Solar Modulation of Cosmic Nuclei over a Solar Cycle: Results from the Alpha Magnetic Spectrometer

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dc.contributor.authorAguilar, M.
dc.contributor.authorAlpat, B.
dc.contributor.authorAmbrosi, G.
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dc.contributor.authorGrandi, D.
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dc.contributor.authorHaino, S.
dc.contributor.authorHan, K. C.
dc.contributor.authorHashmani, R. K.
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dc.contributor.authorHernández-Nicolás, F.
dc.contributor.authorHsieh, T. H.
dc.contributor.authorHu, J. Y.
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dc.contributor.authorLee, H. T.
dc.contributor.authorLee, S. C.
dc.contributor.authorLi, H. L.
dc.contributor.authorLi, J. H.
dc.contributor.authorLi, J. Q.
dc.contributor.authorLi, M.
dc.contributor.authorLi, M.
dc.contributor.authorLi, Q.
dc.contributor.authorLi, Q.
dc.contributor.authorLi, Q. Y.
dc.contributor.authorLi, S.
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dc.contributor.authorLi, Z. H.
dc.contributor.authorLiang, M. J.
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dc.contributor.authorSiemko, A.
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dc.contributor.authorUbaldi, A.
dc.contributor.authorUrban, T.
dc.contributor.authorUsoskin, I.
dc.contributor.authorVagelli, V.
dc.contributor.authorVainio, R.
dc.contributor.authorVäisänen, P.
dc.contributor.authorValencia-Otero, M.
dc.contributor.authorValente, E.
dc.contributor.authorValtonen, E.
dc.contributor.authorVázquez Acosta, M.
dc.contributor.authorVecchi, M.
dc.contributor.authorVelasco, M.
dc.contributor.authorWang, C. X.
dc.contributor.authorWang, J. C.
dc.contributor.authorWang, L.
dc.contributor.authorWang, L. Q.
dc.contributor.authorWang, N. H.
dc.contributor.authorWang, Q. L.
dc.contributor.authorWang, S.
dc.contributor.authorWang, X.
dc.contributor.authorWang, Z. M.
dc.contributor.authorWei, J.
dc.contributor.authorWeng, Z. L.
dc.contributor.authorWu, H.
dc.contributor.authorWu, Y.
dc.contributor.authorWu, Z. B.
dc.contributor.authorXiao
dc.contributor.authorJ. N.
dc.contributor.authorXiong
dc.contributor.authorR. Q.
dc.contributor.authorXiong, X. Z.
dc.contributor.authorXu, W.
dc.contributor.authorYan, Q.
dc.contributor.authorYang, H. T.
dc.contributor.authorYang, Y.
dc.contributor.authorYi, H.
dc.contributor.authorYou, Y. H.
dc.contributor.authorYu, Y. M.
dc.contributor.authorYu, Z. Q.
dc.contributor.authorZhang, C.
dc.contributor.authorZhang, F. Z.
dc.contributor.authorZhang, J.
dc.contributor.authorZhang, J. H.
dc.contributor.authorZhang, Z.
dc.contributor.authorZhao, P. W.
dc.contributor.authorZheng, C.
dc.contributor.authorZheng, Z. M.
dc.contributor.authorZhuang, H. L.
dc.contributor.authorZhukov, V.
dc.contributor.authorZichichi, A.
dc.contributor.authorZuberi, M.
dc.contributor.authorZuccon, P.
dc.contributor.authorAMS Collaboration
dc.contributor.organizationfi=avaruustutkimuslaboratorio|en=Space Research Laboratory|
dc.contributor.organization-code1.2.246.10.2458963.20.47833719389
dc.converis.publication-id491490577
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/491490577
dc.date.accessioned2025-08-28T00:23:45Z
dc.date.available2025-08-28T00:23:45Z
dc.description.abstractWe report the properties of precision time structures of cosmic nuclei He, Li, Be, B, C, N, and O fluxes over an 11-year solar cycle from May 2011 to November 2022 in the rigidity range from 1.92 to 60.3 GV. The nuclei fluxes show similar but not identical time variations with amplitudes decreasing with increasing rigidity. In particular, below 3.64 GV the Li, Be, and B fluxes, and below 2.15 GV the C, N, and O fluxes, are significantly less affected by solar modulation than the He flux. We observe that these differences in solar modulation are linearly correlated with the differences in the spectral indices of the cosmic nuclei fluxes. This shows, in a model-independent way, that solar modulation of galactic cosmic nuclei depends on their spectral shape. In addition, solar modulation differences due to nuclei velocity dependence on the mass-to-charge ratio (A/Z) are not observed.
dc.identifier.eissn1079-7114
dc.identifier.jour-issn0031-9007
dc.identifier.olddbid205636
dc.identifier.oldhandle10024/188663
dc.identifier.urihttps://www.utupub.fi/handle/11111/56249
dc.identifier.urlhttps://doi.org/10.1103/physrevlett.134.051001
dc.identifier.urnURN:NBN:fi-fe2025082791002
dc.language.isoen
dc.okm.affiliatedauthorVainio, Rami
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherAmerican Physical Society (APS)
dc.publisher.countryUnited Statesen_GB
dc.publisher.countryYhdysvallat (USA)fi_FI
dc.publisher.country-codeUS
dc.relation.articlenumber051001
dc.relation.doi10.1103/PhysRevLett.134.051001
dc.relation.ispartofjournalPhysical Review Letters
dc.relation.issue5
dc.relation.volume134
dc.source.identifierhttps://www.utupub.fi/handle/10024/188663
dc.titleSolar Modulation of Cosmic Nuclei over a Solar Cycle: Results from the Alpha Magnetic Spectrometer
dc.year.issued2025

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