Quantitative characteristics of the relationship solar active processes and the transit velocity of interplanetary shock waves.

Details Quantitative characteristics of the relationship solar active processes and the transit velocity of interplanetary shock waves. Quantitative characteristics of the relationship solar active processes and the transit velocity of interplanetary shock waves.

Apr 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acaps..17..191e&link_type=abstract

Acta Astrophys. Sin., Vol. 17, No. 2, p. 191 - 194

Astronomy and Astrophysics

Astrophysics

Interplanetary Shock Waves: Solar Flares, Interplanetary Shock Waves: Solar Filaments, Shock Waves: Solar Activity

Scientific paper

By excluding events with a possible interaction of shock waves caused by nonisolated flare processes, it has been possible to specify the relationship between a characteristic of the X-ray (λ = 1 - 8 Å) flare emission, and the transit velocity VT of the relevant interplanetary shock wave, as first obtained by Eselevich. Also it has been possible to obtain relationships between the size of eruptive filaments outside active regions and the transit velocity of an associated shock wave.

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