Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer

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dc.contributor.authorYu YM
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dc.contributor.authorZannoni M
dc.contributor.authorZhang C
dc.contributor.authorZhang F
dc.contributor.authorZhang FZ
dc.contributor.authorZhang JH
dc.contributor.authorZhang Z
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dc.contributor.authorZheng ZM
dc.contributor.authorZhuang HL
dc.contributor.authorZhukov V
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dc.contributor.authorZuccon P
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dc.contributor.authorZimmermann N
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dc.contributor.authorZhang FZ
dc.contributor.authorZhang F
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-id53417495
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/53417495
dc.date.accessioned2022-10-27T12:20:16Z
dc.date.available2022-10-27T12:20:16Z
dc.description.abstractWe report the observation of new properties of primary iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62 x 10(6) iron nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. Above 80.5 GV the rigidity dependence of the cosmic ray Fe flux is identical to the rigidity dependence of the primary cosmic ray He, C, and O fluxes, with the Fe/O flux ratio being constant at 0.155 +/- 0.006. This shows that unexpectedly Fe and He, C, and O belong to the same class of primary cosmic rays which is different from the primary cosmic rays Ne, Mg, and Si class.
dc.identifier.eissn1079-7114
dc.identifier.jour-issn0031-9007
dc.identifier.olddbid174823
dc.identifier.oldhandle10024/157917
dc.identifier.urihttps://www.utupub.fi/handle/11111/34905
dc.identifier.urlhttps://journals.aps.org/prl/abstract/10.1103/PhysRevLett.126.041104
dc.identifier.urnURN:NBN:fi-fe2021042823261
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 041104
dc.relation.doi10.1103/PhysRevLett.126.041104
dc.relation.ispartofjournalPhysical Review Letters
dc.relation.issue4
dc.relation.volume126
dc.source.identifierhttps://www.utupub.fi/handle/10024/157917
dc.titleProperties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer
dc.year.issued2021

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