Home > Publications database > Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer > print

001     891400
005     20210623131804.0
024 7 _ |a 10.1103/PhysRevLett.126.041104
|2 doi
024 7 _ |a 0031-9007
|2 ISSN
024 7 _ |a 1079-7114
|2 ISSN
024 7 _ |a 1092-0145
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024 7 _ |a 2128/27480
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024 7 _ |a altmetric:98983189
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024 7 _ |a 33576661
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024 7 _ |a WOS:000612682500002
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037 _ _ |a FZJ-2021-01488
082 _ _ |a 530
100 1 _ |a Aguilar, M.
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245 _ _ |a Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer
260 _ _ |a College Park, Md.
|c 2021
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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 iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62×106 iron nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. Above 80.5 GV the rigidity dependence of the cosmic ray Fe flux is identical to the rigidity dependence of the primary cosmic ray He, C, and O fluxes, with the Fe/O flux ratio being constant at 0.155±0.006. This shows that unexpectedly Fe and He, C, and O belong to the same class of primary cosmic rays which is different from the primary cosmic rays Ne, Mg, and Si class.
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700 1 _ |a Zheng, C.
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700 1 _ |a Zhuang, H. L.
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700 1 _ |a Zuccon, P.
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|e Corresponding author
773 _ _ |a 10.1103/PhysRevLett.126.041104
|g Vol. 126, no. 4, p. 041104
|0 PERI:(DE-600)1472655-5
|n 4
|p 041104
|t Physical review letters
|v 126
|y 2021
|x 1079-7114
856 4 _ |u https://juser.fz-juelich.de/record/891400/files/PhysRevLett.126.041104.pdf
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Marc 21