Physics
Scientific paper
Oct 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974dossr.218.1056k&link_type=abstract
Akademiia Nauk SSSR, Doklady, vol. 218, Oct. 11, 1974, p. 1056-1059. In Russian.
Physics
Electromagnetic Interactions, Ionospheric Currents, Magnetospheric Instability, Plasma Conductivity, Solar Wind, Auroral Electrojets, Electron Trajectories, Equatorial Electrojet, Iterative Solution, Magnetoionics, Maxwell Equation
Scientific paper
Expressions are found describing the perturbed field and the current resulting against the background of a steady strong magnetic field which, together with a given undisturbed-plasma distribution, produces the conduction tensor for a perturbation current. The analysis is applied to the earth's magnetosphere. Boundary equations are considered for the two unconnected portions of the magnetosphere boundary: the nonconducting atmosphere and the external transition layer toward the solar wind. Three mechanisms for generating electric and current fields are indicated: ionospheric winds, fast-particle currents, and the applied current from the transition region. The equations derived can be used in future studies of the equatorial jet stream and the polar electron stream.
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