日本地球惑星科学連合2021年大会

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[J] 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-EM15] 宇宙プラズマ理論・シミュレーション

2021年6月4日(金) 09:00 〜 10:30 Ch.06 (Zoom会場06)

コンビーナ:天野 孝伸(東京大学 地球惑星科学専攻)、三宅 洋平(神戸大学計算科学教育センター)、梅田 隆行(名古屋大学 宇宙地球環境研究所)、中村 匡(福井県立大学)、座長:天野 孝伸(東京大学 地球惑星科学専攻)、岩本 昌倫(九州大学総合理工学研究院)

09:15 〜 09:30

[PEM15-02] Simulation for wave-particle interactions of triggered emissions in a uniform magnetic field

*藤原 悠也1、野儀 武志1、大村 善治1 (1.京都大学生存圏研究所)

キーワード:ホイッスラーモード波動、トリガード放射、PICシミュレーション

One-dimensional electromagnetic particle simulations were performed for the study of nonlinear process of the whistler-mode triggered emissions in a uniform magnetic field. We put cold and hot electrons initialized by bi-Maxwellian and subtracted bi-Maxwellian distributions, respectively. Driving two orthogonally aligned antennas by right-handed polarized external currents oscillating with frequencies below the electron cyclotron frequency, we generate whistler-mode triggering waves in the simulation system. We report the characteristics of the triggered emissions in terms of the duration and frequency of the triggering wave. In the cases with rising-tone emissions, we analyze dynamics of resonant electrons in the velocity phase space based on the nonlinear wave growth theory. We find that the formation of an electron hole generates rising-tone emissions after the termination of the triggering waves. In the present study, we discuss the initial process of the formation of an electron hole and hill during triggering waves, which causes frequency variations from the constant triggering frequency.