Home > Publications database > Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer > print

001     866676
005     20210130003600.0
024 7 _ |a 10.1103/PhysRevLett.123.181102
|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 2128/23436
|2 Handle
024 7 _ |a altmetric:69629914
|2 altmetric
024 7 _ |a pmid:31763896
|2 pmid
024 7 _ |a WOS:000493903400004
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037 _ _ |a FZJ-2019-05754
082 _ _ |a 530
100 1 _ |a Aguilar, M.
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245 _ _ |a Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer
260 _ _ |a College Park, Md.
|c 2019
|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 Precision measurements by the Alpha Magnetic Spectrometer (AMS) on the International Space Station of 3He and 4He fluxes are presented. The measurements are based on 100 million 4He nuclei in the rigidity range from 2.1 to 21 GV and 18 million 3He from 1.9 to 15 GV collected from May 2011 to November 2017. We observed that the 3He and 4He fluxes exhibit nearly identical variations with time. The relative magnitude of the variations decreases with increasing rigidity. The rigidity dependence of the 3He/4He flux ratio is measured for the first time. Below 4 GV, the 3He/4He flux ratio was found to have a significant long-term time dependence. Above 4 GV, the 3He/4He flux ratio was found to be time independent, and its rigidity dependence is well described by a single power law ∝RΔ with Δ=−0.294±0.004. Unexpectedly, this value is in agreement with the B/O and B/C spectral indices at high energies.
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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.123.181102
|g Vol. 123, no. 18, p. 181102
|0 PERI:(DE-600)1472655-5
|n 18
|p 181102
|t Physical review letters
|v 123
|y 2019
|x 1079-7114
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Marc 21