Effect of the interplanetary magnetic field on flow in the vicinity of the daytime magnetopause

Details Effect of the interplanetary magnetic field on flow in the vicinity of the daytime magnetopause Effect of the interplanetary magnetic field on flow in the vicinity of the daytime magnetopause

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..526a&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, May-June 1991, p. 526-528. In Russian.

Physics

Interplanetary Magnetic Fields, Magnetopause, Solar Terrestrial Interactions, Solar Wind Velocity, Earth Magnetosphere, Magnetohydrodynamic Flow

Scientific paper

The interaction between the solar wind and the earth's magnetosphere is investigated theoretically on the basis of the solution of the MHD equation. Corrections to the gasdynamic flow due to the magnetic field are obtained on using an analytical expression for the Ampere force obtained in the zeroth, kinematic approximation. The total pressure across the dissipative region in the vicinity of the magnetopause is shown to be conserved.

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