Infuence of the solar wind magnetic field on the structure of the magnetosheath and the location of the magnetopause

Details Infuence of the solar wind magnetic field on the structure of the magnetosheath and the location of the magnetopause Infuence of the solar wind magnetic field on the structure of the magnetosheath and the location of the magnetopause

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8318633p&link_type=abstract

Influence of the solar wind magnetic field on the structure of the magnetosheath and the location of the magnetopause

Physics

Interplanetary Magnetic Fields, Magnetic Effects, Magnetopause, Magnetosheath, Plasmasphere, Solar Wind, Space Plasmas, Bow Waves, Continuity Equation, Displacement, Equations Of Motion, Magnetohydrodynamic Flow, Plasma Density, Shock Waves, Stagnation Point

Scientific paper

The variations of the plasma parameters and of the magnetic field in the vicinity of the stream line passing the subsolar point at the magnetopause are calculated using a special topology of the plasma flow which is the result of the formation of a stagnation line at the nose part of the magnetopause. The displacement of the magnetopause due to the penetration of the solar wind magnetic field is discussed.

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