The magnetosheath

被引：93

作者：

Lucek, EA

Constantinescu, D

Goldstein, ML

Pickett, J

Pinçon, JL

Sahraoui, F

Treumann, RA

Walker, SN

机构：

[1] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, London, England

[2] Tech Univ Braunschweig, Inst Geophys & Extraterr Phys, D-3300 Braunschweig, Germany

[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[4] Univ Iowa, Dept Phys & Astron, Iowa City, IA 52242 USA

[5] CNRS, LPCE, F-45071 Orleans, France

[6] IPSL, CETP, Velizy Villacoublay, France

[7] Max Planck Inst Extraterr Phys, D-37075 Garching, Germany

[8] Univ Sheffield, Sheffield, S Yorkshire, England

来源：

SPACE SCIENCE REVIEWS | 2005年 / 118卷 / 1-4期

基金：

美国国家航空航天局;

关键词：

D O I：

10.1007/s11214-005-3825-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The properties of magnetosheath, which lies between the bow shock and the magnetopause and is formed mainly from decelerated and deflected solar wind, are discussed. Magnetosheath seems to arise from the bouncing of particles between the shock and an oblique discontinuity, as the discontinuity tracks across the shock carried by the solar wind flow. The magnetosheath plasma parameters show both large scale spatial ordering, imposed by the shape of the magnetopause, and variability dependent on the solar wind input. The shocks, whether quasi-perpendicular or quasi-parallel, affects the properties of the magnetosheath plasma.

引用

页码：95 / 152

页数：58

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