Solar wind deceleration at Mars and Earth: A comparison

被引：4
|
作者：
Zhang, TL
Schwingenschuh, K
Riedler, W
Kotova, G
Verigin, M
Tatrallyay, M
Russell, CT
机构：
[1] IKI, MOSCOW, RUSSIA
[2] KFKI, BUDAPEST, HUNGARY
[3] UNIV CALIF LOS ANGELES, IGPP, LOS ANGELES, CA 90024 USA
来源：
PLANETARY IONOSPHERES AND MAGNETOSPHERES | 1997年 / 20卷 / 02期
关键词：
D O I：
10.1016/S0273-1177(97)00522-X
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Phobos 2 plasma measurements have revealed the solar wind deceleration upstream of the Martian terminator bow shock. Earlier studies have shown that the solar wind is decelerated and deflected in the Earth's foreshock region. At Mars, the solar wind decelerated more at duskside than at dawnside. At Earth the solar wind decelerates most upstream of the quasi-parallel bow shock in the foreshock region. In this paper, we investigate and compare the solar wind deceleration at Mars and Earth. (C) 1997 COSPAR. Published by Elsevier Science Ltd.
引用
收藏
页码：133 / 136
页数：4
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