日本地球惑星科学連合2025年大会

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[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

[P-EM13] Dynamics of the Inner Magnetospheric System

2025年5月28日(水) 10:45 〜 12:15 302 (幕張メッセ国際会議場)

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)、三好 由純(名古屋大学宇宙地球環境研究所)、Goldstein Jerry(Southwest Research Institute)、Sun YIXIN(Peking University)、座長:山本 和弘(名古屋大学宇宙地球環境研究所)、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)、Claudia Martinez-Calderon(Nagoya University)


The inner magnetosphere is a highly dynamic and variable region full of cold plasma, energetic particles and wave activities, which is primarily influenced by changes in energy input from the solar wind via the magnetotail, the plasma supply from the ionosphere, and electrodynamic magnetosphere-ionosphere coupling. This complex, driven and self-modifying system - of both plasmas and neutrals - is shaped by various processes that involve cross-regional, cross-scale, and cross-energy coupling. To achieve a deeper understanding of this dynamic environment, it is crucial to conduct comprehensive studies utilizing coordinated observations from multi-point satellite measurements, ground-based networks, and theoretical modeling. During the 24th and 25th solar cycles, advancements in this area have been facilitated by multiple satellite missions (including the Van Allen Probes, MMS, THEMIS, DSX, Arase, and CubeSats), as well as coordinated ground-based observations (such as THEMIS-GBO, SuperDARN, EISCAT, magnetometers, and riometers) and numerical simulations (encompassing global kinetic models, MHD models, micro PIC, hybrid models, and particle tracing simulations).
This session invites submissions of papers highlighting recent research findings related to the inner magnetosphere and its interactions with adjacent regions, including the ionosphere and the outer magnetosphere. We welcome relevant data analysis and contributions from various models and simulations. The initial results of recent severe storm events, such as May and October 2024, are also highly welcome. We encourage papers that discuss new projects, such as sounding rocket experiments, data assimilation and machine learning approaches, and CubeSat projects, as well as insights into future spacecraft missions.

11:00 〜 11:15

*Chae-Woo Jun1Yoshizumi Miyoshi1Tomoaki Hori1Kazuo Shiokawa1Khan-Hyuk Kim2、Jacob Bortnik3、Larry Lyons3Iku Shinohara4Ayako Matsuoka5Yoshiya Kasahara6Shoya Matsuda6Yasumasa Kasaba7Mariko Teramoto8Kazuhiro Yamamoto1Atsuki Shinbori1 (1.Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Japan、2.Kyung-Hee University, Suwon, Korea、3.Atmospheric and Oceanic Sciences, University of California Los Angeles, Los Angeles, USA、4.Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan、5.Kyoto University, Kyoto, Japan、6.Graduate School of Natural Science and Technology, Kanazawa University, Kanazawa, Japan、7.Graduate School of Science, Tohoku University, Sendai, Japan、8.Kyushu Institute of Technology, Iizuka, Japan)

11:15 〜 11:30

*尾花 由紀1海老原 祐輔2新堀 淳樹3土屋 史紀4熊本 篤志5笠原 禎也6松岡 彩子7寺本 万里子8堀 智昭3三好 由純3篠原 育9 (1.九州大学国際宇宙惑星環境研究センター、2.京都大学生存圏研究所、3.名古屋大学宇宙地球環境研究所、4.東北大学惑星プラズマ・大気研究センター、5.東北大・理・地球物理、6.金沢大学、7.京都大学大学院理学研究科附属地磁気世界資料解析センター、8.九州工業大学、9.宇宙科学研究所)

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