Wave activity in the dayside mantle of Venus, Mars, and Titan

被引：5

作者：

Szego, K ^{[1
]}

Dóbé, Z

Huba, J

Quest, K

Shapiro, VD

机构：

[1] KFKI Res Inst Particle & Nucl Phys, Budapest, Hungary

[2] USN, Res Lab, Washington, DC 20375 USA

[3] Univ Calif San Diego, La Jolla, CA 92093 USA

来源：

PLANETARY IONOSPHERES AND MAGNETOSPHERES | 2000年 / 26卷 / 10期

关键词：

D O I：

10.1016/S0273-1177(00)00101-0

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

In this paper we analyse the properties of the waves excited in the interaction layer between the shocked solar wind and planetary plasma on the dayside of non-magnetic bodies. We compare the predictions of existing models for Venus, Mars, and Titan. It is concluded that the currently available measurements at Venus and Mars are not adequate to distinguish between the models, but at Titan the difference between the predictions is significant. (C) 2000 COSPAR. Published by Elsevier Science Ltd. All rights reserved.

引用

页码：1609 / 1612

页数：4

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