Features of MHD flow about the magnetosphere near the stagnation point

Details Features of MHD flow about the magnetosphere near the stagnation point Features of MHD flow about the magnetosphere near the stagnation point

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..705e&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, Sept.-Oct. 1986, p. 705-709. In Russian.

Computer Science

Earth Magnetosphere, Magnetohydrodynamic Flow, Solar Terrestrial Interactions, Solar Wind, Asymptotic Methods, Differential Equations, Plasma Density, Stagnation Point

Scientific paper

A theoretical study of solar wind flow about the earth magnetosphere in the magnetic barrier region is presented. An analytical solution of the asymptotic (with respect to the Mach-Alfven number) equations describing the magnetic barrier structure is obtained for the vicinity of the stagnation point. Variations of MHD parameters near the magnetic barrier are studied, and a comparison is made with the numerical solution.

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