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Unipolar interaction of Mercury with the solar wind; the steady state bow shock problem

✍ Scribed by D.S. Colburn; C.P. Sonett; K. Schwartz


Book ID
115853180
Publisher
Elsevier Science
Year
1972
Tongue
English
Weight
905 KB
Volume
14
Category
Article
ISSN
0012-821X

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Interaction of Mercury with the Solar Wi
✍ K. Kabin; T.I. Gombosi; D.L. DeZeeuw; K.G. Powell πŸ“‚ Article πŸ“… 2000 πŸ› Elsevier Science 🌐 English βš– 590 KB

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