Publication:
Amplitude and Temporal Characteristics of 27-Day Variations in the Galactic Cosmic Ray Flux, Measured during the PAMELA Experiment between 2006 and 2016

dc.contributor.authorYulbarisov, R. F.
dc.contributor.authorGalikyan, N. G.
dc.contributor.authorMayorov, A. G.
dc.contributor.authorGolub, O. A.
dc.contributor.authorMalakhov, V. V.
dc.contributor.authorRodenko, S. A.
dc.contributor.authorЮлбарисов, Рустам Фаритович
dc.contributor.authorГаликян, Норайр Грачьяевич
dc.contributor.authorМайоров, Андрей Георгиевич
dc.contributor.authorГолуб, Ольга Александровна
dc.contributor.authorМалахов, Виталий Валерьевич
dc.contributor.authorРоденко, Светлана Александровна
dc.date.accessioned2024-11-30T00:28:17Z
dc.date.available2024-11-30T00:28:17Z
dc.date.issued2021
dc.description.abstract© 2021, Allerton Press, Inc.Abstract: Several cases of 27-day variations in the flux of galactic cosmic rays (GCRs) are detected by the PAMELA and ARINA spectrometers from June 2006 to January 2016. GCR characteristics are reconstructed, the temporal behavior of the amplitude of variations is described for different energies, and amplitude–energy dependences are obtained for several episodes of variations arising.
dc.format.extentС. 1272-1275
dc.identifier.citationAmplitude and Temporal Characteristics of 27-Day Variations in the Galactic Cosmic Ray Flux, Measured during the PAMELA Experiment between 2006 and 2016 / Yulbarisov, R.F. [et al.] // Bulletin of the Russian Academy of Sciences: Physics. - 2021. - 85. - № 11. - P. 1272-1275. - 10.3103/S1062873821110381
dc.identifier.doi10.3103/S1062873821110381
dc.identifier.urihttps://www.doi.org/10.3103/S1062873821110381
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85120957284&origin=resultslist
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/25092
dc.relation.ispartofBulletin of the Russian Academy of Sciences: Physics
dc.titleAmplitude and Temporal Characteristics of 27-Day Variations in the Galactic Cosmic Ray Flux, Measured during the PAMELA Experiment between 2006 and 2016
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue11
oaire.citation.volume85
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