日本地球惑星科学連合2024年大会
セッション概要| 宇宙惑星科学 (P) | ||||
|---|---|---|---|---|
| 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) |  |
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| 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 | 5/26(日) AM1-PM2 | ||
| 現地 ポスター コアタイム |
5/26(日) PM3 | |||
| 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 a highly dynamic and variable region, mainly due to the changes in energy input from the solar wind through the magnetotail and the plasma supply from the ionosphere. This complex system is affected by various cross-regional, cross-scale, and cross-energy coupling processes. To gain a deeper understanding of this dynamic system, it is essential to conduct comprehensive studies using coordinated observations with multi-point satellite measurements, ground-based networks, and theoretical modeling. Since the 24th solar cycle, such comprehensive studies have been made possible with the help of multiple 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.). This session invites papers presenting recent results on the inner magnetosphere and its coupling/connection with surrounding regions, including the ionosphere and the outer magnetosphere. Papers on new projects (sounding rocket experiments, data assimilation/machine learning, CubeSats, etc.) and future spacecraft missions are also welcome. |
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| 発表方法 | 口頭およびポスターセッション | |||
| 共催情報 | 学協会 | 地球電磁気・地球惑星圏学会 | ||
| ジョイント | - | |||