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

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dc.contributor.authorAguilar, M.
dc.contributor.authorCavasonza, L. A.
dc.contributor.authorAllen, M. S.
dc.contributor.authorAlpat, B.
dc.contributor.authorMikhailov, V. V.
dc.contributor.authorYashin, I. I.
dc.contributor.authorМихайлов, Владимир Владимирович
dc.contributor.authorЯшин, Игорь Иванович
dc.date.accessioned2024-11-29T11:30:22Z
dc.date.available2024-11-29T11:30:22Z
dc.date.issued2021
dc.description.abstract© 2021 authors. Published by the American Physical Society.We report the observation of new properties of primary iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62×106 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.citationProperties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer / Aguilar, M. [et al.] // Physical Review Letters. - 2021. - 126. - № 4. - 10.1103/PhysRevLett.126.041104
dc.identifier.doi10.1103/PhysRevLett.126.041104
dc.identifier.urihttps://www.doi.org/10.1103/PhysRevLett.126.041104
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dc.identifier.urihttp://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=Alerting&SrcApp=Alerting&DestApp=WOS_CPL&DestLinkType=FullRecord&UT=WOS:000612682500002
dc.identifier.urihttps://openrepository.mephi.ru/handle/123456789/23640
dc.relation.ispartofPhysical Review Letters
dc.titleProperties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer
dc.typeArticle
dspace.entity.typePublication
oaire.citation.issue4
oaire.citation.volume126
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