日本地球惑星科学連合2021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-EM10] Frontiers in solar physics

2021年6月6日(日) 10:45 〜 12:14 Ch.06 (Zoom会場06)

コンビーナ:横山 央明(東京大学大学院理学系研究科)、今田 晋亮(名古屋大学宇宙地球環境研究所)、鳥海 森(宇宙航空研究開発機構 宇宙科学研究所)、Sterling Alphonse(NASA/MSFC)、座長:横山 央明(東京大学大学院理学系研究科)

11:29 〜 11:44

[PEM10-09] Current Status of the Solar-C_EUVST Mission

*今田 晋亮1、清水 敏文2、川手 朋子2、鳥海 森2、勝川 行雄3、久保 雅仁3、原 弘久3、Yoshinori Suematsu3、一本 潔4、浅井 歩4、渡邉 恭子6、横山 央明5、鄭 祥子2、Harry Warren7、David Long8、Louise Harra8、Luca Teriaca9、Sarah Matthews8、Vincenzo Andrette10、Frederic Auchere11 (1.名古屋大学宇宙地球環境研究所、2.宇宙科学研究所、3.国立天文台、4.京都大学、5.東京大学、6.防衛大学、7.NRL、8.UCL、9.MPS、10.Istituto Nazionale di Astrofisica、11.IAS)

Solar-C_EUVST (EUV High-Throughput Spectroscopic Telescope) is designed to comprehensively understand the energy and mass transfer from the solar surface to the solar corona and interplanetary space, and to investigate the elementary processes that take place universally in cosmic plasmas. As a fundamental step towards answering how the plasma universe is created and evolves, and how the Sun influences the Earth and other planets in our solar system, the proposed mission is designed to comprehensively understand how mass and energy are transferred throughout the solar atmosphere. Understanding the solar atmosphere, which connects to the heliosphere via radiation, the solar wind and coronal mass ejections, and energetic particles is pivotal for establishing the conditions for life and habitability in the solar system.

The two primary science objectives for Solar-C_EUVST are : I) Understand how fundamental processes lead to the formation of the solar atmosphere and the solar wind, II) Understand how the solar atmosphere becomes unstable, releasing the energy that drives solar flares and eruptions. Solar-C_EUVST will, A) seamlessly observe all the temperature regimes of the solar atmosphere from the chromosphere to the corona at the same time, B) resolve elemental structures of the solar atmosphere with high spatial resolution and cadence to track their evolution, and C) obtain spectroscopic information on the dynamics of elementary processes taking place in the solar atmosphere.

In this talk, we will first discuss the science target of the Solar-C_EUVST, and then discuss the current status of the Solar-C_EUVST mission.