On the dayside region between the shocked solar wind and the ionosphere of Mars

Journal of Geophysical Research: Space Physics

Volumn 103, Issue A5, 1998, Pages 9101-9111

  Szego K ^a  

^a WIGNER RESEARCH CENTRE FOR PHYSICS   (Hungary)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0001226664     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: None     Document Type: Article

References (5)

1. Axford, W. I., A commentary of our present understanding of the Martian magnetosphere, Planet. Space Sci., 39, 167, 1991.
2. Brecht, S. H., Hybrid simulation of the magnetic topology of Mars, J. Geophys. Res., 102, 4743, 1997.
3. Brecht, S. H., J. R. Ferrante, and J. G. Luhmann, Three-dimensional simulations of solar wind interaction with Mars, J. Geophys. Res., 98, 1345, 1993.
4. Breus, T. K., and M. I. Verigin, The investigation of the solar wind plasma near Mars and during the Earth-Mars cruise phase using charged particle analyzers on Soviet spacecraft between 1971-1973, 4.Comparison of the plasma and magnetic field measurements of the Mars 2 space probe; Kosm. Issled. 14(3), 400, 1976.
5. Breus, T. K., S. J. Bauer, A. M. Krymskii, and V. Y. Mitnitskii, Mass loading in the solar wind interaction with Venus and Mars, J. Geophys. Res., 94, 2375, 1989.