日本地球惑星科学連合2022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-EM16] 宇宙プラズマ理論・シミュレーション

2022年5月22日(日) 09:00 〜 10:30 105 (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)、コンビーナ: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)、コンビーナ: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)、三宅 洋平(神戸大学計算科学教育センター)

09:30 〜 09:45

[PEM16-03] Simulation study of the harmonic structure of lower hybrid wave due to energetic-ion injection under strong magnetic field

*小谷 翼1、樋田 美栄子2、森高 外征雄2田口 聡1 (1.京都大学理学研究科、2.核融合科学研究所)


キーワード:低域混成波の高調波、高速イオン駆動のイオンサイクロトロン波、高速イオン注入

Recently, it is reported that the harmonic structure of lower hybrid wave (referred to as harmonic LHW) is observed for the first time in the Earth’s magnetosphere. Here, the harmonic LHWs are characterized by their frequencies with ω = nωLH where n is an integer and ωLH is the lower hybrid resonance frequency. Although these harmonic LHWs are occasionally reported by some simulation studies, their excitation mechanism and influence on the surrounding plasma environment are not fully understood.
We investigate the excitation and non-linear development of the harmonic LHWs driven by ring-like energetic ions using one-dimensional, electromagnetic particle-in-cell simulations. To focus on the long-term evolution of the harmonic LHWs, we adopt an energetic-ion injection model in the simulations where the energetic ions are gradually injected into a plasma.
Our simulation results under strong magnetic field (ωpece = 0.25) show that the harmonic LHWs are excited by the non-linear interactions between the firstly excited LHWs with ω = nωLH and the harmonics of energetic-ion cyclotron waves (ICWs) with frequencies near ω = nωLH These results are also confirmed by bicoherence analysis which is widely used to diagnose the non-linear wave-wave coupling.