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The electromagnetic effects of the solar wind interaction with Phobos

✍ Scribed by M.K. Dougherty; A.M. Krymskii; T.K. Breus; D.J. Southwood; W.I. Axford


Publisher
Elsevier Science
Year
1993
Tongue
English
Weight
301 KB
Volume
13
Category
Article
ISSN
0273-1177

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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