The Alpha Magnetic Spectrometer (AMS) on the international space station: Part II — Results from the first seven years

dc.contributor.authorM.Aguilar
dc.contributor.authorL.Ali Cavasonza
dc.contributor.authorG.Ambrosi
dc.contributor.authorL.Arruda
dc.contributor.authorN.Attig
dc.contributor.authorF.Barao
dc.contributor.authorL.Barrin
dc.contributor.authorA.Bartoloni
dc.contributor.authorS.Başeğmez-du Pree
dc.contributor.authoraJ.Bates
dc.contributor.authorR.Battiston
dc.contributor.authorM.Behlmann
dc.contributor.authorB.Beischer
dc.contributor.authorJ.Berdugo
dc.contributor.authorB.Bertucci
dc.contributor.authorV.Bindi
dc.contributor.authorW.de Boer
dc.contributor.authorK.Bollweg
dc.contributor.authorB.Borgia
dc.contributor.authorM.J.Boschini
dc.contributor.authorM.Bourquin
dc.contributor.authorE.F.Bueno
dc.contributor.authorJ.Burger
dc.contributor.authorW.J.Burger
dc.contributor.authorS.Burmeister
dc.contributor.authorX.D.Cai
dc.contributor.authorM.Capell
dc.contributor.authorJ.Casaus
dc.contributor.authorG.Castellini
dc.contributor.authorF.Cervelli
dc.contributor.authorY.H.Chang
dc.contributor.authorG.M.Chen
dc.contributor.authorH.S.Chen
dc.contributor.authorY.Chen
dc.contributor.authorL.Cheng
dc.contributor.authorH.Y.Chou
dc.contributor.authorS.Chouridou
dc.contributor.authorV.Choutko
dc.contributor.authorC.H.Chung
dc.contributor.authorC.Clark
dc.contributor.authorG.Coignet
dc.contributor.authorC.Consolandi
dc.contributor.authorA.Contin
dc.contributor.authorC.Corti
dc.contributor.authorZ.Cui
dc.contributor.authorK.Dadzie
dc.contributor.authorY.M.Dai
dc.contributor.authorC.Delgado
dc.contributor.authorS.Della Torre
dc.contributor.authorM.B.Demirköz
dc.contributor.authorL.Derome
dc.contributor.authorS.Di Falco
dc.contributor.authorV.Di Felice
dc.contributor.authorbC.Díaz
dc.contributor.authorF.Dimiccoli
dc.contributor.authorP.von Doetinchem
dc.contributor.authorF.Dong
dc.contributor.authorF.Donnini
dc.contributor.authorbM.Duranti
dc.contributor.authorA.Egorov
dc.contributor.authorA.Eline
dc.contributor.authorJ.Feng
dc.contributor.authorE.Fiandrini
dc.contributor.authorP.Fisher
dc.contributor.authorV.Formato
dc.contributor.authorbC.Freeman
dc.contributor.authorY.Galaktionov
dc.contributor.authorC.Gámez
dc.contributor.authorR.J.García-López
dc.contributor.authorC.Gargiulo
dc.contributor.authorH.Gast
dc.contributor.authorI.Gebauer
dc.contributor.authorM.Gervasi
dc.contributor.authorF.Giovacchini
dc.contributor.authorD.M.Gómez-Coral
dc.contributor.authorJ.Gong
dc.contributor.authorC.Goy
dc.contributor.authorV.Grabski
dc.contributor.authorD.Grandi
dc.contributor.authorM.Graziani
dc.contributor.authorK.H.Guo
dc.contributor.authorS.Haino
dc.contributor.authorK.C.Han
dc.contributor.authorR.K.Hashmani
dc.contributor.authorZ.H.He
dc.contributor.authorB.Heber
dc.contributor.authorT.H.Hsieh
dc.contributor.authorJ.Y.Hu
dc.contributor.authorZ.C.Huang
dc.contributor.authorW.Hungerford
dc.contributor.authorM.Incagli
dc.contributor.authorW.Y.Jang
dc.contributor.authorYiJia
dc.contributor.authorH.Jinchi
dc.contributor.authorK.Kanishev
dc.contributor.authorB.Khiali
dc.contributor.authorbG.N.Kim
dc.contributor.authorTh.Kirn
dc.contributor.authorM.Konyushikhin
dc.contributor.authorO.Kounina
dc.contributor.authorA.Kounine
dc.contributor.authorV.Koutsenko
dc.contributor.authorA.Kuhlman
dc.contributor.authorA.Kulemzin
dc.contributor.authorG.La Vacca
dc.contributor.authorE.Laudi
dc.contributor.authorG.Laurenti
dc.contributor.authorI.Lazzizzera
dc.contributor.authorA.Lebedev
dc.contributor.authorH.T.Lee
dc.contributor.authorS.C.Lee
dc.contributor.authorC.Leluc
dc.contributor.authorJ.Q.Li
dc.contributor.authorM.Li
dc.contributor.authorQ.Li
dc.contributor.authorS.Li
dc.contributor.authorT.X.Li
dc.contributor.authorZ.H.Li
dc.contributor.authorC.Light
dc.contributor.authorC.H.Lin
dc.contributor.authorT.Lippert
dc.contributor.authorZ.Liu
dc.contributor.authorS.Q.Lu
dc.contributor.authorY.S.Lu
dc.contributor.authorK.Luebelsmeyer
dc.contributor.authorJ.Z.Luo
dc.contributor.authorS.S.Lyu
dc.contributor.authorF.Machate
dc.contributor.authorC.Mañá
dc.contributor.authorJ.Marín
dc.contributor.authorJ.Marquardt
dc.contributor.authorT.Martin
dc.contributor.authorG.Martínez
dc.contributor.authorN.Masi
dc.contributor.authorD.Maurin
dc.contributor.authorA.Menchaca-Rocha
dc.contributor.authorQ.Meng
dc.contributor.authorD.C.Mo
dc.contributor.authorM.Molero
dc.contributor.authorP.Mott
dc.contributor.authorL.Mussolin
dc.contributor.authorJ.Q.Ni
dc.contributor.authorN.Nikonov
dc.contributor.authorF.Nozzoli
dc.contributor.authorA.Oliva
dc.contributor.authorM.Orcinha
dc.contributor.authorM.Palermo
dc.contributor.authorF.Palmonari
dc.contributor.authorM.Paniccia
dc.contributor.authorA.Pashnin
dc.contributor.authorM.Pauluzzi
dc.contributor.authorS.Pensotti
dc.contributor.authorH.D.Phan
dc.contributor.authorV.Plyaskin
dc.contributor.authorM.Pohl
dc.contributor.authorS.Porter
dc.contributor.authorX.M.Qi
dc.contributor.authorX.Qin
dc.contributor.authorZ.Y.Qu
dc.contributor.authorL.Quadrani
dc.contributor.authorP.G.Rancoita
dc.contributor.authorD.Rapin
dc.contributor.authorA.Reina Conde
dc.contributor.authorS.Rosier-Lees
dc.contributor.authorA.Rozhkov
dc.contributor.authorD.Rozza
dc.contributor.authorR.Sagdeev
dc.contributor.authorS.Schael
dc.contributor.authorS.M.Schmidt
dc.contributor.authorA.Schulz von Dratzig
dc.contributor.authorG.Schwering
dc.contributor.authorE.S.Seo
dc.contributor.authorB.S.Shan
dc.contributor.authorJ.Y.Shi
dc.contributor.authorT.Siedenburg
dc.contributor.authorC.Solano
dc.contributor.authorJ.W.Song
dc.contributor.authorR.Sonnabend
dc.contributor.authorQ.Sun
dc.contributor.authorZ.T.Sun
dc.contributor.authorM.Tacconi
dc.contributor.authorX.W.Tang
dc.contributor.authorZ.C.Tang
dc.contributor.authorJ.Tian
dc.contributor.authorSamuel C.C.Ting
dc.contributor.authorS.M.Ting
dc.contributor.authorN.Tomassetti
dc.contributor.authorJ.Torsti
dc.contributor.authorC.Tüysüz
dc.contributor.authorT.Urban
dc.contributor.authorI.Usoskin
dc.contributor.authorV.Vagelli
dc.contributor.authorR.Vainio
dc.contributor.authorE.Valente
dc.contributor.authorE.Valtonen
dc.contributor.authorM.Vázquez Acosta
dc.contributor.authorM.Vecchi
dc.contributor.authorM.Velasco
dc.contributor.authorJ.P.Vialle
dc.contributor.authorL.Q.Wang
dc.contributor.authorN.H.Wang
dc.contributor.authorQ.L.Wang
dc.contributor.authorS.Wang
dc.contributor.authorX.Wang
dc.contributor.authorZ.X.Wang
dc.contributor.authorJ.Wei
dc.contributor.authorZ.L.Weng
dc.contributor.authorH.Wu
dc.contributor.authorR.Q.Xiong
dc.contributor.authorW.Xu
dc.contributor.authorQ.Yan
dc.contributor.authorY.Yang
dc.contributor.authorH.Yi
dc.contributor.authorY.J.Yu
dc.contributor.authorZ.Q.Yu
dc.contributor.authorM.Zannoni
dc.contributor.authorC.Zhang
dc.contributor.authorF.Zhang
dc.contributor.authorF.Z.Zhang
dc.contributor.authorJ.H.Zhang
dc.contributor.authorZ.Zhang
dc.contributor.authorF.Zhao
dc.contributor.authorZ.M.Zheng
dc.contributor.authorH.L.Zhuang
dc.contributor.authorV.Zhukov
dc.contributor.authorA.Zichichi
dc.contributor.authorN.Zimmermann
dc.contributor.authorP.Zuccon
dc.contributor.authorAMS Collaboration
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-id50976045
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/50976045
dc.date.accessioned2025-08-28T02:19:53Z
dc.date.available2025-08-28T02:19:53Z
dc.description.abstract<p>The Alpha Magnetic Spectrometer (AMS) is a precision particle physics detector on the International Space Station (ISS) conducting a unique, long-duration mission of fundamental physics research in space. The physics objectives include the precise studies of the origin of dark matter, antimatter, and cosmic rays as well as the exploration of new phenomena. Following a 16-year period of construction and testing, and a precursor flight on the Space Shuttle, AMS was installed on the ISS on May 19, 2011. In this report we present results based on 120 billion charged cosmic ray events up to multi-TeV energies. This includes the fluxes of positrons, electrons, antiprotons, protons, and nuclei. These results provide unexpected information, which cannot be explained by the current theoretical models. The accuracy and characteristics of the data, simultaneously from many different types of cosmic rays, provide unique input to the understanding of origins, acceleration, and propagation of cosmic rays.<br /></p>
dc.identifier.eissn1873-6270
dc.identifier.jour-issn0370-1573
dc.identifier.olddbid208938
dc.identifier.oldhandle10024/191965
dc.identifier.urihttps://www.utupub.fi/handle/11111/36323
dc.identifier.urnURN:NBN:fi-fe2021042823168
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.typeA2 Scientific Article
dc.publisherElsevier B.V.
dc.publisher.countryNetherlandsen_GB
dc.publisher.countryAlankomaatfi_FI
dc.publisher.country-codeNL
dc.relation.doi10.1016/j.physrep.2020.09.003
dc.relation.ispartofjournalPhysics Reports
dc.source.identifierhttps://www.utupub.fi/handle/10024/191965
dc.titleThe Alpha Magnetic Spectrometer (AMS) on the international space station: Part II — Results from the first seven years
dc.year.issued2021

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