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Pis'ma v Zhurnal Èksperimental'noi i Teoreticheskoi Fiziki, 2013, Volume 98, Issue 12, Pages 867–870
DOI: https://doi.org/10.7868/S0370274X13240016 (Mi jetpl3604) 		 
This article is cited in 5 scientific papers (total in 5 papers)

ASTROPHYSICS AND COSMOLOGY

Variation of the cosmic ray intensity in an 11-yr solar activity cycle: Experiment and theory

G. F. Krymsky, P. Yu. Gololobov, P. A. Krivoshapkin, S. K. Gerasimova, V. G. Grigor'ev, S. A. Starodubtsev

Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences
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DOI: https://doi.org/10.7868/S0370274X13240016
Abstract: To study long-term variations of the cosmic ray intensity in a wide energy range, a basic model of the modulation of cosmic rays in the heliosphere has been developed at the Institute of Cosmophysical Research and Aeronomy, Siberian Branch, Russian Academy of Sciences. The model involves only one free modulation parameter, the ratio of the regular magnetic field to the turbulent field. It can be used to describe variations of the cosmic ray intensity in a wide energy range of $0.1$ to $100$ GeV. Attempts have been made to most correctly describe the features of the behavior of the cosmic ray intensity in several solar activity cycles.
Received: 29.10.2013
Revised: 25.11.2013
English version:
Journal of Experimental and Theoretical Physics Letters, 2013, Volume 98, Issue 12, Pages 769–772
DOI: https://doi.org/10.1134/S0021364013250139
Bibliographic databases:
Document Type: Article
Language: Russian
Citation: G. F. Krymsky, P. Yu. Gololobov, P. A. Krivoshapkin, S. K. Gerasimova, V. G. Grigor'ev, S. A. Starodubtsev, “Variation of the cosmic ray intensity in an 11-yr solar activity cycle: Experiment and theory”, Pis'ma v Zh. Èksper. Teoret. Fiz., 98:12 (2013), 867–870; JETP Letters, 98:12 (2013), 769–772
Citation in format AMSBIB
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    • This publication is cited in the following 5 articles:
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