Turbulent collectivization processes of new ions near Venus and Mars, and problems of numerical modeling of solar wind interaction with these planets. II - A two-fluid MHD model

Details Turbulent collectivization processes of new ions near Venus and Mars, and problems of numerical modeling of solar wind interaction with these planets. II - A two-fluid MHD model Turbulent collectivization processes of new ions near Venus and Mars, and problems of numerical modeling of solar wind interaction with these planets. II - A two-fluid MHD model

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kosis..29..432b&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 29, May-June 1991, p. 432-442. In Russian.

Computer Science

Magnetohydrodynamic Turbulence, Mars (Planet), Solar Planetary Interactions, Solar Wind, Two Fluid Models, Venus (Planet), Ionic Reactions, Magnetohydrodynamic Waves, Magnetosheath, Neutral Atmospheres, Photoionization, Planetary Atmospheres

Scientific paper

A two-fluid MHD model with anomalous friction between ion species due to turbulence in the magnetosheath is proposed for the solar wind interaction with Venus and Mars. The method for calculations and their results for both planets are given. The results are compared with experimental data from the Pioneer-Venus and Phobos-2 spacecraft and also with the results of the one-fluid MHD mode, with mass loading. The results of the two-fluid MHD model are in better agreement with the experimental data than those obtained earlier.

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