Solar Radio Continua and the X-Ray Emission during Flares

Details Solar Radio Continua and the X-Ray Emission during Flares Solar Radio Continua and the X-Ray Emission during Flares

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987baicz..38...36f&link_type=abstract

Bulletin of the Astronomical Institute of Czechoslovakia, vol. 38, p.36

Astronomy and Astrophysics

Astronomy

Scientific paper

Radio continua measured by the Ondřejov solar radio spectrograph in the frequency band of 100 - 1000 MHz are compared with the X-ray flux in the 2 - 320 keV region, measured by the Czechoslovak photometer aboard the Prognoz 8 satellite. The authors have chosen 20 flare-associated events, recorded by both instruments from March to August 1981, and, using the Solar Geophysical Data, they have determined source flares and their optical characteristics.

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