The localization of flares in the sun's atmosphere from radio observations

Details The localization of flares in the sun's atmosphere from radio observations The localization of flares in the sun's atmosphere from radio observations

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978dossr.243..596p&link_type=abstract

(Akademiia Nauk SSSR, Doklady, vol. 243, Nov. 21, 1978, p. 596-599.) Soviet Physics - Doklady, vol. 23, Nov. 1978, p. 779-781. T

Astronomy and Astrophysics

Astronomy

Microwave Spectra, Solar Atmosphere, Solar Flares, Solar Protons, Solar Radio Bursts, Correlation Coefficients, Particle Acceleration, Radio Astronomy, Solar Flux, Solar Spectra, Solar Wind, Stellar Magnitude

Scientific paper

In the present paper, the existence of a correlation between the intensity of flare-accelerated proton fluxes with energies above 10 MeV at the earth's orbit and the characteristics of the corresponding radio burst at frequencies of 200, 650, 1400, 3000, 5000, 8500, and 15,000 MHz was investigated. The degree of correlation between the proton flux intensities and nine radio-burst parameters is determined for approximately 100 events in the period between 1964 and 1969. The optimal correlation coefficients are plotted against the frequency for each of the nine radio-burst parameters.

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