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)


09:01 〜 09:23

[PEM14-01] Coronal heating under various stellar environments

★Invited Papers

*鷲ノ上 遥香1 (1.大阪大学)

キーワード:太陽コロナ、恒星コロナ、磁気流体数値計算

In the context of the solar-stellar connection, it is necessary to understand the mechanism of coronal heating and coronal activity across diverse stellar conditions. In particular, we focus on the effect of stellar metallicity in coronal heating because it affects the energy loss through radiation in the atmosphere. For this, we study the heating of stellar coronal loops, which are the basic building blocks of the coronal atmosphere, by one-dimensional magnetohydrodynamic simulations. Our simulations have revealed that metallicity has a nonnegligible impact on physical and radiative properties of stellar coronae. To unite the modeling for solar and other stellar coronae, we derived the scaling relations for a hydrostatic coronal loop from the energy balance among heating, radiative cooling and thermal conduction, as an extension of the RTV scaling laws for the Sun. This generalization allows us to characterize the coronal properties under a wide variety of stellar environment.