日本地球惑星科学連合2014年大会

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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-EM29_30AM2] プラズマ宇宙:波動粒子相互作用,粒子加速,相対論的プラズマ

2014年4月30日(水) 11:00 〜 12:45 503 (5F)

コンビーナ:*松清 修一(九州大学大学院総合理工学研究院流体環境理工学部門)、永岡 賢一(核融合科学研究所)、座長:中村 匡(福井県立大学)

11:00 〜 11:15

[PEM29-07] 平行衝撃波での上流波と粒子加速の共進現象

*杉山 徹1藤本 正樹2 (1.海洋研究開発機構、2.宇宙航空研究開発機構)

キーワード:無衝突衝撃波, 粒子加速, 波動粒子相互作用

We have investigated the co-evolution of upstream waves and the accelerated particles around the parallel shock. Hybrid particle simulations are performed in the exactly parallel shock configuration with Mach number of ~10. The upstream waves convecting into the shock surface contribute the particles acceleration as reported in Sugiyama et al. (2001). The appropriate wave-length exists for the particle energization, that is, the longer wave-length wave leads the higher energy particles. Simultaneously, the higher energized particles excite the longer wave-length waves in the upstream region. Here we report that the higher energy particles and longer wave-length waves are observed as the time elapses later in the simulation runs. Therefore, the present process is "co-evolution" of the upstream waves and accelerated particles.