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Forbush Decreases During 2007–2018 According to the Muon Hodoscope URAGAN Data

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dc.contributor.authorKovylyaeva, A. A.
dc.contributor.authorAstapov, I. I.
dc.contributor.authorBarbashina, N. S.
dc.contributor.authorBorog, V. V.
dc.contributor.authorDmitrieva, A. N.
dc.contributor.authorKompaniets, K. G.
dc.contributor.authorMishutina, Y. N.
dc.contributor.authorPetrukhin, A. A.
dc.contributor.authorShutenko, V. V.
dc.contributor.authorYakovleva, E. I.
dc.contributor.authorYashin, I. I.
dc.contributor.authorАстапов, Иван Иванович
dc.contributor.authorБарбашина, Наталья Сергеевна
dc.contributor.authorБорог, Владимир Викторович
dc.contributor.authorДмитриева, Анна Николаевна
dc.contributor.authorКомпаниец, Константин Георгиевич
dc.contributor.authorМишутина, Юлия Николаевна
dc.contributor.authorПетрухин, Анатолий Афанасьевич
dc.contributor.authorШутенко, Виктор Викторович
dc.contributor.authorЯшин, Игорь Иванович
dc.date.accessioned2024-11-21T17:50:38Z
dc.date.available2024-11-21T17:50:38Z
dc.date.issued2019
dc.description.abstract© 2019, Pleiades Publishing, Ltd.Results of the study of variations of cosmic ray muon flux at the Earth surface during Forbush decreases registered in 2007–2018 by means of the muon hodoscope URAGAN are presented. The dynamics of the amplitude spectral index at different stages (the decrease, the minimum, and the recovery), which correspond to different phases of the influence of heliospheric disturbances on the flux of cosmic rays for the period 2012 to 2018, is considered. To investigate possible regularities in the behavior of the projection of the relative local anisotropy vector of the muon flux to the South and to the East (rS and rE) during 2007–2018, the distributions of these parameters for four phases (immediately before FD, decrease phase, minimum phase, recovery phase) were calculated.
dc.format.extentС. 892-896
dc.identifier.citationForbush Decreases During 2007–2018 According to the Muon Hodoscope URAGAN Data / Kovylyaeva, A.A. [et al.] // Physics of Atomic Nuclei. - 2019. - 82. - № 6. - P. 892-896. - 10.1134/S1063778819660323
dc.identifier.doi10.1134/S1063778819660323
dc.identifier.urihttps://www.doi.org/10.1134/S1063778819660323
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85079032365&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000517845500054
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/19411
dc.relation.ispartofPhysics of Atomic Nuclei
dc.titleForbush Decreases During 2007–2018 According to the Muon Hodoscope URAGAN Data
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue6
oaire.citation.volume82
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