Pioneer Venus Plasma Wave Observations: The Solar Wind-Venus Interaction

被引：74

作者：

Scarf, F. L. ^{[1
]}

Taylor, W. W. L. ^{[1
]}

Russell, C. T. ^{[2
]}

Elphic, R. C. ^{[2
]}

机构：

[1] TRW Def & Space Syst Grp, Dept Space Sci, Redondo Beach, CA 90278 USA

[2] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90024 USA

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 1980年 / 85卷 / A13期

关键词：

D O I：

10.1029/JA085iA13p07599

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We briefly describe the Pioneer Venus plasma wave instrument and continue with a discussion wave observations throughout the typical near-noon and near-midnight orbits This is followed by a detailed comparison of the bow shock turbulence characteristics at earth and at, Venus. We then turn to analyze the wave-particle interactions detected near the dayside ionopause, and we show Chit the whistler mode, Landau damping develops when the B field direction changes so that the whistler becomes oblique.

引用

页码：7599 / 7612

页数：14

共 21 条

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