Interstellar pickup hydrogen observations at large heliocentric distances

被引:10
|
作者
Mihalov, JD [1 ]
Gazis, PR [1 ]
机构
[1] NASA, Planetary Syst Branch, Ames Res Ctr, Moffett Field, CA 94035 USA
关键词
D O I
10.1029/97GL03785
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Possible signatures of interstellar pickup hydrogen have been identified in data from the Pioneer 10 and 11 Ames plasma analyzers at locations out to beyond the orbit of Saturn, and at a wide range of longitudes in the heliosphere, both upstream and downstream in the interstellar wind. These signatures provide an extension of pickup ion observations out to beyond 15 AU heliocentric distance, including near where the maximum pickup hydrogen flux is expected. A depletion of interstellar pickup hydrogen downstream from the Sun in the interstellar flow may be indicated. These signatures are consistent with Ulysses pickup ion measurements.
引用
收藏
页码:241 / 244
页数:4
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