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arXiv · 1106.2268

Light Nuclei and Isotope Abundances in Cosmic Rays. Results from AMS-01

N. Tomassetti
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Abstract

Observations of the chemical and isotopic composition of light cosmic-ray nuclei can be used to constrain the astrophysical models of cosmic-ray transport and interactions in the Galaxy. Nearly 200,000 light nuclei (Z>2) have been observed by AMS-01 during the 10-day flight STS-91 in June 1998. Using these data, we have measured the relative abundance of light nuclei Li, Be, B and C in the kinetic energy range 0.35 - 45 GeV/nucleon.

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N. Tomassetti. 2012-10-26. Light Nuclei and Isotope Abundances in Cosmic Rays. Results from AMS-01. https://doi.org/10.1142/9789814329033_0040

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