Energy spectra of solar cosmic rays according to balloon and neutron monitor data

Details Energy spectra of solar cosmic rays according to balloon and neutron monitor data Energy spectra of solar cosmic rays according to balloon and neutron monitor data

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....4..194b&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 4 (A85-2

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Energy Spectra, Neutron Counters, Solar Activity, Solar Cosmic Rays, Solar Protons, Stratosphere, Balloon Sounding, Integral Equations, U.S.S.R.

Scientific paper

The energy spectra of solar protons were obtained in the range from 100 MeV to several GeV on the basis of joint analysis of stratospheric and neutron-monitor measurements. The most powerful events of 1976-1982 were found occurring during the increasing and declining phases of the solar activity cycle. In the event of October 12, 1981, an additional source of fast particles seems to be available.

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