Properties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen

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dc.contributor.authorWeng ZL
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dc.contributor.authorYang Y
dc.contributor.authorYashin II
dc.contributor.authorYi H
dc.contributor.authorYu YM
dc.contributor.authorYu ZQ
dc.contributor.authorZannoni M
dc.contributor.authorZhang C
dc.contributor.authorZhang F
dc.contributor.authorZhang FZ
dc.contributor.authorZhang JH
dc.contributor.authorZhang Z
dc.contributor.authorZhao F
dc.contributor.authorZheng C
dc.contributor.authorZheng ZM
dc.contributor.authorZhuang HL
dc.contributor.authorZhukov V
dc.contributor.authorZichichi A
dc.contributor.authorZuccon P
dc.contributor.organizationfi=avaruustutkimuslaboratorio|en=Space Research Laboratory|
dc.contributor.organization-code1.2.246.10.2458963.20.47833719389
dc.contributor.organization-code2606702
dc.converis.publication-id66601942
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/66601942
dc.date.accessioned2022-10-28T13:06:22Z
dc.date.available2022-10-28T13:06:22Z
dc.description.abstractWe report the properties of sodium (Na) and aluminum (Al) cosmic rays in the rigidity range 2.15 GV to 3.0 TV based on 0.46 million sodium and 0.51 million aluminum nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. We found that Na and Al, together with nitrogen (N), belong to a distinct cosmic ray group. In this group, we observe that, similar to the N flux, both the Na flux and Al flux are well described by the sums of a primary cosmic ray component (proportional to the silicon flux) and a secondary cosmic ray component (proportional to the fluorine flux). The fraction of the primary component increases with rigidity for the N, Na, and Al fluxes and becomes dominant at the highest rigidities. The Na/Si and Al/Si abundance ratios at the source, 0.036 +/- 0.003 for Na/Si and 0.103 +/- 0.004 for Al/Si, are determined independent of cosmic ray propagation.
dc.identifier.jour-issn0031-9007
dc.identifier.olddbid179735
dc.identifier.oldhandle10024/162829
dc.identifier.urihttps://www.utupub.fi/handle/11111/37443
dc.identifier.urnURN:NBN:fi-fe2021093048573
dc.language.isoen
dc.okm.affiliatedauthorTorsti, Jarmo
dc.okm.affiliatedauthorVainio, Rami
dc.okm.affiliatedauthorValtonen, Eino
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.publisherAMER PHYSICAL SOC
dc.publisher.countryUnited Statesen_GB
dc.publisher.countryYhdysvallat (USA)fi_FI
dc.publisher.country-codeUS
dc.relation.articlenumberARTN 021101
dc.relation.doi10.1103/PhysRevLett.127.021101
dc.relation.ispartofjournalPhysical Review Letters
dc.relation.issue2
dc.relation.volume127
dc.source.identifierhttps://www.utupub.fi/handle/10024/162829
dc.titleProperties of a New Group of Cosmic Nuclei: Results from the Alpha Magnetic Spectrometer on Sodium, Aluminum, and Nitrogen
dc.year.issued2021

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