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Solar wind interaction with the tail of Comet Kohoutek

✍ Scribed by A.I. Ershkovich


Publisher
Elsevier Science
Year
1976
Tongue
English
Weight
520 KB
Volume
24
Category
Article
ISSN
0032-0633

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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