An evaluation of the application of modeling for the prediction of solar cosmic spectra

Details An evaluation of the application of modeling for the prediction of solar cosmic spectra An evaluation of the application of modeling for the prediction of solar cosmic spectra

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ge%26ae..20..197b&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 20, Mar.-Apr. 1980, p. 197-202. In Russian.

Mathematics

Energy Spectra, Prediction Analysis Techniques, Proton Flux Density, Solar Cosmic Rays, Solar Protons, Approximation, Isotropy, Mathematical Models, Particle Diffusion, Radiation Protection

Scientific paper

The paper presents evaluations of a model of isotropic diffusion for the description of temporal behavior of proton flux density in the 10-90 MeV range. The correctness of approximation of the solar proton energy spectrum is investigated using the exponential rigidity and power energy functions. Evaluations are made of application of a model of isotropic diffusion for the prediction of the energy spectra of solar cosmic rays.

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