Physics
Scientific paper
Feb 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..100v&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Jan.-Feb. 1987, p. 100-103. In Russian.
Physics
Convection, Electric Field Strength, Ionospheric Currents, Magnetic Storms, Plasma-Electromagnetic Interaction, Polar Substorms, Geomagnetic Tail, Plasma Density, Plasma Layers, Plasma Pressure, Proton Energy, Time Dependence
Scientific paper
Calculations demonstrate that the natural response of particles escaping from the polar ionosphere and moving in the magnetospheric tail to the intensification of the convection electric field leads to the formation of a magnetospheric substorm. A region of elevated plasma pressure which travels toward the earth is formed in the tail; and three stages are clearly delineated in the behavior of the proton energy spectrum, which can be identified with the preliminary, explosive, and recovery phases of a substorm.
Krinberg I. A.
Voronov Evgenii V.
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