日本地球惑星科学連合2019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] 宇宙プラズマ理論・シミュレーション

2019年5月30日(木) 15:30 〜 17:00 A03 (東京ベイ幕張ホール)

コンビーナ:梅田 隆行(名古屋大学 宇宙地球環境研究所)、天野 孝伸(東京大学 地球惑星科学専攻)、成行 泰裕(富山大学人間発達科学部)、中村 匡(福井県立大学)、座長:中村 匡(福井県立大学)、成行 泰裕

15:30 〜 15:45

[PEM17-07] Stochastic models of phase space diffusion via wave-particle interaction with parallel propagating electromagnetic waves

*成行 泰裕1 (1.富山大学人間発達科学部)

キーワード:粒子拡散、波動粒子相互作用、確率モデル、ホイッスラー波、磁気流体波

Particle diffusion due to electromagnetic waves is one of fundamental processes in various phenome in space plasms such as electron acceleration in the outer radiation belt [e.g., Saito et al, JGR, 2016], astrophysical shock [e.g., Yamazaki, JHEA, 2015], and solar wind [e.g., Seough et al, APJ, 2015]. Although quasi-linear theories are widely used as a standard theory of particle scattering, nonlinear wave-particle interactions such as particle trapping also affect particle diffusions in the presence of finite amplitude waves. Saito et al [JGR, 2016] demonstrated that nonlinearity of whistler chorus waves plays a significant role in electron diffusion though nonlinear wave-particle interactions.

In Saito et al [JGR, 2016], the artificial randomization of gyrophases (phase breaking) is incorporated to discuss suppression of coherent wave-particle interactions. Remark that such a randomization corresponds to a noise term in equations of motion of each particles. In this sense, phase breaking causes not only the suppression of coherent processes but also diffusions in phase space. In the present study, we discuss the generalization of phase breaking. It is shown that particle diffusion depends on probability density functions of noises and their parameters. Noise terms in equations of the pitch angle are also necessary to describe diffusion in phase space. Treatment of phase breaking as a stochastic differential equation is also discussed.