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Variation of Cosmic Ray Muons in 2007–2019

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dc.contributor.authorShutenko, V. V.
dc.contributor.authorBarbashina, N. S.
dc.contributor.authorDmitrieva, A. N.
dc.contributor.authorYakovleva, E. I.
dc.contributor.authorШутенко, Виктор Викторович
dc.contributor.authorБарбашина, Наталья Сергеевна
dc.contributor.authorДмитриева, Анна Николаевна
dc.date.accessioned2024-11-29T21:20:49Z
dc.date.available2024-11-29T21:20:49Z
dc.date.issued2021
dc.description.abstract© 2021, Allerton Press, Inc.Abstract: An analysis is performed of the diurnal variation in cosmic-ray muons measured with the URAGAN muon hodoscope from 2007 to 2019. Characteristics are given of the yearly average diurnal variation in the count rate in several zenith-angle intervals. The results are compared to the diurnal variations in the count rate of neutrons from ten neutron monitors.
dc.format.extentС. 1055-1057
dc.identifier.citationVariation of Cosmic Ray Muons in 2007–2019 / Shutenko, V.V. [et al.] // Bulletin of the Russian Academy of Sciences: Physics. - 2021. - 85. - № 9. - P. 1055-1057. - 10.3103/S1062873821090288
dc.identifier.doi10.3103/S1062873821090288
dc.identifier.urihttps://www.doi.org/10.3103/S1062873821090288
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85116789972&origin=resultslist
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/24792
dc.relation.ispartofBulletin of the Russian Academy of Sciences: Physics
dc.titleVariation of Cosmic Ray Muons in 2007–2019
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue9
oaire.citation.volume85
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