Concerning the problem of a magnetic boundary on Venus

Details Concerning the problem of a magnetic boundary on Venus Concerning the problem of a magnetic boundary on Venus

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982kosis..20...97p&link_type=abstract

Kosmicheskie Issledovaniia, vol. 20, Jan.-Feb. 1982, p. 97-103. In Russian.

Mathematics

Boundary Layer Plasmas, Magnetopause, Planetary Magnetic Fields, Planetary Magnetospheres, Plasma Interactions, Solar Wind, Venus Atmosphere, Magnetohydrodynamic Flow, Mathematical Models, Planetary Ionospheres, Plasma Diffusion

Scientific paper

The paper examines the characteristics of the plasma shell boundary of Venus, produced by the interaction of the solar wind with the planet's ionosphere. A mathematical model of plasma flow past bodies is used to provide an analytical description of the magnetic boundary of Venus, and theoretical calculations of the characteristics of the boundary are compared with experimental data.

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