2014/11/27 by М. Б. Крайнев, M. B. Krainev, G. A. Bazilevskaya +9
Physics and Astronomy · #FOS: Physical sciences #Ionosphere and magnetosphere dynamics #Solar and Space Plasma Dynamics #Solar and Stellar Astrophysics (astro-ph.SR) #Space Physics (physics.space-ph) #Stellar, planetary, and galactic studies #astro-ph.SR #physics.space-ph
paper · pdf · doi:10.48550/arxiv.1411.7526
4 pages, 3 figures, paper icrc2013-0305 reported at 33-rd International Cosmic Ray Conference, Rio-de-Janeiro, Brasil, 2013
arxiv created 2014/11/27 · openalex publication_date 2014/11/27 · arxiv updated 2014/12/01 · openalex created_date 2021/04/13 · openalex updated_date 2026/07/28
Using the simple model for the description of the GCR modulation in the heliosphere and the sets of parameters discussed in the accompanying paper we model some features of the time and energy behavior of the GCR intensity near the Earth observed during periods of low solar activity around three last solar minima. In order to understand the mechanisms underlying these features in the GCR behavior, we use the suggested earlier decomposition of the calculated intensity into the partial intensities corresponding to the main processes (diffusion, adiabatic losses, convection and drifts).