Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station

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dc.contributor.authorZeissler S
dc.contributor.authorZhang C
dc.contributor.authorZhang F
dc.contributor.authorZhang J
dc.contributor.authorZhang JH
dc.contributor.authorZhang SW
dc.contributor.authorZhang Z
dc.contributor.authorZheng ZM
dc.contributor.authorZhuang HL
dc.contributor.authorZhukov V
dc.contributor.authorZichichi A
dc.contributor.authorZimmermann N
dc.contributor.authorZuccon P
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dc.contributor.authorZichichi A
dc.contributor.authorZimmermann N
dc.contributor.authorZhuang HL
dc.contributor.authorZhukov V
dc.contributor.authorZhang Z
dc.contributor.authorZheng ZM
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dc.contributor.authorZeissler S
dc.contributor.authorZhang C
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-id30039809
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/30039809
dc.date.accessioned2025-08-27T23:31:25Z
dc.date.available2025-08-27T23:31:25Z
dc.description.abstractWe report on the observation of new properties of secondary cosmic rays Li, Be, and B measured in the rigidity (momentum per unit charge) range 1.9 GV to 3.3 TV with a total of 5.4 x 10(6) nuclei collected by AMS during the first five years of operation aboard the International Space Station. The Li and B fluxes have an identical rigidity dependence above 7 GV and all three fluxes have an identical rigidity dependence above 30 GV with the Li/Be flux ratio of 2.0 +/- 0.1. The three fluxes deviate from a single power law above 200 GV in an identical way. This behavior of secondary cosmic rays has also been observed in the AMS measurement of primary cosmic rays He, C, and O but the rigidity dependences of primary cosmic rays and of secondary cosmic rays are distinctly different. In particular, above 200 GV, the secondary cosmic rays harden more than the primary cosmic rays.
dc.identifier.eissn1079-7114
dc.identifier.jour-issn0031-9007
dc.identifier.olddbid204117
dc.identifier.oldhandle10024/187144
dc.identifier.urihttps://www.utupub.fi/handle/11111/52308
dc.identifier.urnURN:NBN:fi-fe2021042718838
dc.language.isoen
dc.okm.affiliatedauthorBattarbee, Markus
dc.okm.affiliatedauthorEronen, Timo
dc.okm.affiliatedauthorTorsti, Jarmo
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.articlenumber021101
dc.relation.doi10.1103/PhysRevLett.120.021101
dc.relation.ispartofjournalPhysical Review Letters
dc.relation.issue2
dc.relation.volume120
dc.source.identifierhttps://www.utupub.fi/handle/10024/187144
dc.titleObservation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station
dc.year.issued2018

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