Abstract
To date, very little has been done in the field of research of the nuclei cosmic ray spectra in the energy range between 1 and 10 TeV per nucleon and especially there were even fewer direct measurements in space. The PAMELA experiment (Casolini et al., 2008) has a possibility to make progress in this range. The method of the measurement of the helium and proton cosmic ray spectra with the energy higher than 50 GeV/nucleon was developed mainly with the use of the PAMELA calorimeter. This analysis method and the results obtained based on 3 years of measurements are presented. © 2011 Author(s).
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CITATION STYLE
Karelin, A. V., Borisov, S. V., Galper, A. M., & Voronov, S. A. (2011). The Proton and Helium cosmic ray spectra from 50 GeV to 15 TeV. Astrophysics and Space Sciences Transactions, 7(2), 235–238. https://doi.org/10.5194/astra-7-235-2011
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