Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays: Results from AMS-01

Relative Composition and Energy Spectra of Light Nuclei in Cosmic Rays: Results from AMS-01

Measurement of the chemical and isotopic composition of cosmic rays is essential for the precise understanding of their propagation in the galaxy. While the model parameters are mainly determined using the B/C ratio, the study of extended sets of ratios can provide stronger constraints on the propag...

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Main Authors: Becker, R. (Contributor), Becker, Ulrich J. (Contributor), Berges, P. (Contributor), Burger, Joseph D. (Contributor), Cai, X. D. (Contributor), Capell, Michael H. (Contributor), Dai, T. S. (Contributor), Eppling, Frederic J. (Contributor), Fisher, Peter H. (Contributor), Galaktionov, Y. (Contributor), Klimentov, A. (Contributor), Kounine, Andrei (Contributor), Koutsenko, Vladimir (Contributor), Lebedev, Alexei (Contributor), Luckey, P. David, Jr (Contributor), Shoutko, V. (Contributor), Siedenburg, T. (Contributor), Steuer, M. (Contributor), Ting, Samuel C. C. (Contributor), Ting, Susan Marks (Contributor), Wu, Xiaohua Sherry (Contributor), Xu, S. (Contributor), Zhou, F. (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), Massachusetts Institute of Technology. Laboratory for Nuclear Science (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2013-01-18T20:25:00Z.
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