The martian plasma environment: Electric field and Langmuir probe diagnostics

被引:1
|
作者
Blomberg, LG [1 ]
Cumnock, JA
Eriksson, AI
机构
[1] Royal Inst Technol, Alfven Lab, SE-10044 Stockholm, Sweden
[2] Univ Texas, William B Hanson Ctr Space Sci, Richardson, TX 75083 USA
[3] Swedish Inst Space Phys, SE-75121 Uppsala, Sweden
关键词
extraterrestrial plasmas; ionosphere; planetary atmospheres; planets; plasma measurements;
D O I
10.1109/TPS.2003.821353
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
The plasma environment of Mars has been studied by a small handful of spacecraft. From the sparse observations that exist, one may conclude that the solar wind-Martian "magnetosphere" interaction is different in significant ways from the solar wind's interaction with Earth's magnetosphere. Mars offers an opportunity to make significant advances in our understanding of the fundamentals of the solar wind's interaction with cold celestial bodies, with suitable plasma instrumentation orbiting the planet. We briefly review what is known about Mars' plasma environment and address some scientific topics that can be studied by proper plasma instrumentation in Mars' vicinity, in particular the scientific potential of Langmuir probe measurements. Finally, we exemplify how the studies may contribute to an enhanced understanding not only of the plasma surrounding Mars, but also of the planet itself and its neutral atmosphere.
引用
收藏
页码:1232 / 1236
页数:5
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