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 |
現地口頭会場 | 303 |
| 現地 ポスター コアタイム |
5/26(月) PM3 | 現地ポスター会場 | 展示場ホール7・8 | |
| 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. |
|||
| 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 | AGU | |||
| 団体会員以外の組織との共催 | - | |||
| 国際連携団体 | - | |||
| 招待講演 |
Craig Edward DeForest（Polarimeter to UNify the Corona and Heliosphere mission） Mah Asgari-Targhi（Harvard-Smithsonian Center for Astrophysics） Yuanyong DENG dyy@nao.cas.cn（National Astronomical Observatories, Chinese Academy of Sciences） 千葉 翔太（名古屋大学 宇宙地球環境研究所） |
|||
| 時間 | 講演番号 | タイトル | 発表者 |
|---|---|---|---|
| 口頭発表 5月26日 AM1 | |||
| 9:01 - 9:23 | PEM11-01 | NASA's Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission | Craig Edward DeForest |
| 9:23 - 9:45 | PEM11-02 | The heating of the Sun’s Outer Atmosphere: Insights from Modeling and Observations | Mah Asgari-Targhi |
| 9:45 - 10:00 | PEM11-03 | DKISTを用いた太陽電場測定 | 阿南 徹 |
| 10:00 - 10:15 | PEM11-04 | Wavelet 3D-Based Method for the Examination of Propagating Waves Inside a Quiescent Prominence | Aneta Wisniewska |
| 10:15 - 10:30 | PEM11-05 | Feasibility Study of the Radio and Plasma Wave Detector for the Korea-Led L4 Mission | 宮下 幸長 |
| 口頭発表 5月26日 AM2 | |||
| 10:46 - 11:08 | PEM11-06 | Introduction to the Solar Polar orbit Observatory Mission | Yuanyong DENG dyy@nao.cas.cn |
| 11:08 - 11:30 | PEM11-07 | Study of MHD modes population in the mid-corona comparing the radio sounding with MHD simulation and prospects for collaborating with other observations | 千葉 翔太 |
| 11:30 - 11:45 | PEM11-08 | Unveiling the Three-Dimensional Evolution of an Emerging Active Region with SUNRISE III/SCIP | 川畑 佑典 |
| 11:45 - 12:00 | PEM11-09 | A Data-Constrained Magnetohydrodynamic Simulation of the X7.1 Solar Flare on 2024 October 1 | 松本 圭太郎 |
| 12:00 - 12:15 | PEM11-10 | Rapid, short-duration prominence eruptions in M-dwarf: Insights from solar observations | 梶木屋 裕斗 |
| 講演番号 | タイトル | 発表者 |
|---|---|---|
| ポスター発表 5月26日 PM3 | ||
| PEM11-P01 | 深層学習を用いた高温領域の非線形熱伝導シミュレーションの高速化 | 小関 裕真 |
| PEM11-P02 | Statistical Study of Appearance Timing of H-alpha Postflare Loops: Simple Scaling Law Based on Radiative Cooling | 大津 天斗 |
| PEM11-P03 | 減光領域でのプラズマ流によるコロナ質量放出への質量寄与について | 平岡 勇人 |
| PEM11-P04 | Effects of Ionization Nonequilibrium on First Ionization Potential (FIP) Bias during Solar Flares | 小宮山 颯音 |
| PEM11-P05 | Testing a coronal heating model of the young Sun through Model-Observation Comparisons | 坂本 文平 |
| PEM11-P06 | Statistical study about the characteristics of microflares observed with Nobeyama Radioheliograph (NoRH) | 谷口 英駿 |
| PEM11-P07 | 太陽風中での温度異方性を考慮したアルヴェン波の崩壊不安定性の現実的な動径方向発展 | 佐口 隼斗 |
| PEM11-P08 | How Small-scale Jet-like Solar Events from Miniature Flux Rope Eruptions Might Produce the Solar Wind | Sterling Alphonse |
| PEM11-P09 | Statistical study of solar flares by using multiple Time-of-Flight methods observed with Fermi | 矢倉 昌也 |
| PEM11-P10 | A robust MHD relaxation method for reconstructing the solar atmospheric magnetic field | 三好 隆博 |
| PEM11-P11 | Comparison of multiple chromospheric lines for postflare loops accompanied by a flare | 夏目 純也 |
| PEM11-P12 | Solar Flares on the Early Sun: Insights from TESS's Photometric Observations of a Young Sun-like Star, EK Dra. | 一柳 大治朗 |
| PEM11-P13 | Magnetohydrostatic Three-dimensional Coronal Magnetic Field Extrapolation Based on MHD Relaxation Method | 山崎 大輝 |
| PEM11-P14 | Prominence splitting and merging due to interchange instability in helical flux rope | 金子 岳史 |