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 和文 Frontiers in solar physics
英文 Frontiers in solar physics
タイトル短縮名 和文 Frontiers in solar physics
英文 Frontiers in solar physics
代表コンビーナ 氏名 和文 鳥海 森
英文 Shin Toriumi
所属 和文 宇宙航空研究開発機構 宇宙科学研究所
英文 Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency
共同コンビーナ 1 氏名 和文 Sterling Alphonse
英文 Alphonse Sterling
所属 和文 NASA/MSFC
英文 NASA/MSFC
共同コンビーナ 2 氏名 和文 渡邉 恭子
英文 Kyoko Watanabe
所属 和文 防衛大学校
英文 National Defense Academy of Japan
共同コンビーナ 3 氏名 和文 今田 晋亮
英文 Shinsuke Imada
所属 和文 東京大学理学系研究科地球惑星科学専攻
英文 Department of Earth and Planetary Science, Graduate School of Science, University of Tokyo
発表言語 E
スコープ 和文 
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.
英文 
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（または）ポスターセッション
ジョイントセッション AGU
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