Comparison of various methods of determining solar proton spectra

Details Comparison of various methods of determining solar proton spectra Comparison of various methods of determining solar proton spectra

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ge%26ae..16..976d&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 16, Nov.-Dec. 1976, p. 976-979. In Russian.

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Balloon-Borne Instruments, Satellite-Borne Instruments, Solar Activity, Solar Protons, Solar Spectra, Spectral Energy Distribution, Comparison, Cosmic Rays, Geomagnetism, Time Dependence

Scientific paper

Existing methods of solar cosmic ray spectra are compared by applying them to the proton event of January 24, 1971. It is shown that methods based on the geomagnetic (cutoff) effect yield largely exaggerated values of the characteristic rigidity of the exponential pulse spectrum as compared to other methods, particularly, if the vertical rigidity is taken as the cutoff rigidity.

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