Estimates of the proton energy spectrum exponent on the basis of solar microwave radio-burst data

Details Estimates of the proton energy spectrum exponent on the basis of solar microwave radio-burst data Estimates of the proton energy spectrum exponent on the basis of solar microwave radio-burst data

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ge%26ae..22..182c&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 22, Mar.-Apr. 1982, p. 182-186. In Russian.

Physics

8

Energy Spectra, Proton Energy, Solar Flares, Solar Protons, Solar Radio Bursts, Solar Terrestrial Interactions, Gamma Ray Spectra, Microwave Emission

Scientific paper

A method is developed for the short-term prediction of the energy spectrum exponent (gamma) of protons near the earth with energies of the order of tens of MeV; gamma is determined on the basis of the ratio of maximum intensities of solar radio bursts at frequencies of 9 and 15.4 GHz (S9/S15). Data on 35 proton events are used to determine the relationship between S9/S15 and gamma for flares on the western half of the disk, as well as the heliolongitudinal correction for protons arriving at the earth from eastern flares.

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