Latitude Effect of Muons in the Earth’s Atmosphere during Solar Activity Minimum

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dc.contributor.author V. S. Makhmutov
dc.contributor.author G. A. Bazilevskaya
dc.contributor.author Yu. I. Stozhkov
dc.contributor.author N. S. Svirzhevskya
dc.contributor.author A. K. Morzabayev
dc.date.accessioned 2013-04-22T05:35:17Z
dc.date.available 2013-04-22T05:35:17Z
dc.date.issued 2013-04-22
dc.identifier.uri http://repository.enu.kz/handle/123456789/7117
dc.description http://www.enu.kz ru_RU
dc.description.abstract The results of muon flux measurements (E ≥ 70 MeV) in the atmosphere during solar activity min-imum are reported. The measurements were performed during Antarctic sea expedition in 1975–1976 at several geomagnetic locations (from 1 to 14 GV). The experimental data obtained made it possible to determine the latitude effect of muons in the distribution at different levels in the atmosphere. The Geant4 program was used to simulate the galactic cosmic ray transport in the Earth’s atmosphere and evaluate the angular and spectral distributions (p, e–/e+, photons, muons) at different atmospheric levels. The experimental and simulated results are in satisfactory agreement. ru_RU
dc.language.iso en ru_RU
dc.subject measurements ru_RU
dc.subject The GCR proton transport ru_RU
dc.subject PLANETOCOSMICS ru_RU
dc.title Latitude Effect of Muons in the Earth’s Atmosphere during Solar Activity Minimum ru_RU
dc.type Article ru_RU


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