Evaluation of SCR-source spectra for a number of flares in the 19th and 20th solar cycles

Details Evaluation of SCR-source spectra for a number of flares in the 19th and 20th solar cycles Evaluation of SCR-source spectra for a number of flares in the 19th and 20th solar cycles

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ge%26ae..26..490b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 26, May-June 1986, p. 490-493. In Russian.

Physics

Radiation Sources, Solar Cosmic Rays, Solar Cycles, Solar Flares, Solar Protons, Solar Spectra, Diffusion Coefficient, Error Analysis, Particle Acceleration, Proton Energy

Scientific paper

Possible errors in the determination of the spectrum of a solar-cosmic-ray source were investigated for a number of proton flares in the 19th and 20th cycles on the basis of various model descriptions of the propagation process and uniform SCR data for proton energies from 10 to more than 60 MeV. Estimates of the number of accelerated particles (N0) and the diffusion coefficients in the IMF were made for the two cycles, and errors in the determination of absolute values of N0 were examined.

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