Other
Scientific paper
Aug 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ge%26ae..23..619b&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 23, July-Aug. 1983, p. 619-623. In Russian.
Other
Geomagnetism, Magnetic Disturbances, Solar Terrestrial Interactions, Solar Wind, Periodic Variations, Solar Activity Effects, Solar Cycles
Scientific paper
It is shown that at all phases of the cycle of solar activity, high-velocity fluxes of solar wind flow around the earth most of the time. It is determined that the M-fluxes give rise not only to the well-known recurring disturbances of the geomagnetic field (primarily at the phase of low solar activity), but also to a large number of nonrecurring disturbances of the geomagnetic field at all other phases of the cycle. In addition, it is found that short-lived M-fluxes create less intensive disturbances than long-lived fluxes.
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