A global multispecies single-fluid MHD study of the plasma interaction around Venus

Author:

Ma Y. J.1,Nagy A. F.2,Russell C. T.1,Strangeway R. J.1,Wei H. Y.1,Toth G.2

Affiliation:

1. Institute of Geophysics and Planetary Physics, UCLA; Los Angeles California USA

2. Department of Atmospheric, Oceanic and Space Sciences; University of Michigan; Ann Arbor Michigan USA

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Reference38 articles.

1. A three-dimensional MHD study of solar wind mass loading processes at Venus: Effects of photoionization, electron impact ionization and charge exchange;Bauske;J. Geophys. Res.,1998

2. The effect of the hot oxygen corona on the interaction of the solar wind with Venus;Belotserkovskii;Geophys. Res. Lett.,1987

3. Effect of an extended neutral atmosphere on the interaction of the solar wind and the nonmagnetic bodies of the solar wind, I, Venus;Breus;Kosm. Issled.,1987

4. Three-dimensional MHD simulations of the interaction between Venus and the solar wind;Cable;J. Geophys. Res.,1995

5. Solar activity variations of the Venus thermosphere/ionosphere;Fox;J. Geophys. Res.,2001

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