宇宙惑星科学 (P) | ||||
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セッション小記号 | 太陽地球系科学・宇宙電磁気学・宇宙環境 (EM) | |||
セッション ID | P-EM13 | |||
タイトル | Dynamics of the Inner Magnetospheric System | |||
タイトル短縮名 | Inner Magnetospheric System | |||
開催日時 | ||||
口頭 セッション |
5/23(火) AM2-PM2 |
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現地 ポスター コアタイム |
5/23(火) PM3 | |||
オンライン ポスター セッション |
5/23(火) AM1 | |||
代表コンビーナ | 氏名 | 桂華 邦裕 | ||
所属 | 東京大学大学院理学系研究科地球惑星科学専攻 | |||
共同コンビーナ1 | 氏名 | 三好 由純 | ||
所属 | 名古屋大学宇宙地球環境研究所 | |||
共同コンビーナ2 | 氏名 | Theodore E Sarris | ||
所属 | Democritus University of Thrace | |||
共同コンビーナ3 | 氏名 | Evan G Thomas | ||
所属 | Dartmouth College | |||
セッション言語 | E | |||
スコープ |
The inner magnetosphere is highly variable due to dynamic variations of energy input from the solar wind through the magnetotail and plasma supply from the ionosphere. This dynamics system is also contributed from cross-regional, cross-scale, and cross-energy coupling processes. Coordinated observations with multi-point satellites measurements, ground-based networks, and theoretical modeling are very essential to revealing the dynamic system. In the 24th and 25th solar cycles, a number of satellites (Van Allen Probes, MMS, THEMIS, DSX, Arase, cubesats, etc.), coordinated ground-based observations (THEMIS-GBO, SuperDARN, EISCAT, magnetometers, riometer, etc), and numerical simulations (global kinetic model, MHD model, micro PIC, hybrid, particle tracing simulations, etc.) have greatly contributed to better understanding the inner magnetosphere system. We invite papers presenting recent results on the inner magnetosphere and its coupling/connection with other regions including the ionosphere and the outer magnetosphere. Papers on new projects (sounding rocket experiments, data assimilation/machine learning, etc.) and future spacecraft missions including cubesats are also welcome. |
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発表方法 | 口頭およびポスター | |||
共催情報 | 学協会 | 地球電磁気・地球惑星圏学会 | ||
ジョイント | - |