Time Variations of Proton Flux in Earth Inner Radiation Belt for 2006-2015 Years based on the PAMELA and the ARINA Data

• Published in: Physics procedia 2015, Vol.74, p.377-381
• Main Authors: Malakhov, V.V., Koldashov, S.V., Mayorov, A.G., Mayorova, M.A., Mikhailov, V.V., Aleksandrin, S.Yu
• Format: Article
• Language: English
• Subjects: radiation belt; solar cycle; space environment
• ISSN: 1875-3892; 1875-3892
• DOI: 10.1016/j.phpro.2015.09.200

The PAMELA and the ARINA experiments are carried out aboard satellite RESURS-DK1 since 2006 up to now. Both these instruments have possibility to measure charged particles in the inner radiation belt. Combination of these two devices covers proton energy range from 30 MeV up to trapping limit (E ∽2GeV). Continuous measurements with PAMELA and ARINA include minimum between 23rd and 24th solar cycles falling and rising phases of 23/24 solar cycles and maximum of 24th one. It is important because existing empirical radiation belt models does not intend to calculate fluxes taking into account solar activity varying, e.g. widely used AP-8 model allows to evaluate proton fluxes just in two cases: for minimum or maximum of a solar activity. In this report we present temporal profiles of proton flux in the lower edge of the inner proton radiation belt (1.12 < L < 1.20, 0.18 < B < 0.22 G) and ratio between solar minimum and maximum fluxes. Dependence of proton fluxes on degree of solar activity were studied for various phases of 23/24 solar cycle. At that it was shown that proton fluxes of energy >80MeV at the solar minimum several times greater than at the solar maximum. Maximum difference is seen on the L-shell 1.15.