Formulation of the problem of the evolution of the auroral bulge

Details Formulation of the problem of the evolution of the auroral bulge Formulation of the problem of the evolution of the auroral bulge

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..933m&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, Nov.-Dec. 1990, p. 933-938. In Russian.

Physics

Auroral Arcs, Field Aligned Currents, Magnetosphere-Ionosphere Coupling, Mathematical Models, Geomagnetism, Plasma Dynamics, Solitary Waves, Time Dependence

Scientific paper

A physical-mathematical model of the auroral-bulge evolution is developed. This model is based on a closed system of equations describing the motion of a plasma tube and the electric-field distribution, with self-consistent allowance for the effects of ionospheric-magnetospheric interaction through field-aligned currents. The magnetospheric plasma is described by the CGL approximation, while the ionospheric plasma is described by the height-integral conductivity tensor.

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