Turbulent collective processes of new ions at Venus and Mars: problems of numerical models for the interaction between the solar wind and these planets. II. A two-fluid MHD model.

Details Turbulent collective processes of new ions at Venus and Mars: problems of numerical models for the interaction between the solar wind and these planets. II. A two-fluid MHD model. Turbulent collective processes of new ions at Venus and Mars: problems of numerical models for the interaction between the solar wind and these planets. II. A two-fluid MHD model.

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991cosre..29..370b&link_type=abstract

Cosmic Res., Vol. 29, No. 3, p. 370 - 379

Computer Science

Solar Wind: Venus Atmosphere, Solar Wind: Mars Atmosphere, Magnetohydrodynamics: Mars Atmosphere, Magnetohydrodynamics: Venus Atmosphere

Scientific paper

The authors present a numerical scheme and numerical results for flow around Venus and Mars using a two-fluid MHD model. The model includes anomalous drag between ion species (protons and O+ ions) due to turbulent acceleration processes in the transition region. They compare the numerical results with data from Pioneer-Venus-Orbiter and Phobos-2, and also with results from a one-dimensional MHD loading model. They find that their results agree better with the experimental data than the previous results do.

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