Notice
This is not the latest version of this item. The latest version can be found at:https://dspace.mit.edu/handle/1721.1/141736.3
Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer
Author(s)
Unknown author
DownloadPublished version (883.8Kb)
Publisher with Creative Commons License
Publisher with Creative Commons License
Creative Commons Attribution
Terms of use
Metadata
Show full item recordAbstract
© 2021 authors. Published by the American Physical Society. 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.
Date issued
2021Journal
Physical Review Letters
Publisher
American Physical Society (APS)
Citation
2021. "Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer." Physical Review Letters, 126 (4).
Version: Final published version