Some problems of the solar wind interaction with Venus

Details Some problems of the solar wind interaction with Venus Some problems of the solar wind interaction with Venus

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987p%26ss...35.1213b&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 35, Sept. 1987, p. 1213-1219.

Physics

6

Atmospheric Ionization, Ionopause, Photoionization, Planetary Magnetospheres, Plasma Interactions, Solar Planetary Interactions, Solar Wind, Venus Atmosphere, Atmospheric Models, Magnetohydrodynamic Flow, Magnetohydrodynamic Stability, Magnetosheath, Mass Distribution, Venus, Solar Wind, Interaction, Mass Loading, Corona, Photoionization, Plasma, Flow, Parameters, Oxygen, Magnetosheath, Stability, Symmetry, Analysis, Magnetic Fields, Ionopause, Distance, Shock, Calculations, Atmosphere, Thickness, Turbulenc

Scientific paper

The aim of this paper is to analyze the effect of solar wind mass-loading due to hot-oxygen Venus corona photoionization on the plasma flow parameters in the nose part of the magnetosheath and the flow stability, taking into consideration the axial symmetry of the flow. The analysis has shown that the mass-loading effect increases the distance between the shock front and the ionopause and reduces the maximum magnetic field strength in the magnetic barrier in the vicinity of the stagnation region of the ionopause. The axial symmetry of the stream stabilizes the ionopause disturbances in the nose part. For shorter wavelengths the instability problem should be investigated numerically and should account for the stabilizing effect of the finite Larmor ion radius.

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