Flare-associated variations in the spectral slope of radio emission /lambda approximately 3 cm/ from solar active regions

Details Flare-associated variations in the spectral slope of radio emission /lambda approximately 3 cm/ from solar active regions Flare-associated variations in the spectral slope of radio emission /lambda approximately 3 cm/ from solar active regions

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980raf....22.1165a&link_type=abstract

(Radiofizika, vol. 22, no. 10, 1979, p. 1165-1176.) Radiophysics and Quantum Electronics, vol. 22, no. 10, Apr. 1980, p. 803-811

Physics

Centimeter Waves, Solar Activity Effects, Solar Flares, Solar Radio Emission, Solar Spectra, Spectrum Analysis, Radio Telescopes, Slopes, Solar Physics

Scientific paper

The paper examines data on the spectrum slope variations of emission at a wavelength of 3 cm from McMath 13786 and 13790 regions obtained for August 1975 using the Crimean Astrophysical Observatory radio telescope and observations of the World Radio and Optical Sun Service. These data are used to correlate spectrum slope variations with solar flare activity.

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