日本地球惑星科学連合2025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) | |||
| セッション ID | P-EM11 | |||
| タイトル | Frontiers in solar physics | |||
| タイトル短縮名 | Frontiers in solar physics | |||
| 開催日時 | 口頭セッション | 5/26(月) AM1-AM2 | ||
| 現地ポスター コアタイム |
5/26(月) PM3 | |||
| 代表コンビーナ | 氏名 | 鳥海 森 | ||
| 所属 | 宇宙航空研究開発機構 宇宙科学研究所 | |||
| 共同コンビーナ１ | 氏名 | Sterling Alphonse | ||
| 所属 | NASA/MSFC | |||
| 共同コンビーナ２ | 氏名 | 渡邉 恭子 | ||
| 所属 | 防衛大学校 | |||
| 共同コンビーナ３ | 氏名 | 今田 晋亮 | ||
| 所属 | 東京大学理学系研究科地球惑星科学専攻 | |||
| セッション言語 | E | |||
| スコープ |
As Solar Cycle 25 is reaching its maximum phase, we are witnessing a variety of activity phenomena, including large solar flares and powerful coronal mass ejections, some of which are potentially damaging to our terrestrial environment. While cutting-edge solar observations are now regularly obtained from ground-based observatories such as DKIST, a new space-borne solar observing network is also being established, including the Solar Orbiter and Parker Solar Probe explorers, as well as the recently launched CHASE, ASO-S, and Adytia-L1 missions. Moreover, exciting new space observatories, including MUSE and SOLAR-C, are only a few years away. Progress is also being made in state-of-the-art numerical modeling that is essential for disentangling complex observations and for gaining fresh insights into the highly dynamic nature of solar and solar-wind magnetism and fluid/particle motions. To share and discuss recent advancements in solar physics and related fields, we invite contributions from solar researchers, and also from researchers in heliospheric, planetary, and stellar physics, covering results from their latest observation, numerical modeling, and experimental investigations. |
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| セッション形式 | 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 | AGU | |||
| 団体会員以外の組織との共催 | - | |||
| 国際連携団体 | - | |||