セッション詳細
[P-EM14]Frontiers in solar physics
2023年5月24日(水) 10:45 〜 12:15
オンラインポスターZoom会場 (2) オンラインポスター
コンビーナ:鳥海 森(宇宙航空研究開発機構 宇宙科学研究所)、横山 央明(京都大学大学院理学研究科)、今田 晋亮(東京大学理学系研究科地球惑星科学専攻)、Sterling Alphonse(NASA/MSFC)
現地ポスター発表開催日時 (2023/5/23 17:15-18:45)
This session is for discussion of recent advancement in solar physics and related fields including heliospheric, planetary, and stellar physics. As Solar Cycle 25 progresses on pace to surpass the previous cycle, we have already witnessed numerous massive flares and CMEs. With the addition of new missions such as Parker Solar Probe, Solar Orbiter, CHASE, and ASO-S, the fleet of solar-observing spacecraft continues to watch the Sun to solve its mysteries. In Japan, the SOLAR-C mission completed its mission definition review in the summer of 2022 and is moving into the next phase, anticipating joint observations with NASA's upcoming MUSE mission. We invite contributions not only by solar researchers but also from all related disciplines (including helio, plasma, astrophysics, etc.), covering observations, numerical modeling, and experiments.
[PEM14-P01]衝撃波と Alfven 波乱流によるコロナ加熱を考慮したプロミネンス形成についての 1.5 次元 MHDシミュレーション
*吉久 健朗1、横山 央明1、金子 岳史2 (1.京都大学、2.LMSAL, HAO/NCAR)
[PEM14-P02]Quantitative study of pitch angle distribution through microwave fast propagation in a solar flare observed with Nobeyama Radioheliograph
*松本 圭太郎1、増田 智1、岩井 一正1、金子 岳史2、簑島 敬3 (1.名古屋大学宇宙地球環境研究所 、2.ロッキード・マーティン太陽天体物理学研究所 、3.海洋研究開発機構 数理科学・先端技術研究開発センター )
[PEM14-P03]Multiwavelength Sun-as-a-star Analysis of an M8.7 Flare on 2022 Oct. 2 with H-alpha and EUV Using SMART/SDDI and SDO/EVE
*大津 天斗1,2、浅井 歩2 (1.京都大学理学研究科宇宙物理学教室、2.京都大学理学研究科附属天文台)
[PEM14-P04]Differential Emission Measure (DEM) Analysis of Small-scale Eruptions in AR 12860
*Cheng-Ying Chiang1、Ya-Hui Yang1 (1.Department of Space Science and Engineering, National Central University, Taiwan)
[PEM14-P05]Inconspicuous Solar Polar Coronal X-ray Jets as the Source of Conspicuous Hinode/EUV Imaging Spectrometer (EIS) Doppler Outflows
*Alphonse Sterling1、Conrad Schwanitz2,3、Louise K Harra2,3、Nour E Raouafi4、Navdeep K Panesar5,6、Ronald L Moore7,1 (1.NASA/MSFC, Huntsville, AL, 35812, USA、2.Institute for Particle Physics and Astrophysics, ETH, 8092 Zurich, Switzerland、3.Physikalisch Meteorologisches Observatorium Davos, World Radiation Center, 7260 Davos, Switzerland、4.The John Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA、5. Bay Area Environmental Research Institute, NASA Research Park, Moffett Field, CA 94035, USA、6.Lockheed Martin Solar and Astrophysics Laboratory, 3251 Hanover Street, Building 252, Palo Alto, CA 94304, USA、7.Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, Huntsville, AL 35805, USA)
[PEM14-P06]Solar p-mode as an additional energy source for coronal heating
*国吉 秀鷹1、リチャード モートン2、横山 央明3 (1.東京大学、2.ノーサンブリア大学、3.京都大学)
[PEM14-P07]Comprehensive simulation of solar wind formation from the solar interior
*飯島 陽久1、松本 琢磨1,2、堀田 英之3、今田 晋亮4 (1.名古屋大学、2.国立天文台、3.千葉大学、4.東京大学)
[PEM14-P08]Study on the time evolution of the electron acceleration site in a solar flare by using Time-of-Flight analysis method
*矢倉 昌也1、増田 智1 (1.名古屋大学)
[PEM14-P09]Verification of the inversion method for electric field and velocity on the photosphere
*野畑 昌浩1、金子 岳史2,3、草野 完也1 (1.名古屋大学宇宙地球環境研究所、2.LMSAL、3.HAO/NCAR)
[PEM14-P10]Investigating differences of magnetic fields in Solar active regions that produce eruptive and confined flares
*後藤 一郎1、草野 完也1、Leka KD1,2 (1.名古屋大学宇宙地球環境研究所、2.NorthWest Research Associates)