Physics
Scientific paper
Jun 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..390i&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, May-June 1983, p. 390-396. In Russian.
Physics
5
Geomagnetism, Interplanetary Magnetic Fields, Magnetic Disturbances, Magnetohydrodynamic Turbulence, Solar Flares, Solar Terrestrial Interactions, Magnetic Poles, Shock Wave Propagation, Solar Corpuscular Radiation, Solar Magnetic Field
Scientific paper
It is shown that the cross-section configurations of MHD flare disturbances can be constructed on a sphere with a radius of 1 AU using data on the coordinates of intense solar flares and on the magnetic poles of bipolar groups. The empirical and formal foundations of this approach are developed, and the method is demonstrated for a number of isolated flares and flare series. The effect of the earth's position with respect to the cross sections on the geomagnetic disturbances is examined.
Ivanov K. G.
Kharshiladze A. F.
Mikerina N. V.
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