VENUS IONOSPHERE' AN INTERPRETATION OF MARINER 10 OBSERVATIONS

被引：52

作者：

Bauer, S. J. ^{[1
]}

Hartle, R. E. ^{[1
]}

机构：

[1] NASA, Goddard Space Flight Ctr, Lab Planetary Atmospheres, Greenbelt, MD 20771 USA

来源：

GEOPHYSICAL RESEARCH LETTERS | 1974年 / 1卷 / 01期

关键词：

D O I：

10.1029/GL001i001p00007

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

The dayside ionosphere of Venus observed by Mariner 10 may be understood in terms of a dyhamic interaction with the solar wind which results in a compressed topside above an "F-2 ledge" consisting of O+ and a dynamically unaffected F-1 layer corresponding to a neutral temperature T similar or equal to 380 degrees K and consisting of O-2(+) and CO2+. The top of the upper ledge appears to be an ionopause caused by solar wind scavenging of He+, representing a solar-wind obstacle consistent with the bow shock observations.

引用

页数：3

共 10 条

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[10]

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