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Characteristics of Forbush Decreases Measured by the PAMELA Instrument During 2006–2014

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dc.contributor.authorLagoida, I.
dc.contributor.authorVoronov, S.
dc.contributor.authorMikhailov, V.
dc.contributor.authorЛагойда, Илья Алексеевич
dc.contributor.authorВоронов, Сергей Александрович
dc.contributor.authorМихайлов, Владимир Владимирович
dc.date.accessioned2024-11-21T17:58:38Z
dc.date.available2024-11-21T17:58:38Z
dc.date.issued2019
dc.description.abstract© 2019, Pleiades Publishing, Ltd.During the several decades of Forbush decrease (FD) studies the main properties of this phenomenon were established. Today is clear that Forbush decreases originate as the responses of cosmic ray particle fluxes to solar-induced processes inside interplanetary space. Moreover the profiles of FD’s are the manifestation of the complex structure of coronal mass ejections (CMEs) which are driving from the Sun and often accompanied by flares. So the investigation of FD’s is a useful tool for understanding the dynamics of CME processes and the effects they have on in the interplanetary space. Classification and theoretical interpretation of different FD’s are important for understanding the complex effect of CME’s as well as the search for new features of their behavior. Spectra of cosmic ray protons and helium nuclei obtained by the PAMELA experiment in the rigidity range between 1–15 GV were used to investigate the characteristics of Forbush decreases. Additional data on the interplanetary magnetic field and solar wind speed were taken from the ACE data center for correlation analysis. Rigidity dependences for selected Forbush decreases are also presented.
dc.format.extentС. 750-753
dc.identifier.citationLagoida, I. Characteristics of Forbush Decreases Measured by the PAMELA Instrument During 2006–2014 / Lagoida, I., Voronov, S., Mikhailov, V. // Physics of Atomic Nuclei. - 2019. - 82. - № 6. - P. 750-753. - 10.1134/S1063778819660347
dc.identifier.doi10.1134/S1063778819660347
dc.identifier.urihttps://www.doi.org/10.1134/S1063778819660347
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85079454745&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000517845500029
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/19429
dc.relation.ispartofPhysics of Atomic Nuclei
dc.titleCharacteristics of Forbush Decreases Measured by the PAMELA Instrument During 2006–2014
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue6
oaire.citation.volume82
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