Empirical model of long‐time variations of galactic cosmic ray particle fluxes
Authors:
- 7 February 2017
- journal article
- research article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Space Physics
- Vol. 122 (2) , 1463-1472
Abstract
The galactic cosmic ray (GCR) particle flux model has been developed by using the experimental data obtained during the solar cycles 21–24. The model calculates fluxes of GCR particles (with charge z from 1 to 28 and energy E from 80 up to 105 MeV/nucleon) in the interplanetary space (ecliptic plane) as a function of solar activity (sunspot number) and the heliocentric distance. GCR proton fluxes computed by the model for the case of a possible decrease in solar activity during solar cycles 25 and 26 are discussed.Keywords
Funding Information
- Russian Science Foundation (16‐17‐00098, 16‐17‐10097)
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