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The nature of the solar wind interaction with CO2/CO-dominated comets

✍ Scribed by Harry L. F. Houpis; D. A. Mendis


Publisher
Springer Netherlands
Year
1981
Tongue
English
Weight
689 KB
Volume
25
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