Computer Science
Scientific paper
Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..889m&link_type=abstract
Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Nov.-Dec. 1989, p. 889-895. In Russian.
Computer Science
Current Sheets, Heliosphere, Solar Flares, Solar Terrestrial Interactions, Electron Avalanche, Shock Wave Propagation, Solar Activity Effects, Temporal Distribution
Scientific paper
The properties of the heliospheric current sheet (HCS) near the earth under quiet conditions and after intense isolated flares are compared. It is shown that shock waves are observed in front of the HCS and the frequency of occurrence of high-amplitude streamer oscillations associated with the HCS rises sharply only after the occurrence of flares. It is suggested that sometimes shock waves appear in the forbidden zone in front of the HCS because of a nonlinear steepening of the front of a quasi-steady stream accelerated by the flare, while oscillations of the HCS arise during its interaction with a coronal flare transient near the sun and propagate along the streamer to earth orbit.
Ivanov K. G.
Mikerina N. V.
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