Investigation of solar flares in the X-ray and optical ranges

Details Investigation of solar flares in the X-ray and optical ranges Investigation of solar flares in the X-ray and optical ranges

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989kosis..27..425k&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 27, May-June 1989, p. 425-432. In Russian.

Astronomy and Astrophysics

Astronomy

1

Solar Flares, Solar X-Rays, Visible Spectrum, X Ray Astronomy, Electron Energy, Energy Dissipation, H Alpha Line, Thermal Radiation, Venera Satellites

Scientific paper

Measurements of hard X-ray emission from 180 solar flares, as obtained on the Venera 13 and 14 probes, are compared with measurements of optical and thermal X-ray emissions. Values of the total energy release during a flare are calculated in these ranges, and a correlation analysis is carried out. The correlations found indicate that the total energy of fast electrons causing hard X-ray bursts in the impulsive flare phase and the thermal energy at the end of the impulsive phase have practically a functional relationship.

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