日本地球惑星科学連合2024年大会

講演情報

[E] 口頭発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM14] Frontiers in solar physics

2024年5月30日(木) 09:00 〜 10:15 201B (幕張メッセ国際会議場)

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)、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)、渡邉 恭子(防衛大学校)、座長:鳥海 森(宇宙航空研究開発機構 宇宙科学研究所)、渡邉 恭子(防衛大学校)


09:23 〜 09:45

[PEM14-02] FOXSI-4 Sounding Rocket Experiment: Solar Flare X-ray Focusing-Imaging Spectroscopic Observation

★Invited Papers

*成影 典之1,2、渡辺 伸3、高橋 忠幸4,5、長澤 俊作4,5、南 喬博5清水 里香2、佐藤 慶暉2坂尾 太郎3、加島 颯太3、三石 郁之6、作田 皓基6、安福 千貴6、藤井 隆登6、Lindsay Glesener7、Athanasios Pantazides7、Kristopher Cooper7、Yixian Zhang7、Juan Camilo Buitrago-Casas8、Juan Carlos Martinez Oliveros8、Hunter Kanniainen8、Savannah Perez Piel9、Tamar Ervin9、Orlando Romeo9、Sasha Courtade9、Wayne Baumgartner10、Stephen Bongiorno10、Patrick Champey10、Steven Christe11、Eliad Peretz11、Juliana Vievering12、Daniel Ryan13、Sam Krucker13草野 完也14 (1.国立天文台、2.総合研究大学院大学、3.宇宙航空研究開発機構、4.カブリIPMU、5.東京大学、6.名古屋大学、7.University of Minnesota Twin Cities、8.Space Sciences Laboratory、9.University of California Berkeley、10.NASA Marshall Space Flight Center、11.NASA Goddard Space Flight Center、12.Johns Hopkins University Applied Physics Laboratory、13.University of Applied Sciences and Arts Northwestern Switzerland FHNW、14.名古屋大学宇宙地球環境研究所)

キーワード:solar flare、magnetic reconnection、plasma heating、particle acceleration、imaging spectroscopy、X-rays

FOXSI-4 is a sounding rocket experiment to achieve the world's first solar flare X-ray focusing-imaging spectroscopic observation. The scientific objective of this experiment is to understand the mechanisms of energy release, energy conversion, and energy propagation in a solar flare driven by magnetic reconnection. The spatially and temporally resolved spectra in the soft to hard X-ray bands obtained by the FOXSI-4 allow detailed survey and diagnostics for plasmas heated to super-hot temperatures and accelerated electrons.
Since the observation time of the sounding rocket experiment was limited to about 5 minutes, it was almost impossible to observe solar flares, whose occurrence is difficult to predict. Thus, by monitoring the solar activity in real-time, the FOXSI-4 will be launched as soon as a flare occurs. In addition, to observe a large-scale flare, flare size will be predicted based on measured vector magnetic field data. The FOXSI-4 is planned to be launched in April 2024, together with the other sounding rocket of Hi-C FLARE, which will take high-spatial resolution EUV images.
In this presentation, an overview of the FOXSI-4 project is introduced and preliminary observation results are reported.