JpGU-AGU Joint Meeting 2017

講演情報

[JJ] 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-EM21] [JJ] 宇宙プラズマ理論・シミュレーション

2017年5月24日(水) 15:30 〜 17:00 A01 (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)、成行 泰裕(富山大学人間発達科学部)、三宅 洋平(神戸大学計算科学教育センター)、中村 匡(福井県立大学)、座長:梅田 隆行(名古屋大学 宇宙地球環境研究所)、座長:成行 泰裕(富山大学人間発達科学部)

16:30 〜 16:45

[PEM21-05] Cyclic self-reformation of perpendicular shocks in two-dimensional particle-in-cell simulation

*梅田 隆行1大長 勇輝1 (1.名古屋大学 宇宙地球環境研究所)

キーワード:無衝突衝撃波、粒子シミュレーション

The cyclic self-reformation of perpendicular collisionless shocks was first identified in one-dimensional (1D) kinetic particle-in-cell simulations. In early studies, the reformation was defined as the cyclic accumulation and release of ions. The release ions toward upstream (ion reflection) takes place periodically at the ion gyro period of the downstream, which forms the shock foot region. Later, the cyclic self-reformation of perpendicular shocks was also identified in two-dimensional (2D) full particle-in-cell simulations with a simulation domain shorter than the ion inertial length in the shock tangential direction. However, some of recent 2D full particle-in-cell simulations with a large simulation domain argued against the evidence of the cyclic self-reformation of perpendicular shocks due to rippled structures at the shock front. In the previous studies, the cyclic self-reformation was identified from the cyclic oscillation of the magnetic field at overshoot, since the magnetic field and the ion density are well correlated in 1D simulations and 2D simulations with a small simulation domain. In the present study, we analyze ion particle data obtained from large-scale 2D full particle-in-cell simulations with different ion-to-electron mass ratio, and discuss the effect of the mass ratio to the evidence of the cyclic self-reformation of perpendicular shocks.