Publication:
Analysis of Variations of the Muon and Hadron Components of Cosmic Rays at Different Phases of the Solar Activity During the 11-Year Solar Cycle

Простая страница элемента
dc.contributor.authorMelnikova, I. A.
dc.contributor.authorKovylyaeva, A. A.
dc.contributor.authorMishutina, Y. N.
dc.contributor.authorShutenko, V. V.
dc.contributor.authorМишутина, Юлия Николаевна
dc.contributor.authorШутенко, Виктор Викторович
dc.date.accessioned2024-11-27T07:03:09Z
dc.date.available2024-11-27T07:03:09Z
dc.date.issued2020
dc.description.abstract© 2020, Pleiades Publishing, Ltd.Abstract: Variations of secondary cosmic rays on the Earth’s surface depend on the solar activity. To study these variations, neutron monitors and muon detectors are used. Observations of muons and hadrons complement each other in terms of the energies of the primary cosmic rays and their angular distribution. Muons save the direction of the motion of primary particles and make it possible to obtain the angular distribution of cosmic ray modulations using a single setup—as a muon hodoscope. This paper presents a comparison of variations of muon and neutron components of cosmic rays at the Earth surface at different phases of the solar activity in the period from 2008 to 2018. For the comparison, data of two neutron monitors (Moscow and Apatity stations) and the muon hodoscope URAGAN were used.
dc.format.extentС. 294-299
dc.identifier.citationAnalysis of Variations of the Muon and Hadron Components of Cosmic Rays at Different Phases of the Solar Activity During the 11-Year Solar Cycle / Melnikova, I.A. [et al.] // Physics of Atomic Nuclei. - 2020. - 83. - № 2. - P. 294-299. - 10.1134/S1063778820020209
dc.identifier.doi10.1134/S1063778820020209
dc.identifier.urihttps://www.doi.org/10.1134/S1063778820020209
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85089228086&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000557030700025
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/22168
dc.relation.ispartofPhysics of Atomic Nuclei
dc.titleAnalysis of Variations of the Muon and Hadron Components of Cosmic Rays at Different Phases of the Solar Activity During the 11-Year Solar Cycle
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue2
oaire.citation.volume83
relation.isAuthorOfPublication8d86d984-d1f7-4383-95a4-5520fa329976
relation.isAuthorOfPublicationd0ef710a-cff6-4aa6-9c43-dfa6b57e4c80
relation.isAuthorOfPublication.latestForDiscovery8d86d984-d1f7-4383-95a4-5520fa329976
relation.isOrgUnitOfPublicationba0b4738-e6bd-4285-bda5-16ab2240dbd1
relation.isOrgUnitOfPublication.latestForDiscoveryba0b4738-e6bd-4285-bda5-16ab2240dbd1
Файлы
Коллекции
Публикации