Plasma convection at high latitudes

Details Plasma convection at high latitudes Plasma convection at high latitudes

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..366r&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, Mar.-Apr. 1991, p. 366-368. In Russian.

Physics

Earth Magnetosphere, Plasma Turbulence, Polar Cusps, Polar Substorms, Convection Currents, Interplanetary Magnetic Fields, Magnetic Field Reconnection, Plasma-Electromagnetic Interaction, Solar Wind

Scientific paper

It is shown that, under the combined effect of D-type and E-H-type convection, there exists a critical value of the D potential under which a large quasi-stagnation region arises in the magnetospheric boundary layer. When the value of the D-type convection is less than the critical D potential, convection in this layer occurs in the antisolar direction; when it is greater than the critical value, the convection is directed toward the sun.

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