Some peculiarities of statistical distributions of solar radio bursts

Details Some peculiarities of statistical distributions of solar radio bursts Some peculiarities of statistical distributions of solar radio bursts

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982azh....59..376p&link_type=abstract

(Astronomicheskii Zhurnal, vol. 59, Mar.-Apr. 1982, p. 376-379.) Soviet Astronomy, vol. 26, Mar.-Apr. 1982, p. 226-229. Transla

Astronomy and Astrophysics

Astronomy

1

Solar Radio Bursts, Statistical Distributions, Electron Energy, Microwaves, Solar Flares

Scientific paper

An empirical-statistical method is proposed for estimating the optical depth of a source of radio emission. Through an analysis of statistical distributions of the parameters of the corpuscular and electromagnetic radiation of solar flares it is shown that microwave radio bursts on the sun are generated by electrons which reach the earth's orbit with an energy of more than 40 keV. The results of a number of earlier reports on this subject are brought into agreement.

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