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Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station

dc.contributor.authorAMS collaboration (296 authors)
dc.contributor.authorArruda, L.
dc.contributor.authorBarao, F.
dc.contributor.authorNunes, P.
dc.contributor.authorOrcinha, M.
dc.contributor.authorPereira, R.
dc.date.accessioned2019-02-04T06:47:15Z
dc.date.available2019-02-04T06:47:15Z
dc.date.issued2015-04-30
dc.date.updated2019-02-04T06:47:15Z
dc.description.abstractA precise measurement of the proton flux in primary cosmic rays with rigidity (momentum/charge) from 1 GV to 1.8 TV is presented based on 300 million events. Knowledge of the rigidity dependence of the proton flux is important in understanding the origin, acceleration, and propagation of cosmic rays. We present the detailed variation with rigidity of the flux spectral index for the first time. The spectral index progressively hardens at high rigidities.
dc.description.versionPeer Reviewed
dc.identifierPhys.Rev.Lett. 114 (2015) 171103; DOI 10.1103/PhysRevLett.114.171103
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevLett.114.171103
dc.identifier.urihttp://hdl.handle.net/10400.26/26836
dc.language.isoeng
dc.titlePrecision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station
dc.typejournal article
dspace.entity.typePublication
rcaap.rightsopenAccesspt
rcaap.typearticle

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