Microwave and soft X-ray emission of solar flare events associated with coronal transients

Details Microwave and soft X-ray emission of solar flare events associated with coronal transients Microwave and soft X-ray emission of solar flare events associated with coronal transients

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992azh....69..593c&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 69, no. 3, May-June 1992, p. 593-603. In Russian.

Astronomy and Astrophysics

Astronomy

3

Microwave Emission, Solar Corona, Solar Flares, Solar Radio Bursts, Solar X-Rays, Magnetic Field Configurations, Magnetic Flux, Solar Magnetic Field

Scientific paper

The characteristics of microwave and soft X-ray bursts accompanying coronal transients (CTs) observed with the P78-1 satellite are examined. It is shwon that the distribution of the events on the burst intensity-duration plots makes it possible not only to distinguish flares with CTs from those without CTs, but also to determine the relationship between the burst characteristics and the main parameters of the CTs (angular size, velocity, mass, and shape). The relationship between CTs and flare energy release is considered.

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