Solar-wind parameters in the transition region in a model with a magnetic barrier

Details Solar-wind parameters in the transition region in a model with a magnetic barrier Solar-wind parameters in the transition region in a model with a magnetic barrier

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27...22p&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Jan.-Feb. 1987, p. 22-27. In Russian.

Astronomy and Astrophysics

Astronomy

3

Astronomical Models, Earth Magnetosphere, Magnetic Field Configurations, Plasma Dynamics, Solar Terrestrial Interactions, Solar Wind Velocity, Interplanetary Magnetic Fields, Magnetic Flux, Plasma Density, Shock Waves, Transition Points

Scientific paper

The paper examines a model of the transition region between the front of a detached shock wave and the magnetopause is examined which includes a magnetic barrier (a region of quasi-two-dimensional flow near the magnetopause) and the region in front of the barrier. Calculations are made of the plasma density and magnetic field strength near the magnetopause for different values of the Mach-Alfven number (4-50) in the solar wind and for different orientations of the interplanetary magnetic field.

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