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The solar wind interaction with comet P/Grigg-Skjellerup

✍ Scribed by K. R. Flammer; D. A. Mendis; V. D. Shapiro; V. I. Shevchenko


Publisher
Springer Netherlands
Year
1993
Tongue
English
Weight
510 KB
Volume
60
Category
Article
ISSN
1573-0794

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We present the structure of the hermean magnetosphere obtained by a global three-dimensional MHD simulation. The magnetic field of Mercury is strong enough to form a permanent magnetosphere under typical solar wind conditions. Mercury does not have a substantial atmosphere or ionosphere which makes