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-EM37_30PM2] 磁気圏構造とダイナミクス

2014年4月30日(水) 16:15 〜 17:30 414 (4F)

コンビーナ:*三好 由純(名古屋大学太陽地球環境研究所)、長谷川 洋(宇宙航空研究開発機構宇宙科学研究所)、座長:三好 由純(名古屋大学太陽地球環境研究所)、藤田 茂(気象庁気象大学校)

17:00 〜 17:15

[PEM37-P08_PG] 小型ダイポール磁場とプラズマ流の相互作用に関する3次元粒子シミュレーション

ポスター講演3分口頭発表枠

*臼井 英之1芦田 康将2篠原 育3中村 雅夫4山川 宏2三宅 洋平1 (1.神戸大学大学院システム情報学研究科、2.京都大学生存圏研究所、3.宇宙航空研究開発機構/宇宙科学研究所、4.大阪府立大学)

キーワード:磁気ダイポール, メソスケール, プラズマ応答, 境界電流層, プラズマ粒子シミュレーション

Plasma flow response to a magnetic dipole and the resulting formation of a magnetosphere depends on the intensity of the magnetic moment of the dipole. In this study, we examined plasma flow interactions with a magnetic dipole which is much smaller than the Earth's intrinsic magnetic dipole by performing three-dimensional full Particle-In-Cell simulations. The size of a magnetic dipole immersed in a plasma flow is characterized by distance L from its center at which the equilibrium is satisfied between the pressure of the magnetic field of the dipole and that of the plasma flow. In the Earth's magnetosphere, L implies the magnetopause location. We particularly focused on meso- and micro-scale magnetic dipoles in which L is comparable to and smaller than the gyroradius of ions in the flow. In the meso-scale case, ions kinetics should be dominantly considered while electrons whose gyroradius is sufficiently small can be treated as fluid. In the micro-scale, however, electrons as well as ions should be treated particles because L becomes small and the electron kinetics cannot be ignored either. Our interest is in the formation of current layer at the magnetosphere boundary in the both scales. Corresponding to the formation of a magnetosphere, the boundary current also depends on the size of the magnetosphere.
In the meso-scale case, the boundary current is dominated by the electron diamagnetic current at the large density gradient found at the distance of L. This signature is similar to the case of the Earth's magnetosphere. In the micro-scale case, however, the trajectories of ions and electrons gyration play an important role to determine the boundary current. Since the ion's gyroradius is larger than L, charge separation between ions and electrons occurs in the upstream region. As particles approach to the inner dipole, the electron gyroradius becomes small and electron drift motion becomes dominant. It is also confirmed that static electric field caused by the charge separation affect the plasma dynamics and the resulting current flow.