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-EM15 | |||
| タイトル | Frontiers in solar physics: observation, modeling, and long-term research from the past to the future | |||
| タイトル短縮名 | Frontiers in solar physics | |||
| 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 | 渡邉 恭子 | ||
| 所属 | 防衛大学校 | |||
| 共同コンビーナ 2 | 氏名 | Sterling Alphonse | ||
| 所属 | NASA/MSFC | |||
| 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 | |||
| 共同コンビーナ 4 | 氏名 | Viktor Fedun | ||
| 所属 | University of Sheffield | |||
| 共同コンビーナ 5 | 氏名 | 飯島 陽久 | ||
| 所属 | 名古屋大学 宇宙地球環境研究所 | |||
| 共同コンビーナ 6 | 氏名 | Malcolm Keith Druett | ||
| 所属 | University of Sheffield, UK | |||
| 共同コンビーナ 7 | 氏名 | Alexander Pevtsov | ||
| 所属 | National Solar Observatory | |||
| 共同コンビーナ 8 | 氏名 | 勝川 行雄 | ||
| 所属 | 自然科学研究機構国立天文台 | |||
| セッション言語 | E | |||
| スコープ | In recent years, there has been remarkable progress in solar and heliospheric physics, driven by advancements in observation, theory, and numerical modeling. Breakthrough results from missions such as Solar Orbiter, Parker Solar Probe, CHASE, ASO-S, Aditya-L1, PUNCH, and Proba-3, and from ground-based observatories such as DKIST, have deepened our understanding of solar atmospheric heating, flare-producing eruptions, solar wind acceleration, and the dynamic coupling between the Sun and the heliosphere. Numerical codes such as MURaM, Bifrost, Mancha, RAMENS, R2D2, WholeSun, and SAMS have been developed or are under development to simulate various physical processes in the different layers of the solar atmosphere. However, a fully self-consistent numerical model that spans the entire solar atmosphere and beyond has yet to be achieved. This session aims to provide a platform for researchers to share their latest findings on a variety of topics, including observational studies, numerical simulations, and theory. This session will place special emphasis on numerical modeling approaches and observations, which illuminate the physical processes governing the dynamical activity events in the solar atmosphere, and on the evolution of long-term solar research, which has provided critical insights into solar cycles and variability. We encourage submissions on not only core solar and heliospheric physics topics, but also on topics from related fields, such as magnetospheric, planetary, and stellar physics. By fostering interdisciplinary dialogue, we hope to stimulate new collaborations and insights that will advance our understanding of the Sun and its influence in the solar system. Contributions from early-career researchers and established experts are welcome, and we look forward to vibrant discussions that reflect the diversity and dynamism of this rapidly evolving area of investigation. |
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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 | |||