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Solar-cycle Variations of South Atlantic Anomaly Proton Intensities Measured with the PAMELA Mission

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dc.contributor.authorBruno, A.
dc.contributor.authorMartucci, M.
dc.contributor.authorCafagna, F. S.
dc.contributor.authorSparvoli, R.
dc.contributor.authorGalper, A. M.
dc.contributor.authorKoldashov, S. V.
dc.contributor.authorKoldobskiy, S.
dc.contributor.authorLeonov, A. A.
dc.contributor.authorMalakhov, V. V.
dc.contributor.authorMayorov, A. G.
dc.contributor.authorMikhailov, V. V.
dc.contributor.authorSpillantini, P.
dc.contributor.authorVoronov, S. A.
dc.contributor.authorYurkin, Y. T.
dc.contributor.authorZharaspayev, T. R.
dc.contributor.authorКолдобский, Сергей Александрович
dc.contributor.authorЛеонов, Алексей Анатольевич
dc.contributor.authorМалахов, Виталий Валерьевич
dc.contributor.authorМайоров, Андрей Георгиевич
dc.contributor.authorМихайлов, Владимир Владимирович
dc.contributor.authorВоронов, Сергей Александрович
dc.contributor.authorЮркин, Юрий Тихонович
dc.date.accessioned2024-11-29T19:44:58Z
dc.date.available2024-11-29T19:44:58Z
dc.date.issued2021
dc.description.abstract© 2021. The American Astronomical Society. All rights reserved..We present a study of the solar-cycle variations of >80 MeV proton flux intensities in the lower edge of the inner radiation belt, based on the measurements of the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) mission. The analyzed data sample covers an ∼8 yr interval from 2006 July to 2014 September, thus spanning from the decaying phase of the 23rd solar cycle to the maximum of the 24th cycle. We explored the intensity temporal variations as a function of drift shell and proton energy, also providing an explicit investigation of the solar modulation effects at different equatorial pitch angles. PAMELA observations offer new important constraints for the modeling of low-altitude particle radiation environment at the highest trapping energies.
dc.identifier.citationSolar-cycle Variations of South Atlantic Anomaly Proton Intensities Measured with the PAMELA Mission / Bruno, A. [et al.] // Astrophysical Journal Letters. - 2021. - 917. - № 2. - 10.3847/2041-8213/ac1a74
dc.identifier.doi10.3847/2041-8213/ac1a74
dc.identifier.urihttps://www.doi.org/10.3847/2041-8213/ac1a74
dc.identifier.urihttps://www.scopus.com/record/display.uri?eid=2-s2.0-85113386762&origin=resultslist
dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000685899400001
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/24624
dc.relation.ispartofAstrophysical Journal Letters
dc.titleSolar-cycle Variations of South Atlantic Anomaly Proton Intensities Measured with the PAMELA Mission
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue2
oaire.citation.volume917
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