Distribution law of integrated intensity of solar optical flares

Details Distribution law of integrated intensity of solar optical flares Distribution law of integrated intensity of solar optical flares

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984baicz..35..241d&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 35, Aug. 1984, p. 241-243.

Astronomy and Astrophysics

Astronomy

2

Solar Flares, Statistical Distributions, Visible Spectrum, Frequency Distribution, H Alpha Line

Scientific paper

A distribution law is proposed which connects the occurrence frequency distribution of solar optical flares with their integrated intensity values. A total of 1438 observations of solar optical flares were taken from NOAA Solar Geophysical Daily bulletins for the period from 1970 to 1977. The integrated intensities of the flares are calculated by means of Sawyer's (1967) expression for the measured area of a solar flare in square degrees. The calculations show that the number of flares diminishes when the integrated intensities are less than 2 sq degrees.

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