日本地球惑星科学連合2024年大会

講演情報

[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-EM17] 宇宙プラズマ科学

2024年5月30日(木) 13:45 〜 15:15 101 (幕張メッセ国際会議場)

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(神戸大学大学院システム情報学研究科)、諌山 翔伍(九州大学総合理工学研究院)、梅田 隆行(北海道大学 情報基盤センター)、座長:天野 孝伸(東京大学 地球惑星科学専攻)、松清 修一(九州大学大学院総合理工学研究院)

14:00 〜 14:15

[PEM17-02] Electromagnetic particle simulation of nonlinear wave growth process of whistler-mode hiss emissions in the magnetosphere

*殷 振興1,2大村 善治1,2謝 怡凱1,2 (1.京都大学、2.京都大学生存圏研究所)

キーワード:非線形成長、ホイッスラーモード・ヒス、磁気圏プラズマ

We perform a series of electromagnetic particle simulations in the magnetospheric plasma for studying the nonlinear wave growth of hiss emissions. We examine dependency of the nonlinear growth rates on the gradient of the background magnetic field by varying the gradient of the background magnetic field from zero. At the same time we add a frequency band filter to focus on specific frequency range.
We find that in the case of the zero gradient the wave amplitude attains the smallest value compared with other cases of finite gradients. There is an optimum value with which wave amplitude grows to the largest value. To gain a deeper insight into this phenomenon, we compute and visualize both the growth rate and nonlinear growth rate throughout the process of wave generation and propagation. We observe a remarkable growth rate in the wave generation process at the system's boundary. Interestingly, we find that this growth rate remained nearly constant with no apparent variations, even when we manipulated the background magnetic field gradient. The investigation into whether the amplitude of the wave exhibits linear or nonlinear growth, or if it assumes nonphysical behavior during this process, constitutes a compelling topic for future research.