Hauptseite > Publikationsdatenbank > Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer > print

001     877692
005     20210213131240.0
024 7 _ |a 10.1103/PhysRevLett.124.211102
|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 2128/25146
|2 Handle
024 7 _ |a altmetric:83024072
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024 7 _ |a pmid:32530660
|2 pmid
024 7 _ |a WOS:000536404500001
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037 _ _ |a FZJ-2020-02402
082 _ _ |a 530
100 1 _ |a Aguilar, M.
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|e Corresponding author
245 _ _ |a Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer
260 _ _ |a College Park, Md.
|c 2020
|b APS
336 7 _ |a article
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336 7 _ |a Output Types/Journal article
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336 7 _ |a Journal Article
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336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
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336 7 _ |a Journal Article
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520 _ _ |a We report the observation of new properties of primary cosmic rays, neon (Ne), magnesium (Mg), and silicon (Si), measured in the rigidity range 2.15 GV to 3.0 TV with 1.8×106  Ne, 2.2×106  Mg, and 1.6×106  Si nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. The Ne and Mg spectra have identical rigidity dependence above 3.65 GV. The three spectra have identical rigidity dependence above 86.5 GV, deviate from a single power law above 200 GV, and harden in an identical way. Unexpectedly, above 86.5 GV the rigidity dependence of primary cosmic rays Ne, Mg, and Si spectra is different from the rigidity dependence of primary cosmic rays He, C, and O. This shows that the Ne, Mg, and Si and He, C, and O are two different classes of primary cosmic rays.
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536 _ _ |a Cosmic-ray physics with the AMS experiment on the International Space Station (jara0052_20150501)
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|f Cosmic-ray physics with the AMS experiment on the International Space Station
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773 _ _ |a 10.1103/PhysRevLett.124.211102
|g Vol. 124, no. 21, p. 211102
|0 PERI:(DE-600)1472655-5
|n 21
|p 211102
|t Physical review letters
|v 124
|y 2020
|x 1079-7114
856 4 _ |u https://juser.fz-juelich.de/record/877692/files/PhysRevLett.124.211102.pdf
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Marc 21