[E] 口頭発表
セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境
コンビーナ:桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、Aleksandr Y Ukhorskiy(Johns Hopkins University Applied Physics Laboratory)、三好 由純(名古屋大学宇宙地球環境研究所)、Lynn M Kistler(University of New Hampshire Main Campus)
The inner magnetosphere is highly variable because dynamical
variations of incoming energy from the solar wind, magnetospheric tail,
and the ionosphere. Cross-regional/cross-scale/cross-energy couplings
are key processes to understand this dynamical system, and coordinated
observations by multi-satellites and ground-based observations are
very essential to reveal these processes. In the 24th solar cycle,
a number of satellites such as Van Allen Probes, MMS, THEMIS, DSX and
Arase, coordinated ground-based observations (THEMIS-GBO, SuperDARN,
EISCAT, magnetometers, riometer, etc), and numerical simulations
(global kinetic model, MHD model, micro PIC, hybrid simulations) have
successfully investigated the inner magnetosphere system. Papers on recent results
on the inner magnetosphere and/or its coupling with the other regions,
including the ionosphere and the outer magnetosphere are invited. And
presentations on new projects for the inner magnetosphere are also
welcome.
*Christine Gabrielse1、James Roeder1、Justin Lee1、Seth Claudepierre1,2、Drew L. Turner3、T. Paul O'Brien1、Joseph Fennell1、J. Bernard Blake1 (1.The Aerospace Corporation、2.UCLA、3.John Hopkins Applied Physics Lab.)
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*ALEXEI DMITRIEV1,2、Shoichiro Yokota3、Kunihiro Keika4、Tomoaki Hori5、Yoshizumi Miyoshi5 (1.Institute of Space Science and Engineering, National Central University, Jungli City, Taiwan、2.Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, Russia、3.Univesity Osaka, Japan、4.Univesity Tokyo, Japan、5.Univesity Nagoya, Japan)
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*Nigang Liu1、Zhenpeng Su1、Zhonglei Gao2、Huinan Zheng1、Yuming Wang1、Shui Wang1、Yoshizumi Miyoshi3、Iku Shinohara4、Yoshiya Kasahara5、Fuminori Tsuchiya6、Atsushi Kumamoto6、Shoya Matsuda4、Masafumi Shoji3、Takefumi Mitani4、Takeshi Takashima4、Yoichi Kazama7、Bo-Jhou Wang7、Shiang-Yu Wang7、Chae-Woo Jun3、Tzu-Fang Chang8、Sunny W. Y. Tam8、Satoshi Kasahara9、Shoichiro Yokota10、Kunihiro Keika9、Tomoaki Hori3、Ayako Matsuoka4 (1.University of Science and Technology of China, Hefei, China、2.Harbin Institute of Technology, Shenzhen, China、3.Nagoya University, Nagoya, Japan、4.Japan Aerospace Exploration Agency, Kanagawa, Japan、5.Kanazawa University, Kanazawa, Japan、6.Tohoku University, Sendai, Japan、7.Academia Sinica Institute of Astronomy and Astrophysics, Taiwan、8.National Cheng Kung University, Taiwan、9.University of Tokyo, Tokyo, Japan、10.Osaka University, Osaka, Japan)
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*栗田 怜1、三好 由純1、笠原 禎也2、小嶋 浩嗣3、松田 昇也4、松岡 彩子4、篠原 育4 (1.名古屋大学宇宙地球環境研究所、2.金沢大学総合メディア基盤センター、3.京都大学生存圏研究所、4.宇宙科学研究所)
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*Chae-Woo Jun1、Yoshizumi Miyoshi1、Chao Yue2、Jacob Bortnik3、Larry Lyons3、Toshi Nishimura5、Craig Kletzing4、Satoshi Kasahara6、Yasumasa Kasaba7、Shoya Matsuda8、Masafumi Shoji1、Fuminori Tsuchiya6、Atsushi Kumamoto6、Ayako Matsuoka8、Iku Shinohara8 (1.Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan、2.Department of Earth and Space Science, Peking University, Beijing, China、3.Atmospheric and Oceanic Sciences, University of California Los Angeles, Los Angeles, USA、4.Department of Physics and Astronomy, University of Iowa, Iowa City, USA、5.Boston University, Boston, USA、6.Kanazawa University, Kakuma, Japan.、7.Tohoku University, Sendai, Japan. 、8.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan.)
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*小路 真史1、三好 由純1、浅村 和史2、宮崎 惇史1、笠羽 康正3、笠原 禎也4、松田 昇也2、松岡 彩子2、Kistler Lynn5,1 (1.名古屋大学宇宙地球環境研究所、2.宇宙科学研究所、3.東北大学、4.金沢大学、5.ニューハンプシャー大学)
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