A study of the solar wind deceleration in the earth's foreshock region

被引：22

作者：

Zhang, TL ^{[1
]}

Schwingenschuh, K ^{[1
]}

Russell, CT ^{[1
]}

机构：

[1] UNIV CALIF LOS ANGELES,IGPP,LOS ANGELES,CA

来源：

PHYSICS OF COLLISIONLESS SHOCKS | 1995年 / 15卷 / 8-9期

基金：

美国国家航空航天局;

关键词：

D O I：

10.1016/0273-1177(94)00095-I

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

Previous observations have shown that the solar wind is decelerated and deflected in the earth's upstream region populated by long-period waves /1-3/. This deceleration is correlated with the 'diffuse' but not with the 'reflected' ion population. The speed of the solar wind may decrease tens of km/s in the foreshock region. The solar wind dynamic pressure exerted on the magnetopause may vary due to the fluctuation of the solar wind speed and density in the foreshock region. In this study, we examine this solar wind deceleration and determine how the solar wind deceleration varies in the foreshock region.

引用

页码：137 / 140

页数：4

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