Solar modulation of galactic cosmic rays with the ARINA and PAMELA spectrometers

Solar modulation of the proton flux in Galactic space radiation during the period from the end of the 23rd to the beginning of 24th cycle of solar activity is investigated using data from the PAMELA magnetic spectrometer and ARINA scintillation spectrometer. The time dependence of proton intensity i...

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Bibliographic Details
Published in:Bulletin of the Russian Academy of Sciences. Physics 2013-05, Vol.77 (5), p.517-519
Main Authors: Bzheumikhova, M. A., Koldashov, S. V., Losev, D. S., Mayorov, A. G., Mikhailov, V. V., Sidorov, A. V., Ulitin, A. A.
Format: Article
Language:English
Subjects:
Cosmic rays
Extraterrestrial radiation
Flux
Galactic cosmic rays
Hadrons
Heavy Ions
Modulation
Nuclear Physics
Physics
Physics and Astronomy
Proceedings of the 32nd All-Russia Conference on Cosmic Rays
Scintillation
Solar activity
Spectrometers
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Summary:Solar modulation of the proton flux in Galactic space radiation during the period from the end of the 23rd to the beginning of 24th cycle of solar activity is investigated using data from the PAMELA magnetic spectrometer and ARINA scintillation spectrometer. The time dependence of proton intensity is plotted, and shows typical features in a form of rises and falls against a main trend. In order to explain these, the correlation between variations in the Galactic proton flux and solar/interplanetary parameters is investigated.
ISSN:1062-8738
1934-9432
DOI:10.3103/S1062873813050134