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Magnetic field and plasma inside and outside of the Martian magnetosphereSimultaneous magnetic and plasma measurements, carried out by wide angle plasma detectors in the Mars environment, are compared in order to identify regions with significantly different physical properties. Magnetograms and ion spectra indicate changes in the magnetopause and magnetosphere of Mars that are associated with the dynamic pressure effect of the solar wind.
Document ID
19760018038
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Dolginov, S. S. (Academy of Sciences (USSR) Moscow, Ussr)
Yeroshenko, Y. G. (Academy of Sciences (USSR) Moscow, Ussr)
Zhuzgov, L. N. (Academy of Sciences (USSR) Moscow, Ussr)
Sharova, V. A. (Academy of Sciences (USSR) Moscow, Ussr)
Gringauz, K. I. (Academy of Sciences (USSR) Moscow, Ussr)
Bezrukikh, V. V. (Academy of Sciences (USSR) Moscow, Ussr)
Breus, T. K. (Academy of Sciences (USSR) Moscow, Ussr)
Verigin, M. I. (Academy of Sciences (USSR) Moscow, Ussr)
Remizov, A. P. (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
Lunar And Planetary Exploration
Accession Number
76N25126
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 Mars19760018037Collected WorksSolar-wind interaction with the planets Mercury, Venus, and Mars
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