Physics
Scientific paper
Jun 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ge%26ae..24..517b&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 24, May-June 1984, p. 517-520. In Russian.
Physics
Geomagnetic Pulsations, Magnetic Disturbances, Magnetospheric Instability, Ring Currents, Solar Terrestrial Interactions, Magnetic Variations, Solar Flares, Solar Wind, Space Plasmas
Scientific paper
A theoretical analysis of the replenishment phenomenon for M-type geomagnetic disturbances and flare-related disturbances is presented. It is shown that the replenishment of the ring current in the recovery phase has a significant effect on the course of the disturbance. This phenomenon gives to Dst variations an irregular (often wavy) shape. As for flare-related disturbances, the replenishment has a more modest (though still appreciable) effect, usually leaving the Dst variation curve unchanged.
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