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Numerical simulation of the effects of magnetic field induced by plasma flow past nonmagnetic planetsThe interaction of a nonstationary plasma flow with a model ionosphere is studied. On the basis of a numerical simulation, the calculation yields results of the distribution of the plasma concentration and magnetic field in the transition region.
Document ID
19760018049
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Lipatov, A. S. (Academy of Sciences (USSR) Moscow, Ussr)
Date Acquired
August 8, 2013
Publication Date
January 1, 1976
Publication Information
Publication: NASA. Goddard Space Flight Center Solar-Wind Interaction with the Planets Mercury, Venus, and Mars
Subject Category
Astrophysics
Accession Number
76N25137
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19760018037Collected WorksSolar-wind interaction with the planets Mercury, Venus, and Mars
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