Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer

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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 ZM
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dc.contributor.authorZimmermann N
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-id48457424
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/48457424
dc.date.accessioned2022-10-28T14:06:34Z
dc.date.available2022-10-28T14:06:34Z
dc.description.abstractWe report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8 x 10(6) Ne, 2.2 x 10(6) Mg, and 1.6 x 10(6) Si nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The Ne and Mg spectra have identical rigidity dependence above 3.65 GV. The three spectra have identical rigidity dependence above 86.5 GV, deviate from a single power law above 200 GV, and harden in an identical way. Unexpectedly, above 86.5 GV the rigidity dependence of primary cosmic rays Ne, Mg, and Si spectra is different from the rigidity dependence of primary cosmic rays He, C, and O. This shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary cosmic rays.
dc.identifier.eissn1079-7114
dc.identifier.jour-issn0031-9007
dc.identifier.olddbid186311
dc.identifier.oldhandle10024/169405
dc.identifier.urihttps://www.utupub.fi/handle/11111/37063
dc.identifier.urnURN:NBN:fi-fe2021042825125
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 211102
dc.relation.doi10.1103/PhysRevLett.124.211102
dc.relation.ispartofjournalPhysical Review Letters
dc.relation.issue21
dc.relation.volume124
dc.source.identifierhttps://www.utupub.fi/handle/10024/169405
dc.titleProperties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer
dc.year.issued2020

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