

  • MSc.Thesis Research

    2024.4 - 2025.3   Full year

  • 宙空物理学

    2024.4 - 2024.9   First semester

  • 宇宙科学概論

    2024.4 - 2024.9   First semester

  • 地球惑星科学演習Ⅲ

    2024.4 - 2024.9   First semester

  • 地学通論

    2024.4 - 2024.9   First semester

  • Research Seminar Ⅰ

    2024.4 - 2024.9   First semester

  • Literature Survey

    2024.4 - 2024.9   First semester

▼display all

FD Participation

  • 2010.11   Role:Planning   Title:ゆとり教育世代の新入生の理数系基礎学力

    Organizer:Undergraduate school department

  • 2008.8   Role:Speech   Title:学部新カリキュラム 実験・実習について

    Organizer:Undergraduate school department

  • 2007.7   Role:Participation   Title:地球惑星科学科の新しいカリキュラムについて

    Organizer:Undergraduate school department

  • 2002.11   Role:Participation   Title:必修実験を考える

    Organizer:Undergraduate school department

  • 2001.11   Role:Speech   Title:実習を考える

    Organizer:Undergraduate school department

  • 2000.11   Role:Speech   Title:選択実験を考える

    Organizer:Undergraduate school department

▼display all

Visiting, concurrent, or part-time lecturers at other universities, institutions, etc.

  • 2023  京都大学 大学院理学研究科  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:9/13〜15

  • 2017  マラ工科大学 マレーシア(ジョホールバル)  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:2017年 8月11日-8月13日 2nd National School on EARTH and ELECTROMAGNETISMでの集中講義

  • 2017  Covenant University  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:2017年 9月9日-9月16日 第2回国際赤道・低緯度電離圏に関する国際学校(ISELLI-2)への講師参加

  • 2016  ロシア科学技術アカデミーIKIFIA研究所  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:2016年8月13日~8月17日 COSPAR Capacity Building Workshop:Impact of Space Weather on Earthの招聘講師参加

  • 2016  SMT. KASTURBAI WALCHAND COLLEGE, インド(シャングリ)  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:ICOSTEP/ISWI International School on Space Scienceへの講師参加

  • 2015  ナイジェリア 宇宙科学研究所  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:2015年9月13~20日 International school on equatorial and lo-latitude ionosphereでの招聘講師

  • 2014  インドネシア気象国物理庁  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:9/6〜9インドネシア気象庁(BMKG)での集中講義 計8コマ

  • 2014  ペルー地球物理学研究所  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:9月13〜20日 SCOSTEP/ISWI International Space Science School (ISSS) in Peruでの講師

  • 2014  マレーシア 宇宙科学研究所  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:12/1〜12/6 National school on Space and Earth Electromagnetism (SEE) 2014での集中講義

  • 2013  インドネシア気象国物理庁  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:2013年10月22日から25日、計4回 計6時間

  • 2010  フィンランド気象研究所  Classification:Intensive course  Domestic/International Classification:Overseas 

    Semester, Day Time or Duration:2回、計6時間

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Participation in international educational events, etc.

  • 2018.3

    九州大学 国際宇宙天気科学・教育センター

    Japan-Malaysia Joint Seminar on Space and Earth Electromagnetism 2018の主催、集中講義

      More details

    Venue:日本・福岡市

    Number of participants:20

  • 2017.9

    ナイジェリア国家宇宙研究開発機関

    第2回国際赤道・低緯度電離圏に関する国際学校(ISELLI-2)(ナイジェリア、ラゴス:「磁気圏電離圏結合の基礎」、「磁場データの宇宙天気研究への活用」、「MAGDAS磁力計システムとそのデータ活用」に関する集中講義

      More details

    Venue:ナイジェリア・ラゴス

    Number of participants:150

  • 2017.8

    マラ工科大学

    2nd National School on EARTH and ELECTROMAGNETISMでの基調講演、及び集中講義

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    Venue:マレーシア・ジョホールバル

    Number of participants:150

  • 2016.8

    ロシア科学アカデミーIKIFIA研究所

    COSPAR Capacity Building Workshop:Impact of Space Weather on Earthへの講師参加

      More details

    Venue:ロシア・パラツンカ

    Number of participants:100

  • 2016.2

    ICUS/SCOSTEP

    ICUS/SCOSTEP スクールへの講師参加

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    Venue:インド(シャングリ)

    Number of participants:300

  • 2015.9

    ナイジェリア宇宙科学研究所

    スーパーグローバル大学創成支援派遣を得て、International school on equatorial and lo-latitude ionosphereでの集中講義をおこなった。

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    Venue:ナイジェリア・アブジャ

    Number of participants:120

  • 2014.12

    National Space Agency, Malaysia (ANGKASA)

    National school on Space and Earth Electromagnetism(SEE) 2014にて宇宙天気に関する集中講義を行った。

      More details

    Venue:Langkawi , Malaysia

    Number of participants:20

  • 2014.9

    インドネシア気象庁(BMKG)

    Geomagnetic Workshop in Medanにて宇宙天気研究に関する集中講義を行った。

      More details

    Venue:Indonesia, Medan

    Number of participants:60

  • 2014.9

    ICUS⁄SCOSTEP

    ICUS⁄SCOSTEP⁄ISWI International Space Science School (ISSS) in Peruにて集中講義を行った。

      More details

    Venue:Lima, Peru

    Number of participants:60

  • 2014.2

    国連

    オーストリア・ウィーンで開催された国連宇宙平和利用委員会に於いて、九州大学、国際宇宙天気科学・教育センター設置に関するテクニカル・プレゼンテーションを行った。

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    Venue:オーストリア・ウィーン

    Number of participants:500

  • 2013.9

    国連

    コートジボワール・アブジャで開催された国連ISWI⁄MAGDAS-Internationalスクールをオーガナイザーとして統括し、講師として講演を行った。

      More details

    Venue:コートジボワール・アブジャ

    Number of participants:70

  • 2013.9

    国連、九州大学

    UN/Austria Symposium on “Space Weather Data, Instruments and Models: Looking Beyond the International Space Weather Initiativeをプログラム委員としてオーガナイズし、招待講演を行った

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    Venue:オーストリア・グラーツ

    Number of participants:60

  • 2013.2

    国連

    オーストリア・ウィーンで開催された国連宇宙平和利用委員会に於いて、九州大学の国際的キャパシティ・ビルディング活動に関するテクニカル・プレゼンテーションを行った。

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    Venue:オーストリア・ウィーン

    Number of participants:500

  • 2012.10

    国連、エクアドル外務省

    エクアドル・キトで開催された国連/国際宇宙天気科学イニシアチブ会議にて、九州大学国際宇宙天気科学・教育センターに関するkeynote講演を行った。

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    Venue:エクアドル・キト

    Number of participants:200

  • 2012.9

    国連、九州大学

    オーストリア・グラーツで開催された国連宇宙環境データ解析Internationalスクールに講師として参加し、keynote講演を行った。

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    Venue:オーストリア・グラーツ

    Number of participants:40

  • 2012.9

    国連、九州大学

    インドネシア・バンドンで行われた国連ISWI/MAGDAS-Internationalスクールにオーガナイザー及び講師として参加した。

      More details

    Venue:インドネシア・バンドン

    Number of participants:60

  • 2012.6

    国連

    オーストリア・ウィーンで開催された国連宇宙平和利用委員会に於いて、九州大学、国際宇宙天気科学・教育センター設置に関するテクニカル・プレゼンテーションを行った。

      More details

    Venue:オーストリア・ウィーン

    Number of participants:500

  • 2011.8

    国連、九州大学

    ナイジェリ・アラゴスで行われた国連ISWI-Internationalスクールに講師として参加した。

      More details

    Venue:ナイジェリア・ラゴス

    Number of participants:60

▼display all

Other educational activity and Special note

  • 2024  Special Affairs  研究指導、論文指導を行っている学生(川上航典)が科研費 国際先導研究「国際地上観測網と人工衛星観測網・モデリングに基づくジオスペースの先導研究」の研究アシスタント・リサーチフェロー(R6~R8)として採用された。

     詳細を見る

    研究指導、論文指導を行っている学生(川上航典)が科研費 国際先導研究「国際地上観測網と人工衛星観測網・モデリングに基づくジオスペースの先導研究」の研究アシスタント・リサーチフェロー(R6~R8)として採用された。

  • 2023  Special Affairs  研究指導、論文指導を行っている学生(西村美紀)が次世代研究者挑戦的研究プログラム未来創造コースのコース生に採用された。

     詳細を見る

    研究指導、論文指導を行っている学生(西村美紀)が次世代研究者挑戦的研究プログラム未来創造コースのコース生に採用された。

  • 2023  Special Affairs  研究指導、論文指導を行っている学生(伊集院拓也)が科研費 国際先導研究「国際地上観測網と人工衛星観測網・モデリングに基づくジオスペースの先導研究」の研究アシスタント・リサーチフェロー(R5~R7)として採用された。

     詳細を見る

    研究指導、論文指導を行っている学生(伊集院拓也)が科研費 国際先導研究「国際地上観測網と人工衛星観測網・モデリングに基づくジオスペースの先導研究」の研究アシスタント・リサーチフェロー(R5~R7)として採用された。

  • 2023  Special Affairs  研究指導、論文指導を行っている学生(林萌英)が地球電磁気・地球惑星圏学会において学生優秀発表を受賞した。

     詳細を見る

    研究指導、論文指導を行っている学生(林萌英)が地球電磁気・地球惑星圏学会において学生優秀発表を受賞した。

  • 2023  Special Affairs  九州大学Quriesプログラムに参加し、女子高生の研究指導を行った。

     詳細を見る

    九州大学Quriesプログラムに参加し、女子高生の研究指導を行った。

  • 2023  Special Affairs  研究指導、論文指導を行っている学生(樋口颯人)が2023年度九州大学量子ネイティブシンポジウムにて学生優秀発表賞を受賞した。

     詳細を見る

    研究指導、論文指導を行っている学生(樋口颯人)が2023年度九州大学量子ネイティブシンポジウムにて学生優秀発表賞を受賞した。

  • 2022  Special Affairs  研究指導、論文指導を行っている学生(橋本翼)が次世代研究者挑戦的研究プログラム未来創造コースのコース生に採用された。

     詳細を見る

    研究指導、論文指導を行っている学生(橋本翼)が次世代研究者挑戦的研究プログラム未来創造コースのコース生に採用された。

  • 2022  Special Affairs  研究指導、論文指導を行っている学生(高山久美)が次世代研究者挑戦的研究プログラム未来創造コースのコース生に採用された。

     詳細を見る

    研究指導、論文指導を行っている学生(高山久美)が次世代研究者挑戦的研究プログラム未来創造コースのコース生に採用された。

  • 2022  Special Affairs  研究指導、論文指導を行っている学生(樋口颯人)が、九州大学先導的人材育成フェローシップ(量子分野)に採用された。

     詳細を見る

    研究指導、論文指導を行っている学生(樋口颯人)が、九州大学先導的人材育成フェローシップ(量子分野)に採用された。

  • 2022  Special Affairs  研究指導、論文指導を行っている学生(林萌英)が学術振興会特別研究員(DC1)に選出された

     詳細を見る

    研究指導、論文指導を行っている学生(林萌英)が学術振興会特別研究員(DC1)に選出された

  • 2022  Special Affairs  九州大学Quriesプログラムに参加し、女子高生の研究指導を行った。

     詳細を見る

    九州大学Quriesプログラムに参加し、女子高生の研究指導を行った。

  • 2021  Special Affairs  九州大学Quriesプログラムに参加し、女子高生の研究指導を行った。

     詳細を見る

    九州大学Quriesプログラムに参加し、女子高生の研究指導を行った。

  • 2020  Class Teacher  学部

  • 2019  Class Teacher  学部

  • 2019  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2018  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2017  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2016  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2016  Special Affairs  研究指導、論文指導を行ってきた学生(今城峻)が学術振興会特別研究員(DC2)に選出された

     詳細を見る

    研究指導、論文指導を行ってきた学生(今城峻)が学術振興会特別研究員(DC2)に選出された

  • 2016  Special Affairs  研究指導、論文指導を行ってきた学生(今城峻)が九州大学学生表彰(学術研究活動表彰)を授賞した

     詳細を見る

    研究指導、論文指導を行ってきた学生(今城峻)が九州大学学生表彰(学術研究活動表彰)を授賞した

  • 2015  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2014  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2014  Special Affairs  研究指導、論文指導を行ってきた学生(今城峻)が地球電磁気・地球惑星圏学会においてオーロラメダル賞を受賞した。

     詳細を見る

    研究指導、論文指導を行ってきた学生(今城峻)が地球電磁気・地球惑星圏学会においてオーロラメダル賞を受賞した。

  • 2013  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2012  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2011  Class Teacher  学部

  • 2011  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2010  Class Teacher  学部

  • 2010  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2010  Special Affairs  研究指導、論文指導を行ってきた学生(山崎洋介)が飛び級にて博士課程を修了した。

     詳細を見る

    研究指導、論文指導を行ってきた学生(山崎洋介)が飛び級にて博士課程を修了した。

  • 2009  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2009  Special Affairs  研究指導、論文指導を行ってきた学生(山崎洋介)が学術振興会特別研究員(DC1)に選出された

     詳細を見る

    研究指導、論文指導を行ってきた学生(山崎洋介)が学術振興会特別研究員(DC1)に選出された

  • 2009  Special Affairs  研究指導、論文指導を行ってきた学生(徳永旭将)が地球電磁気・地球惑星圏学会においてオーロラメダル賞を受賞した。

     詳細を見る

    研究指導、論文指導を行ってきた学生(徳永旭将)が地球電磁気・地球惑星圏学会においてオーロラメダル賞を受賞した。

  • 2008  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2008  Special Affairs  研究指導、論文指導を行ってきた学生(徳永旭将)が学術振興会特別研究員(DC1)に選出された

     詳細を見る

    研究指導、論文指導を行ってきた学生(徳永旭将)が学術振興会特別研究員(DC1)に選出された

  • 2007  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2006  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2005  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2005  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2004  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2003  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2002  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2001  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 2000  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 1999  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 1998  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 1997  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

  • 1996  Coaching of Students' Association  磁力計設置・メンテナンスグループ

     詳細を見る

    久住高原農場に設置してある電磁場観測所に於いて、学生の地磁気観測手法・観測装置設置・メンテナンスの指導を行う。
    頻度は1月半に一回、年10回程度

▼display all

Outline of Social Contribution and International Cooperation activities

  • MAGDAS/CPMNプロジェクトを、PIとして統括、国内外58研究機関と国際連携活動を推進している。
    また、国連と連携して、宇宙天気キャパシティ・ビルディング活動を推進、国際宇宙天気イニシアティブプロジェクトの中核的メンバーとして、
    宇宙天気研究・観測の国際連携に貢献している。

Social Activities

  • 伊藤早苗記念基金事業「QURIESプログラム」において、夏休みの1週間女子高生への研究指導を行った。

    伊藤早苗記念基金事業「QURIESプログラム」  九州大学・国際宇宙惑星環境研究センター  2023.8

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    Audience:General, Scientific, Company, Civic organization, Governmental agency

    Type:Research consultation

  • 伊藤早苗記念基金事業「QURIESプログラム」において、夏休みの1週間女子高生への研究指導を行った。

    伊藤早苗記念基金事業「QURIESプログラム」  九州大学・国際宇宙惑星環境研究センター  2023.8

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    Type:Research consultation

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  • 伊藤早苗記念基金事業「QURIESプログラム」において、夏休みの1週間女子高生への研究指導を行った。

    伊藤早苗記念基金事業「QURIESプログラム」  九州大学・国際宇宙惑星環境研究センター  2022.8

     More details

    Audience:General, Scientific, Company, Civic organization, Governmental agency

    Type:Research consultation

  • 伊藤早苗記念基金事業「QURIESプログラム」において、夏休みの1週間女子高生への研究指導を行った。

    伊藤早苗記念基金事業「QURIESプログラム」  九州大学・国際宇宙惑星環境研究センター  2022.8

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    Type:Research consultation

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  • 伊藤早苗記念基金事業「QURIESプログラム」において、夏休みの1週間女子高生への研究指導を行った。

    伊藤早苗記念基金事業「QURIESプログラム」  九州大学・国際宇宙惑星環境研究センター  2021.8

     More details

    Audience:General, Scientific, Company, Civic organization, Governmental agency

    Type:Research consultation

  • 令和3年度九州大学Quries プログラムの実施

    2021.8

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    Audience:Infants, Schoolchildren, Junior students, High school students

    Type:Seminar, workshop

  • 令和3年度九州大学Quries プログラムの実施

    2021.8

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    Type:Science cafe

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  • 伊藤早苗記念基金事業「QURIESプログラム」において、夏休みの1週間女子高生への研究指導を行った。

    伊藤早苗記念基金事業「QURIESプログラム」  九州大学・国際宇宙惑星環境研究センター  2021.8

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    Type:Research consultation

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  • (1)オーストリア(ウィーン)国連宇宙平和利用委員会・UNISPACE50の参加 (2)マレーシア(クアラルンプール, ペナン)ICESSAT2018での基調講演(クアラルンプール,マラ工科大学)及び,MAGDAS観測点整備(ペナン島) (3)ロシア(ヤクーツク)ロシア科学アカデミー宇宙線研究所(IKFIA)との国際交流 (4)インドネシア(ジャカルタ)Geomagnetic Focus Group Discussion 2018での招待講演,及びインドネシア国土気象庁(BMKG)大学での特別講演 (5)スリランカ(コロンボ)Scientific lecture at the annual Theme Seminar of the Sri Lanka Association for the Advancement of Scienceでの基調講演 (6)ペルー(ワンカイヨ)FM-CWレーダー建設の協力

    2018

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    (1)オーストリア(ウィーン)国連宇宙平和利用委員会・UNISPACE50の参加 (2)マレーシア(クアラルンプール, ペナン)ICESSAT2018での基調講演(クアラルンプール,マラ工科大学)及び,MAGDAS観測点整備(ペナン島) (3)ロシア(ヤクーツク)ロシア科学アカデミー宇宙線研究所(IKFIA)との国際交流 (4)インドネシア(ジャカルタ)Geomagnetic Focus Group Discussion 2018での招待講演,及びインドネシア国土気象庁(BMKG)大学での特別講演 (5)スリランカ(コロンボ)Scientific lecture at the annual Theme Seminar of the Sri Lanka Association for the Advancement of Scienceでの基調講演 (6)ペルー(ワンカイヨ)FM-CWレーダー建設の協力

  • (1)オーストリア(ウィーン)国連宇宙平和利用委員会・UNISPACE50の参加 (2)マレーシア(クアラルンプール, ペナン)ICESSAT2018での基調講演(クアラルンプール,マラ工科大学)及び,MAGDAS観測点整備(ペナン島) (3)ロシア(ヤクーツク)ロシア科学アカデミー宇宙線研究所(IKFIA)との国際交流 (4)インドネシア(ジャカルタ)Geomagnetic Focus Group Discussion 2018での招待講演,及びインドネシア国土気象庁(BMKG)大学での特別講演 (5)スリランカ(コロンボ)Scientific lecture at the annual Theme Seminar of the Sri Lanka Association for the Advancement of Scienceでの基調講演 (6)ペルー(ワンカイヨ)FM-CWレーダー建設の協力

    2018

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    Type:Other

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  • (1)2nd National School on EARTH and ELECTROMAGNETISM(マレーシア:マラ工科大学)での集中講義(2017年8月)、(2)ANGASA(マレーシア国立宇宙局) Public talk(マレーシア:マレーシア大学)での特別講演(2017年8月)、(3)第2回国際赤道・低緯度電離圏に関する国際学校(ISELLI-2)(ナイジェリア、宇宙開発機構)での「磁気圏電離圏結合の基礎」、「磁場データの宇宙天気研究への活用」、に関する集中講義(2017年9月)、(4)Japan-Malaysia Joint Seminar on Space and Earth Electromagnetism 2018(九州大学)での集中講義、(5)大学・部局間国際交流協定等推進事業に係る外国人教員招聘に基づく国際共同プロジェクト「Composite study on Magnetosphere-Ionosphere Coupling by using MAGDAS and SWARM satelliteの遂行」(2017年11月から2018年5月)

    2017

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    (1)2nd National School on EARTH and ELECTROMAGNETISM(マレーシア:マラ工科大学)での集中講義(2017年8月)、(2)ANGASA(マレーシア国立宇宙局) Public talk(マレーシア:マレーシア大学)での特別講演(2017年8月)、(3)第2回国際赤道・低緯度電離圏に関する国際学校(ISELLI-2)(ナイジェリア、宇宙開発機構)での「磁気圏電離圏結合の基礎」、「磁場データの宇宙天気研究への活用」、に関する集中講義(2017年9月)、(4)Japan-Malaysia Joint Seminar on Space and Earth Electromagnetism 2018(九州大学)での集中講義、(5)大学・部局間国際交流協定等推進事業に係る外国人教員招聘に基づく国際共同プロジェクト「Composite study on Magnetosphere-Ionosphere Coupling by using MAGDAS and SWARM satelliteの遂行」(2017年11月から2018年5月)

  • (1)2nd National School on EARTH and ELECTROMAGNETISM(マレーシア:マラ工科大学)での集中講義(2017年8月)、(2)ANGASA(マレーシア国立宇宙局) Public talk(マレーシア:マレーシア大学)での特別講演(2017年8月)、(3)第2回国際赤道・低緯度電離圏に関する国際学校(ISELLI-2)(ナイジェリア、宇宙開発機構)での「磁気圏電離圏結合の基礎」、「磁場データの宇宙天気研究への活用」、に関する集中講義(2017年9月)、(4)Japan-Malaysia Joint Seminar on Space and Earth Electromagnetism 2018(九州大学)での集中講義、(5)大学・部局間国際交流協定等推進事業に係る外国人教員招聘に基づく国際共同プロジェクト「Composite study on Magnetosphere-Ionosphere Coupling by using MAGDAS and SWARM satelliteの遂行」(2017年11月から2018年5月)

    2017

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    Type:Other

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  • (1) ICUS/SCOSTEP International School(インド、シャングリ)での「磁気圏電離圏結合」に関する集中講義(2016年8月)、(2)COSPAR Capacity Building Workshop:Impact of Space Weather on Earth (ロシア、パラツンカ)での「宇宙天気」に関する集中講義(2016年11月)、(3)JASSO帰国外国人留学生研究指導事業に基づく共同研究プロジェクト「MAGDASデータを用いた太陽活動と地殻変動現象の関連性」に関する調査活動の遂行、(2016年7月から2016年9月)、(4)大学・部局間国際交流協定等推進事業に係る外国人教員招聘に基づく国際共同プロジェクト「Seismoelectromagnetics of the Moro Gulf Quake project」の遂行(2016年10月から2017年5月)

    2016

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    (1) ICUS/SCOSTEP International School(インド、シャングリ)での「磁気圏電離圏結合」に関する集中講義(2016年8月)、(2)COSPAR Capacity Building Workshop:Impact of Space Weather on Earth (ロシア、パラツンカ)での「宇宙天気」に関する集中講義(2016年11月)、(3)JASSO帰国外国人留学生研究指導事業に基づく共同研究プロジェクト「MAGDASデータを用いた太陽活動と地殻変動現象の関連性」に関する調査活動の遂行、(2016年7月から2016年9月)、(4)大学・部局間国際交流協定等推進事業に係る外国人教員招聘に基づく国際共同プロジェクト「Seismoelectromagnetics of the Moro Gulf Quake project」の遂行(2016年10月から2017年5月)

  • (1) ICUS/SCOSTEP International School(インド、シャングリ)での「磁気圏電離圏結合」に関する集中講義(2016年8月)、(2)COSPAR Capacity Building Workshop:Impact of Space Weather on Earth (ロシア、パラツンカ)での「宇宙天気」に関する集中講義(2016年11月)、(3)JASSO帰国外国人留学生研究指導事業に基づく共同研究プロジェクト「MAGDASデータを用いた太陽活動と地殻変動現象の関連性」に関する調査活動の遂行、(2016年7月から2016年9月)、(4)大学・部局間国際交流協定等推進事業に係る外国人教員招聘に基づく国際共同プロジェクト「Seismoelectromagnetics of the Moro Gulf Quake project」の遂行(2016年10月から2017年5月)

    2016

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    Type:Other

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  • (1) International school on equatorial and low-latitude ionosphere での宇宙天気研究に関する集中講義(2015年9月ナイジェリア宇宙科学機構)、(2)マニラ観測所開所150周年式典でのキーノートスピーチ(2015年9月)、(3)コロンボ大学総長との学術交流打ち合わせ、これに基づく地磁気観測所開設、(3)大学・部局間国際交流協定等推進事業に係る外国人教員招聘に基づく国際共同プロジェクト「Studies on global aspects of Storm Sudden Commencement」の遂行(2015年2月~8月)

    2015

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    (1) International school on equatorial and low-latitude ionosphere での宇宙天気研究に関する集中講義(2015年9月ナイジェリア宇宙科学機構)、(2)マニラ観測所開所150周年式典でのキーノートスピーチ(2015年9月)、(3)コロンボ大学総長との学術交流打ち合わせ、これに基づく地磁気観測所開設、(3)大学・部局間国際交流協定等推進事業に係る外国人教員招聘に基づく国際共同プロジェクト「Studies on global aspects of Storm Sudden Commencement」の遂行(2015年2月~8月)

  • (1) International school on equatorial and low-latitude ionosphere での宇宙天気研究に関する集中講義(2015年9月ナイジェリア宇宙科学機構)、(2)マニラ観測所開所150周年式典でのキーノートスピーチ(2015年9月)、(3)コロンボ大学総長との学術交流打ち合わせ、これに基づく地磁気観測所開設、(3)大学・部局間国際交流協定等推進事業に係る外国人教員招聘に基づく国際共同プロジェクト「Studies on global aspects of Storm Sudden Commencement」の遂行(2015年2月〜8月)

    2015

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  • (1)United Nations/Japan for Space Weather Symposium, Fukuoka, Japan, 2-6 March 2015を主催し、Keynote speechを行った。 (2)インドネシア気象庁(BMKG)での宇宙天気研究に関する集中講義, Geomagnetic Workshop in Medan(North Sumatra, Indonesia), Hotel Sibayak Berastagi, 7-9 September 2014、 (3) マレーシア宇宙科学研究所での集中講義, National school on Space and Earth Electromagnetism(SEE) 2014, Langkawi National Observatory, National Space Agency, Malaysia(ANGKASA), 2-5 December 2014、(4)ICUS/SCOSTEP/ISWI International Space Science School (ISSS) in Peruでの集中講

    2014

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    (1)United Nations/Japan for Space Weather Symposium, Fukuoka, Japan, 2-6 March 2015を主催し、Keynote speechを行った。 (2)インドネシア気象庁(BMKG)での宇宙天気研究に関する集中講義, Geomagnetic Workshop in Medan(North Sumatra, Indonesia), Hotel Sibayak Berastagi, 7-9 September 2014、 (3) マレーシア宇宙科学研究所での集中講義, National school on Space and Earth Electromagnetism(SEE) 2014, Langkawi National Observatory, National Space Agency, Malaysia(ANGKASA), 2-5 December 2014、(4)ICUS/SCOSTEP/ISWI International Space Science School (ISSS) in Peruでの集中講

  • (1)United Nations/Japan for Space Weather Symposium, Fukuoka, Japan, 2-6 March 2015を主催し、Keynote speechを行った。 (2)インドネシア気象庁(BMKG)での宇宙天気研究に関する集中講義, Geomagnetic Workshop in Medan(North Sumatra, Indonesia), Hotel Sibayak Berastagi, 7-9 September 2014、 (3) マレーシア宇宙科学研究所での集中講義, National school on Space and Earth Electromagnetism(SEE) 2014, Langkawi National Observatory, National Space Agency, Malaysia(ANGKASA), 2-5 December 2014、(4)ICUS/SCOSTEP/ISWI International Space Science School (ISSS) in Peruでの集中講

    2014

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  • 国連・外務省と連携して国際的な宇宙天気科学キャパシティ・ビルディング・イニシアティブ活動を継続。 (1)2013/9月;国連宇宙環境データ解析会議でのキーノートスピーチ実施 (2)2013/10月;国際宇宙天気イニシアチブ/MAGDAS アフリカ国際学校の実施 (3)2013/10月;インドネシア地震気象庁での集中講義の実施 (4)2014/1月;アフリカ・南米から5名の外国人若手研究者を招聘し、MAGDASトレーニングを実施 (5)2014/2月;国連宇宙平和利用委員会での九州大学のテクニカルプレゼンテーション、日本のステートメント発表、国際宇宙天気イニシアチブ会議での国際イニシアチブ事業再構成の提案

    2013

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    国連・外務省と連携して国際的な宇宙天気科学キャパシティ・ビルディング・イニシアティブ活動を継続。 (1)2013/9月;国連宇宙環境データ解析会議でのキーノートスピーチ実施 (2)2013/10月;国際宇宙天気イニシアチブ/MAGDAS アフリカ国際学校の実施 (3)2013/10月;インドネシア地震気象庁での集中講義の実施 (4)2014/1月;アフリカ・南米から5名の外国人若手研究者を招聘し、MAGDASトレーニングを実施 (5)2014/2月;国連宇宙平和利用委員会での九州大学のテクニカルプレゼンテーション、日本のステートメント発表、国際宇宙天気イニシアチブ会議での国際イニシアチブ事業再構成の提案

  • 国連・外務省と連携して国際的な宇宙天気科学キャパシティ・ビルディング・イニシアティブ活動を継続。 (1)2013/9月;国連宇宙環境データ解析会議でのキーノートスピーチ実施 (2)2013/10月;国際宇宙天気イニシアチブ/MAGDAS アフリカ国際学校の実施 (3)2013/10月;インドネシア地震気象庁での集中講義の実施 (4)2014/1月;アフリカ・南米から5名の外国人若手研究者を招聘し、MAGDASトレーニングを実施 (5)2014/2月;国連宇宙平和利用委員会での九州大学のテクニカルプレゼンテーション、日本のステートメント発表、国際宇宙天気イニシアチブ会議での国際イニシアチブ事業再構成の提案

    2013

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    Type:Other

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  • 国連・外務省と連携して国際的な宇宙天気科学キャパシティ・ビルディング活動を開始した。 (1)2012/6月;国連宇宙平和利用委員会での国際宇宙天気科学・教育センターの設置に関するテクニカルプレゼンテーションの実施 (2)2012/9月;国連宇宙環境データ解析会議でのセミナーとキーノートスピーチの実施 (3)2012/9月;国際宇宙天気イニシアチブ/MAGDAS 国際学校の実施 (4)2012/10月;国際宇宙天気イニシアチブ会議での国際宇宙天気科学・教育センターの活動報告 (5)2013/2月;国連宇宙平和利用委員会での国際宇宙天気科学・教育センターの活動に関するテクニカルプレゼンテーションの実施

    2012

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    国連・外務省と連携して国際的な宇宙天気科学キャパシティ・ビルディング活動を開始した。 (1)2012/6月;国連宇宙平和利用委員会での国際宇宙天気科学・教育センターの設置に関するテクニカルプレゼンテーションの実施 (2)2012/9月;国連宇宙環境データ解析会議でのセミナーとキーノートスピーチの実施 (3)2012/9月;国際宇宙天気イニシアチブ/MAGDAS 国際学校の実施 (4)2012/10月;国際宇宙天気イニシアチブ会議での国際宇宙天気科学・教育センターの活動報告 (5)2013/2月;国連宇宙平和利用委員会での国際宇宙天気科学・教育センターの活動に関するテクニカルプレゼンテーションの実施

  • 国連・外務省と連携して国際的な宇宙天気科学キャパシティ・ビルディング活動を開始した。 (1)2012/6月;国連宇宙平和利用委員会での国際宇宙天気科学・教育センターの設置に関するテクニカルプレゼンテーションの実施 (2)2012/9月;国連宇宙環境データ解析会議でのセミナーとキーノートスピーチの実施 (3)2012/9月;国際宇宙天気イニシアチブ/MAGDAS 国際学校の実施 (4)2012/10月;国際宇宙天気イニシアチブ会議での国際宇宙天気科学・教育センターの活動報告 (5)2013/2月;国連宇宙平和利用委員会での国際宇宙天気科学・教育センターの活動に関するテクニカルプレゼンテーションの実施

    2012

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    Type:Other

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Media Coverage

  • NHK番組内でのオーロラに関するコメント TV or radio program

    2023.3

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    NHK番組内でのオーロラに関するコメント

  • NHK番組内でのオーロラに関するコメント TV or radio program

    2023.3

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  • 内部磁気圏探査衛星「あらせ」プロジェクト及び、その地上連携観測に関するインタビュー記事 Newspaper, magazine

    2015.11

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    内部磁気圏探査衛星「あらせ」プロジェクト及び、その地上連携観測に関するインタビュー記事

  • 国連宇宙天気ワークショップ開催に関する、日本側主催者としてのインタビュー TV or radio program

    2015.3

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    国連宇宙天気ワークショップ開催に関する、日本側主催者としてのインタビュー

Activities contributing to policy formation, academic promotion, etc.

  • 2022.4 - 2024.3   ・第25期学術会議地球惑星科学委員会地球惑星科学国際連携分科会SCOSTEP/STPP小委員会 ・International Space Weather Initiative (ISWI) Project Steering committee

    第25期学術会議地球惑星科学委員会地球惑星科学国際連携分科会SCOSTEP/STPP小委員会委員(副委員長)として、地球惑星科学に関する国際的なプロジェクトの立案、促進寄与に関する学術活動を行っている。同時に、国連・各国機関と連携したISWIにおいては、Steering committee memberとして各国の連携に貢献鶴と共に調整を図ると共に、 我が国の宇宙空間の国際的観測活動を束ねるnational coordinatorに就任した。

  • 2018.4 - 2021.3   第24期学術会議地球惑星科学委員会地球惑星科学国際連携分科会SCOSTEP/STPP小委員会

    第24期学術会議地球惑星科学委員会地球惑星科学国際連携分科会SCOSTEP/STPP小委員会委員(副委員長)として、地球惑星科学に関する国際的なプロジェクトの立案、促進寄与に関する学術活動を行っている。

  • 2018.4 - 2021.3   第24期学術会議地球惑星科学委員会

    地球惑星科学国際連携分科会 SCOSTEP-STPP小委員会(副委員長)

  • 2016.6 - 2021.6   国際科学者会議(ICUS):太陽地球系物理学委員会(SCOSTEP)

    国際科学者会議(ICUS)、太陽地球系物理学委員会(SCOSTEP)の SVSプログラム(国際的な若手研究者育成プログラム)の審査委員としての活動

  • 2016.4 - 2018.3   第23期学術会議情報学委員会国際サイエンスデータ分科会WDS小委員会

    第23期学術会議情報学委員会国際サイエンスデータ分科会WDS小委員会委員として、国際的なデータ活動の促進寄与に関する学術活動を行った

  • 2016.4 - 2018.3   第23期学術会議地球惑星科学委員会地球惑星科学国際連携分科会STPP小委員会

    第23期学術会議地球惑星科学委員会地球惑星科学国際連携分科会STPP小委員会委員(幹事)として、地球惑星科学に関する国際的なプロジェクトの立案、促進寄与に関する学術活動を行った

  • 2015.4 - 2018.3   第23期学術会議地球惑星科学委員会(幹事)

    地球惑星科学国際連携分科会STPP小委員会委員

  • 2015.4 - 2018.3   第23期学術会議情報学委員会

    国際サイエンスデータ分科会WDS小委員会委員

  • 2014.4 - Present   名古屋大学太陽地球環境研究所

    総合観測解析部門専門委員会委員

  • 2014.4 - 2030.3   International Space Weather Initiative Project Steering committee (http://www.iswi-secretariat.org)

    国際連合宇宙部(UN/OOSA)と連携して、国際宇宙天気イニシアチブプロジェクト(ISWI: International Space Weather Initiative)のexcecutive commiteeメンバーとして、国際的なキャパシティビルディング活動や学術振興活動を行っている。

  • 2013.4 - 2018.3   地球電磁気・地球惑星圏学会

    大林奨励賞候補者推薦委員

  • 2012.4 - Present   地球電磁気・地球惑星圏学会

    将来検討委員会委員

  • 2012.4 - 2016.3   Earth, Planets, and Space誌

    編集委員会委員

  • 2012.4 - 2015.3   第22期学術会議情報学委員会

    国際サイエンスデータ分科会WDS小委員会委員

  • 2012.4 - 2015.3   第22期学術会議地球惑星科学委員会

    地球惑星科学国際連携分科会STPP小委員会委員

  • 2012.4 - 2014.3   名古屋大学太陽地球環境研究所ジオスペース研究センター

    総合観測専門委員会委員

  • 2008.4 - Present   欧州非干渉散乱データ特別実験観測分科会

    審査委員

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Educational Activities for Highly-Specialized Professionals in Other Countries

  • 2018.3   Japan-Malaysia Joint Seminar on Space and Earth Electromagnetism 2018 (マレーシア7大学、12名の若手教員を九州大学に招へいし、宇宙空間科学、宇宙天気科学を推進するための基礎学問についての集中セミナーを実行)

    Main countries of student/trainee affiliation:Malaysia

    Other countries of student/trainee affiliation:マレーシア

  • 2014.4 - 2015.3   MAGDAS/International Capacity building (JSPS学術基盤形成に基づき、計6名を九州大学に招聘、2週間のMAGDASトレーニングを行った)

    Main countries of student/trainee affiliation:Philippines

    Other countries of student/trainee affiliation:エジプト、ナイジェリア、コートジボワール、モザンビーク、ペルー、インドネシア、フィリピン

  • 2013.4 - 2014.5   MAGDAS/International Capacity building (JSPS学術基盤形成に基づき計7名を九州大学に招聘、2週間のMAGDASトレーニングを行った)

    Main countries of student/trainee affiliation:Indonesia

    Other countries of student/trainee affiliation:フィリピン、ベトナム、マレーシア、オーストラリア

  • 2012.5 - 2013.3   MAGDAS/International Capacity building (JSPS学術基盤形成に基づき計7名を九州大学に招聘、2週間のMAGDASトレーニングを行った)

    Main countries of student/trainee affiliation:Indonesia

    Other countries of student/trainee affiliation:フィリピン、ベトナム、マレーシア、オーストラリア

Acceptance of Foreign Researchers, etc.

  • Kyushu University

    Acceptance period: 2024.4 - 2025.3   (Period):1 month or more

    Nationality:Egypt

    Business entity:Japan Society for the Promotion of Science

  • カルフォルニア大学バークレー校

    Acceptance period: 2023.9 - 2024.11   (Period):1 month or more

    Nationality:Germany

    Business entity:Japan Society for the Promotion of Science

  • 日本エジプト科学技術大学

    Acceptance period: 2022.12 - 2023.3   (Period):1 month or more

    Nationality:Nigeria

    Business entity:Foreign governments, foreign research institutes, international organizations

  • コロンボ大学

    Acceptance period: 2022.10 - 2022.12   (Period):1 month or more

    Nationality:Sri Lanka

  • ジョンズ・ホプキンス大学

    Acceptance period: 2022.9 - 2024.9   (Period):Less than 2 weeks

    Nationality:United States

    Business entity:Japan Society for the Promotion of Science

  • Indian Institute of Geomagnetism

    Acceptance period: 2022.7 - 2023.9   (Period):1 month or more

    Nationality:India

    Business entity:Foreign governments, foreign research institutes, international organizations

  • National Research Institute of Astronomy and Geophysics

    Acceptance period: 2020.1 - 2020.9   (Period):1 month or more

    Nationality:Egypt

    Business entity:Foreign governments, foreign research institutes, international organizations

  • National Research Institute of Astronomy and Geophysics

    Acceptance period: 2019.12 - 2020.8   (Period):1 month or more

    Nationality:Egypt

    Business entity:Foreign governments, foreign research institutes, international organizations

  • コロンボ大学

    Acceptance period: 2019.10 - 2019.12   (Period):1 month or more

    Nationality:Sri Lanka

    Business entity:Foreign governments, foreign research institutes, international organizations

  • National Research Institute of Astronomy and Geophysics (NRIAG)

    Acceptance period: 2018.6 - 2018.7   (Period):1 month or more

    Nationality:Egypt

    Business entity:Foreign governments, foreign research institutes, international organizations

  • Department of Physics, Oulu University

    Acceptance period: 2017.11 - 2018.5   (Period):1 month or more

    Nationality:Finland

    Business entity:On-campus funds

  • マラ工科大学

    Acceptance period: 2017.7 - 2017.9   (Period):1 month or more

    Nationality:Malaysia

    Business entity:Foreign governments, foreign research institutes, international organizations

  • マラ工科大学

    Acceptance period: 2017.7 - 2017.9   (Period):1 month or more

    Nationality:Malaysia

    Business entity:Foreign governments, foreign research institutes, international organizations

  • National Research Institute of Astronomy and Geophysics (NRIAG)

    Acceptance period: 2017.5 - 2017.6   (Period):1 month or more

    Nationality:Egypt

    Business entity:Japan Society for the Promotion of Science

  • コロンボ大学

    Acceptance period: 2017.2 - 2017.3   (Period):2weeks to less than 1 month

    Nationality:Sri Lanka

    Business entity:Foreign governments, foreign research institutes, international organizations

  • Department of Physics, Ateneo de Manila University, Program Manager, Upper Atmosphere Dynamics, Manila Observatory

    Acceptance period: 2016.10 - 2017.5   (Period):1 month or more

    Nationality:Philippines

    Business entity:On-campus funds

  • National Research Institute of Astronomy and Geophysics (NRIAG)

    Acceptance period: 2016.7 - 2016.9   (Period):1 month or more

    Nationality:Egypt

    Business entity:Japan Society for the Promotion of Science

  • ロシア科学アカデミーYu.Gシャファー宇宙物理・超高層大気物理学研究所

    Acceptance period: 2015.2 - 2015.8   (Period):1 month or more

    Nationality:Russian Federation

    Business entity:On-campus funds

  • フィンランド気象研究所

    Acceptance period: 2014.9 - 2014.11   (Period):1 month or more

    Nationality:Germany

    Business entity:Other

  • ジョンズ・ホプキンス大学応用物理学研究所

    Acceptance period: 2014.3 - 2014.4   (Period):2weeks to less than 1 month

    Nationality:United States

    Business entity:On-campus funds

  • ナイジェリア宇宙開発事業団

    Acceptance period: 2014.3   (Period):Less than 2 weeks

    Nationality:Other

    Business entity:Japan Society for the Promotion of Science

  • インドネシア航空宇宙庁

    Acceptance period: 2013.10 - 2013.11   (Period):2weeks to less than 1 month

    Nationality:Indonesia

    Business entity:Foreign governments, foreign research institutes, international organizations

  • パリ先端科学校(グランセコール)

    Acceptance period: 2013.6 - 2013.8   (Period):1 month or more

    Nationality:France

    Business entity:Foreign governments, foreign research institutes, international organizations

  • ジョンズ・ホプキンス大学応用物理学研究所

    Acceptance period: 2013.1   (Period):Less than 2 weeks

    Nationality:United States

    Business entity:On-campus funds

  • ジョンズ・ホプキンス大学応用物理学研究所

    Acceptance period: 2012.10 - 2013.10   (Period):Less than 2 weeks

    Nationality:United States

    Business entity:Foreign governments, foreign research institutes, international organizations

  • フィンランド気象研究所

    Acceptance period: 2012.4   (Period):Less than 2 weeks

    Nationality:Germany

    Business entity:Foreign governments, foreign research institutes, international organizations

  • フィンランド気象研究所

    Acceptance period: 2011.11 - 2012.4   (Period):1 month or more

    Nationality:Finland

    Business entity:Japan Society for the Promotion of Science

  • フィンランド気象研究所

    Acceptance period: 2010.3 - 2009.3   (Period):Less than 2 weeks

    Nationality:Finland

    Business entity:Foreign governments, foreign research institutes, international organizations

  • フィンランド気象研究所

    Acceptance period: 2009.1   (Period):Less than 2 weeks

    Nationality:Finland

    Business entity:Foreign governments, foreign research institutes, international organizations

  • コロラド大学大気海洋研究センター

    Acceptance period: 2008.3   (Period):Less than 2 weeks

    Nationality:Japan

    Business entity:On-campus funds

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Travel Abroad

  • 2023.12

    Staying countory name 1:United States   Staying institution name 1:モスコーニ国際会議場

  • 2023.10

    Staying countory name 1:Malaysia   Staying institution name 1:ヒルトンペナン

  • 2023.10

    Staying countory name 1:Malaysia   Staying institution name 1:マレーシア国民大学

  • 2023.5 - 2023.6

    Staying countory name 1:Germany   Staying institution name 1:Berlin, Germany

  • 2019.12

    Staying countory name 1:United States   Staying institution name 1:モスコーニ国際会議場

  • 2018.12

    Staying countory name 1:Peru   Staying institution name 1:ペルー地球物理学研究所

  • 2018.11 - 2018.12

    Staying countory name 1:Sri Lanka   Staying institution name 1:スリランカ学術会議

  • 2018.11

    Staying countory name 1:United States   Staying institution name 1:USGS観測所

  • 2018.9

    Staying countory name 1:Russian Federation   Staying institution name 1:ロシア科学アカデミー宇宙線研究所(IKFIA)

  • 2018.9

    Staying countory name 1:Indonesia   Staying institution name 1:BMKG

  • 2018.8 - 2017.8

    Staying countory name 1:Malaysia   Staying institution name 1:マラ工科大学

  • 2018.6

    Staying countory name 1:Austria   Staying institution name 1:国連

  • 2018.6

    Staying countory name 1:Austria   Staying institution name 1:国際連合本部

  • 2018.6 - 2017.6

    Staying countory name 1:United States   Staying institution name 1:USGS観測所

  • 2017.12

    Staying countory name 1:Australia   Staying institution name 1:オーストラリア気象庁

  • 2017.12

    Staying countory name 1:Other   Staying institution name 1:YAP気象ステーション

  • 2017.9

    Staying countory name 1:Nigeria   Staying institution name 1:ナイジェリア国立宇宙研究開発機構

  • 2017.9

    Staying countory name 1:Russian Federation   Staying institution name 1:ロシア科学アカデミー極東研究所(IKRI)

  • 2017.8 - 2017.9

    Staying countory name 1:Peru   Staying institution name 1:Universidad Nacional Agraria de la Selva

    Staying institution name 2:ペルー地球物理学研究所

  • 2017.8

    Staying countory name 1:Malaysia   Staying institution name 1:マラ工科大学

    Staying institution name 2:マレーシア大学

  • 2017.6

    Staying countory name 1:Russian Federation   Staying institution name 1:ロシア科学アカデミー極東研究所(IKRI)

  • 2017.6

    Staying countory name 1:United States   Staying institution name 1:ノーフォーク国際会議場

  • 2017.3

    Staying countory name 1:Indonesia   Staying institution name 1:インドネシア気象気候地球物理庁(BMKG)

  • 2017.2 - 2017.3

    Staying countory name 1:Peru   Staying institution name 1:ペルー地球物理学研究所

  • 2017.2

    Staying countory name 1:Malaysia   Staying institution name 1:マラ工科大学

  • 2016.12

    Staying countory name 1:United States   Staying institution name 1:モスコーニ国際会議場

  • 2016.10

    Staying countory name 1:India   Staying institution name 1:シャングリ国際会議場

  • 2016.9

    Staying countory name 1:Other   Staying institution name 1:YAP気象ステーション

  • 2016.8

    Staying countory name 1:China   Staying institution name 1:北京オリンピックセンター

  • 2016.8

    Staying countory name 1:Russian Federation   Staying institution name 1:ロシア科学アカデミー極東研究所

  • 2016.8

    Staying countory name 1:Korea, Republic of   Staying institution name 1:ソウル国際会議場

  • 2016.5

    Staying countory name 1:Croatia   Staying institution name 1:国際会議場

  • 2016.2

    Staying countory name 1:Austria   Staying institution name 1:国際連合本部

  • 2016.2

    Staying countory name 1:Sri Lanka   Staying institution name 1:コロンボ大学

  • 2016.1 - 2016.2

    Staying countory name 1:United States   Staying institution name 1:ジョンズ・ホプキンズ大学応用物理学研究所

  • 2015.10

    Staying countory name 1:Ethiopia   Staying institution name 1:エチオピア大学

  • 2015.9

    Staying countory name 1:Nigeria   Staying institution name 1:ナイジェリア国立宇宙研究開発機構

  • 2015.9

    Staying countory name 1:Philippines   Staying institution name 1:アテネオ大学

    Staying institution name 2:マニラ観測所

  • 2015.8 - 2015.9

    Staying countory name 1:Finland   Staying institution name 1:Oulu大学

    Staying institution name 2:フィンランド気象研究所

  • 2015.6 - 2014.6

    Staying countory name 1:United States   Staying institution name 1:スノーマス国際会議場

  • 2014.12

    Staying countory name 1:United States   Staying institution name 1:Moscone Center

  • 2014.11 - 2014.12

    Staying countory name 1:Malaysia   Staying institution name 1:マレーシア航空宇宙庁

  • 2014.9

    Staying countory name 1:Korea, Republic of   Staying institution name 1:ハイアットホテル

  • 2014.9

    Staying countory name 1:Austria   Staying institution name 1:オーストリア科学アカデミー

  • 2014.9

    Staying countory name 1:Peru   Staying institution name 1:ペルー地球物理学研究所

  • 2014.9

    Staying countory name 1:Indonesia   Staying institution name 1:インドネシア気象庁(BMKG)

  • 2014.2

    Staying countory name 1:Austria   Staying institution name 1:国連ウィーン本部

  • 2013.12

    Staying countory name 1:United States   Staying institution name 1:ジョンズ・ホプキンズ大学 応用物理学研究所

    Staying institution name 2:モスコーニコンベンションセンター

  • 2013.10

    Staying countory name 1:Finland   Staying institution name 1:フィンランド気象研究所

  • 2013.10

    Staying countory name 1:Indonesia   Staying institution name 1:インドネシア地震・気象庁

  • 2013.9

    Staying countory name 1:Austria   Staying institution name 1:オーストリア科学アカデミー

  • 2013.9

    Staying countory name 1:Other   Staying institution name 1:ココディ大学

  • 2013.4

    Staying countory name 1:Switzerland   Staying institution name 1:スイス国際宇宙科学研究所

    Staying countory name 2:Austria   Staying institution name 2:ウィーン国際会議場

    Staying institution name 3:オーストリア科学アカデミー

  • 2013.2

    Staying countory name 1:Austria   Staying institution name 1:国連ウィーン本部

  • 2013.2

    Staying countory name 1:Switzerland   Staying institution name 1:スイス国際宇宙科学研究所

  • 2012.11 - 2012.12

    Staying countory name 1:United States   Staying institution name 1:ジョンズ・ホプキンズ大学 応用物理学研究所

    Staying institution name 2:モスコーニコンベンションセンター

  • 2012.9 - 2012.10

    Staying countory name 1:Ecuador   Staying institution name 1:エクアドル外務省

  • 2012.9

    Staying countory name 1:Peru   Staying institution name 1:ペルー地球物理学研究所

    Staying institution name 2:イカ大学太陽観測所

  • 2012.9

    Staying countory name 1:Indonesia   Staying institution name 1:インドネシア航空宇宙庁

  • 2012.9

    Staying countory name 1:Austria   Staying institution name 1:オーストリア科学アカデミー

  • 2012.6

    Staying countory name 1:Austria   Staying institution name 1:国連ウィーン本部

  • 2012.6

    Staying countory name 1:United States   Staying institution name 1:スノーマス会議場

  • 2011.12

    Staying countory name 1:United States   Staying institution name 1:モスコーンセンター

  • 2011.10

    Staying countory name 1:United States   Staying institution name 1:ジョンズ・ホプキンズ大学 応用物理学研究所

  • 2011.8

    Staying countory name 1:Other   Staying institution name 1:Redeemers大学

  • 2011.2 - 2011.3

    Staying countory name 1:United States   Staying institution name 1:アラスカ大学地球物理学研究所

  • 2010.8 - 2010.9

    Staying countory name 1:Finland   Staying institution name 1:フィンランド気象研究所

  • 2010.7

    Staying countory name 1:India   Staying institution name 1:ハイデラバード国際会議場

  • 2010.6

    Staying countory name 1:Taiwan, Province of China   Staying institution name 1:台北国際会議場

  • 2010.5

    Staying countory name 1:Austria   Staying institution name 1:ウィーン国際会議場

  • 2009.12

    Staying countory name 1:United States   Staying institution name 1:モスコーンセンター

  • 2008.11

    Staying countory name 1:United States   Staying institution name 1:ミシガン大学

  • 2008.6

    Staying countory name 1:Korea, Republic of   Staying institution name 1:釜山国際コンベンションセンター

  • 2008.3

    Staying countory name 1:Australia   Staying institution name 1:Central Queesland University

    Staying countory name 2:Australia   Staying institution name 2:IPS

    Staying countory name 3:Australia   Staying institution name 3:CISRO

  • 2007.9

    Staying countory name 1:Switzerland   Staying institution name 1:スイス国際宇宙科学研究所

  • 2007.7 - 2007.8

    Staying countory name 1:Italy   Staying institution name 1:ペルージャ大学

    Staying countory name 2:Finland   Staying institution name 2:ヘルシンキ大学

  • 2005.8

    Staying countory name 1:France   Staying institution name 1:ツールース・コンベンションセンター

  • 2005.8

    Staying countory name 1:Australia   Staying institution name 1:オーストラリア南極庁

  • 2005.3

    Staying countory name 1:United States   Staying institution name 1:サンディエゴ・コンベンションセンター

  • 2004.2

    Staying countory name 1:Other   Staying institution name 1:西インド諸島大学

    Staying countory name 2:Brazil   Staying institution name 2:ブラジル宇宙科学研究所

    Staying countory name 3:Peru   Staying institution name 3:ペルー地球物理学研究所

  • 2004.2

    Staying countory name 1:Korea, Republic of   Staying institution name 1:kyonhee大学

  • 2003.8 - 2003.10

    Staying countory name 1:United States   Staying institution name 1:アラスカ大学北極圏研究センター

    Staying institution name 2:ジョンホプキンス大学応用物理学研究所(APL)

  • 2002.12

    Staying countory name 1:Peru   Staying institution name 1:ペルー地球物理学研究所

    Staying countory name 2:Brazil   Staying institution name 2:ブラジル宇宙科学研究所

  • 2002.11

    Staying countory name 1:United States   Staying institution name 1:SFO/Moscone convention center

  • 2002.3 - 2003.5

    Staying countory name 1:United States   Staying institution name 1:ミネソタ大学

    Staying institution name 2:ジョンホプキンス大学

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