日本地球惑星科学連合2014年大会

講演情報

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-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)

11:30 〜 11:45

[PEM29-09] 高マッハ数の準平行衝撃波における粒子加速

*加藤 恒彦1 (1.広島大学)

キーワード:粒子加速, プラズマ, 無衝突衝撃波

We study particle acceleration process of electrons and protons in high Mach number (MA~30) quasi-parallel collisionless shocks by particle-in-cell (PIC) simulation. We found that a fraction of protons which consist of the plasma are injected into acceleration mechanisms and efficiently accelerated around the shock. The energy spectrum of the accelerated protons becomes power-law like distribution. A part of electrons are also accelerated around the shock although they are roughly two orders of magnitude fewer than the accelerated protons. For both protons and electrons, the acceleration processes are often not diffusive and their time-scales are even shorter than the respective gyration times. We also found that protons reflected at the shock generate circularly polarized Alfven waves with very large amplitude in the upstream region of the shock and that, because of the strong perpendicular magnetic field of these waves, the structure of the collisionless shock itself is in fact similar to that of quasi-perpendicular shocks.