Mirror waves and mode transition observed in the magnetosheath by Double Star TC-1

被引：4
|
作者：
Du, J. [1 ]
Wang, C. [1 ]
Zhang, T. L. [2 ]
Volwerk, M. [2 ]
Carr, C. [3 ]
机构：
[1] Chinese Acad Sci, Ctr Space Sci & Appl Res, State Key Lab Space Weather, Beijing, Peoples R China
[2] Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria
[3] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London, England
来源：
ANNALES GEOPHYSICAE | 2009年 / 27卷 / 01期
基金：
美国国家科学基金会;
关键词：
Magnetospheric physics; Magnetosheath; MHD waves and instabilities; Solar wind-magnetosphere interactions; LOW-FREQUENCY FLUCTUATIONS; ANISOTROPY INSTABILITIES; EARTHS MAGNETOSHEATH; EQUATOR-S; IDENTIFICATION; PERFORMANCE;
D O I：
10.5194/angeo-27-351-2009
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The Double Star TC-1 magnetosheath pass on 26 February 2004 is used to investigate magnetic field fluctuations. Strong compressional signatures which last for more than an hour have been found near the magnetopause behind a quasi-perpendicular bow shock. These compressional structures are most likely mirror mode waves. There is a clear wave transition in the magnetosheath which probably results from the change of the interplanetary magnetic field (IMF) cone angle. The wave characteristics in the magnetosheath are strongly controlled by the type of the upstream bow shock.
引用
收藏
页码：351 / 355
页数：5
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