Hauptseite > Publikationsdatenbank > Observation of Fine Time Structures in the Cosmic Proton and Helium Fluxes with the Alpha Magnetic Spectrometer on the International Space Station > print

001     851759
005     20210129235014.0
024 7 _ |a 10.1103/PhysRevLett.121.051101
|2 doi
024 7 _ |a 0031-9007
|2 ISSN
024 7 _ |a 1079-7114
|2 ISSN
024 7 _ |a 1092-0145
|2 ISSN
024 7 _ |a 2128/19688
|2 Handle
024 7 _ |a pmid:30118264
|2 pmid
024 7 _ |a WOS:000440386100001
|2 WOS
024 7 _ |a altmetric:46134259
|2 altmetric
037 _ _ |a FZJ-2018-05283
082 _ _ |a 550
100 1 _ |a Aguilar, M.
|0 P:(DE-HGF)0
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245 _ _ |a Observation of Fine Time Structures in the Cosmic Proton and Helium Fluxes with the Alpha Magnetic Spectrometer on the International Space Station
260 _ _ |a College Park, Md.
|c 2018
|b APS
336 7 _ |a article
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336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
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|s 1552578372_31636
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336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
520 _ _ |a We present the precision measurement from May 2011 to May 2017 (79 Bartels rotations) of the proton fluxes at rigidities from 1 to 60 GV and the helium fluxes from 1.9 to 60 GV based on a total of 1×109 events collected with the Alpha Magnetic Spectrometer aboard the International Space Station. This measurement is in solar cycle 24, which has the solar maximum in April 2014. We observed that, below 40 GV, the proton flux and the helium flux show nearly identical fine structures in both time and relative amplitude. The amplitudes of the flux structures decrease with increasing rigidity and vanish above 40 GV. The amplitudes of the structures are reduced during the time period, which started one year after solar maximum, when the proton and helium fluxes steadily increase. Above ∼3  GV the p/He flux ratio is time independent. We observed that below ∼3  GV the ratio has a long-term decrease coinciding with the period during which the fluxes start to rise.
536 _ _ |a 513 - Supercomputer Facility (POF3-513)
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536 _ _ |a Cosmic-ray physics with the AMS experiment on the International Space Station (jara0052_20150501)
|0 G:(DE-Juel1)jara0052_20150501
|c jara0052_20150501
|f Cosmic-ray physics with the AMS experiment on the International Space Station
|x 1
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