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-EM13] Dynamics of the Inner Magnetospheric System

2024年5月26日(日) 10:45 〜 12:00 105 (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)、Sarris E Sarris(Democritus University of Thrace)、Thomas G Thomas(Dartmouth College)、座長:山本 和弘(東京大学理学研究科)、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)


11:15 〜 11:30

[PEM13-08] Variations of energetic electrons via nonlinear interactions with lower-band chorus emissions around the Earth’s outer radiation belt

*謝 怡凱1大村 善治1 (1.京都大学生存圏研究所)

キーワード:非線形波動粒子相互作用、ホイッスラーモード・コーラス放射、電子加速、電子降下

Energetic electron accelerations and precipitations in the Earth's outer radiation belt are highly associated with wave-particle interactions between whistler mode chorus waves and electrons. Two nonlinear processes, which change the energy and pitch angle of electrons effectively, take place in whistler mode wave-particle interactions. One is the nonlinear scattering, which makes electron energy slightly smaller. The other is the nonlinear trapping, which makes effective energy gain of the resonant electrons. We utilized the Green's function method to reproduce the wave-particle interactions in the radiation belt and investigate the electron acceleration and precipitation interacting with both parallel and obliquely propagating chorus emissions. The formation processes and the loss processes of the outer radiation belt electron fluxes interacting with consecutive chorus emissions are traced by applying the convolution integrals for the Green's functions. In the acceleration parts, MeV electrons are generated promptly due to the combination of cyclotron resonance and Landau resonance of oblique chorus waves. We compare the precipitation phenomena between parallel waves and oblique waves, and the results show that oblique chorus emissions lead to more electron precipitation than that led by parallel chorus emissions. Furthermore, we found that the acceleration process is stronger than the loss process, indicating that the radiation belt becomes stronger under the wave-particle interaction between chorus emissions and electrons comprehensively.