Hermean magnetosphere-solar wind interaction

被引:40
|
作者
Fujimoto, M. [2 ]
Baumjohann, W. [1 ]
Kabin, K. [3 ]
Nakamura, R. [1 ]
Slavin, J. A. [4 ]
Terada, N. [5 ]
Zelenyi, L. [6 ]
机构
[1] Austrian Acad Sci, Space Res Inst, A-8010 Graz, Austria
[2] Inst Space & Astronaut Sci, Sagamihara, Kanagawa 229, Japan
[3] Univ Alberta, Edmonton, AB, Canada
[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[5] NiCT, Koganei, Tokyo, Japan
[6] Russian Acad Sci, Inst Space Res, Moscow V71, Russia
关键词
Mercury; magnetosphere; substorm; solar wind;
D O I
10.1007/s11214-007-9245-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The small intrinsic magnetic field of Mercury together with its proximity to the Sun makes the Hermean magnetosphere unique in the context of comparative magnetosphere study. The basic framework of the Hermean magnetosphere is believed to be the same as that of Earth. However, there exist various differences which cause new and exciting effects not present at Earth to appear. These new effects may force a substantial correction of our naive predictions concerning the magnetosphere of Mercury. Here, we outline the predictions based on our experience at Earth and what effects can drastically change this picture. The basic structure of the magnetosphere is likely to be understood by scaling the Earth's case but its dynamic aspect is likely modified significantly by the smallness of the Hermean magnetosphere and the substantial presence of heavy ions coming from the planet's surface.
引用
收藏
页码:529 / 550
页数:22
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