日本地球惑星科学連合2025年大会

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[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-EM13] Dynamics of the Inner Magnetospheric System

2025年5月28日(水) 15:30 〜 17:00 302 (幕張メッセ国際会議場)

コンビーナ:桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)、三好 由純(名古屋大学宇宙地球環境研究所)、Goldstein Jerry(Southwest Research Institute)、Sun YIXIN(Peking University)、Chairperson:Claudia Martinez-Calderon(Nagoya University)、三好 由純(名古屋大学宇宙地球環境研究所)、桂華 邦裕(東京大学大学院理学系研究科地球惑星科学専攻)


16:10 〜 16:30

[PEM13-17] Electron Precipitation driven by Chorus Wave in the Earth’s inner magnetosphere

*Xueyi Wang1、Huayue Chen1Lunjin ChenYoshiharu OmuraYikai Hsieh (1.Auburn University)

キーワード:chorus wave, particle simulation, electron precipitation

Particle precipitation is a significant energy input into the Earth’s ionosphere and plays an important role in magnetosphere-ionosphere coupling. Previous studies employed test particle simulations to investigate wave-particle interaction and associated precipitation, in which the wave evolution is presumed and the particle feedback to waves is neglected. In this study, we employ a self-consistent simulation model, GCPIC (the general curvilinear plasma simulation code), to investigate particle precipitation in a dipole magnetic field. It is found that the quasi-periodic, energy-dispersive electron precipitation is driven by chorus waves, with the electron precipitation period aligning with that of chorus waves. Moreover, the fine structures within the precipitation spectrogram are identified, and are consistent with the high-frequency modulation of precipitation in observation. The chorus wave modulated by ULF wave and background plasma density and associated electron “on” and “off” precipitation has been investigated.