Spectral correlations between solar flare radio bursts and associated proton fluxes, 2

Details Spectral correlations between solar flare radio bursts and associated proton fluxes, 2 Spectral correlations between solar flare radio bursts and associated proton fluxes, 2

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7627153b&link_type=abstract

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Physics

Solar Flares, Solar Radio Bursts, Solar Spectra, Spectral Correlation, Proton Flux Density, Solar Physics, Solar Protons

Scientific paper

An earlier study of the solar flare U-shaped radio burst spectra and associated proton flux data has been extended to include additional events. The slope of the proton peak-flux profile is correlated to the radio frequency ratio (omega3)/(omega sub 2) where (omega3) equals frequency of maximum radio peak flux of the upper branch of the U, and (omega2) equals cut-off frequency for the lower branch of the U. The use of the slope allows inclusion of the pre-Explorer (1966-67) events, recorded on various different proton-energy channels.

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