Structure and kinetic properties of slow-mode shocks associated with magnetic reconnection in the near-Earth magnetotail

被引:1
|
作者
Lin, Xi [1 ]
Deng, Xiaohua [1 ,2 ]
Yuan, Zhigang [1 ]
Zhou, Meng [2 ]
Li, Shiyou [1 ]
Pang, Ye [2 ]
机构
[1] Wuhan Univ, Sch Elect Informat, Wuhan 430079, Peoples R China
[2] Nanchang Univ, Inst Space Sci & Technol, Nanchang 330031, Peoples R China
基金
中国国家自然科学基金;
关键词
Slow-mode shock; Ion dynamics; Plasma wave; PLASMA SHEET BOUNDARY; CLUSTER OBSERVATIONS; ELECTRIC-FIELD; DISTANT; REGION; WALEN; TAIL;
D O I
10.1016/j.asr.2011.03.007
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
We study the structure and kinetic properties of slow-mode shocks near the plasma sheet boundary layer (PSBL) associated with magnetic reconnection by Cluster observation. The presence of slow-mode shocks is confirmed by traditional Rankine-Hugoniot (RI-I) analysis and Monte-Carlo shock fitting method. The Walen analysis, applied to the tailward flow associated with slow-mode shocks, also supports that plasma was accelerated across a Petschek-type slow-mode shock connected to the diffusion region. Back-streaming ions were observed on the shock layer, and cold ions were accelerated and heated by slow-mode shocks. In addition, whistler and electrostatic solitary waves were observed around the slow-mode shocks. These waves might be excited by the observed field-aligned electron beams near the shocks. (C) 2011 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:227 / 239
页数:13
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