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Origin of the Short-Term Variations of the Cosmic Ray Flux

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dc.contributor.authorLagoida, I. A.
dc.contributor.authorVoronov, S. A.
dc.contributor.authorMikhailov, V. V.
dc.contributor.authorЛагойда, Илья Алексеевич
dc.contributor.authorВоронов, Сергей Александрович
dc.contributor.authorМихайлов, Владимир Владимирович
dc.date.accessioned2024-11-21T15:40:33Z
dc.date.available2024-11-21T15:40:33Z
dc.date.issued2019
dc.description.abstract© 2019, Pleiades Publishing, Ltd.Abstract: Detection of cosmic ray fluxes makes it possible to study dynamics of the interplanetary magnetic field and gain information about processes that occur both on the solar surface and in the entire Solar system. The main variations in the cosmic ray intensity are 27-day variations and Forbush effects. These variations are caused by complex spatial solar-plasma formations resulting from various processes on the solar surface and propagating in space with widely varying velocities. The data recorded by the PAMELA magnetic spectrometer on board the Resurs-DK1 satellite in 2006–2016 are used.
dc.format.extentС. 826-835
dc.identifier.citationLagoida, I. A. Origin of the Short-Term Variations of the Cosmic Ray Flux / Lagoida, I.A., Voronov, S.A., Mikhailov, V.V. // Physics of Particles and Nuclei. - 2019. - 50. - № 6. - P. 826-835. - 10.1134/S1063779619060054
dc.identifier.doi10.1134/S1063779619060054
dc.identifier.urihttps://www.doi.org/10.1134/S1063779619060054
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85077050306&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000510709300005
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/19071
dc.relation.ispartofPhysics of Particles and Nuclei
dc.titleOrigin of the Short-Term Variations of the Cosmic Ray Flux
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue6
oaire.citation.volume50
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