Model of particle fluxes and averaged energy spectra of solar cosmic rays.
Abstract
As a result of an analysis of acquired experimental data on solar cosmic ray fluences a classification of these events is suggested. It is shown that the averaged energy spectra of particle peak fluxes and fluences, characterizing solar cosmic ray events of various magnitude, with proton energies of over 30 MeV, are well described by power law functions of particle rigidity.
- Publication:
-
Kosmicheskie Issledovaniia
- Pub Date:
- January 1993
- Bibcode:
- 1993KosIs..31...51N
- Keywords:
-
- Solar Cosmic Rays;
- Energy Spectra;
- Solar Protons;
- Proton Flux Density;
- Proton Energy;
- Power Series;
- Solar Terrestrial Interactions;
- Solar Physics