Astrophys. Space Sci. Trans., 7, 235-238, 2011
www.astrophys-space-sci-trans.net/7/235/2011/
doi:10.5194/astra-7-235-2011
© Author(s) 2011. This work is distributed
under the Creative Commons Attribution 3.0 License.
 
27 Jun 2011
The Proton and Helium cosmic ray spectra from 50 GeV to 15 TeV
A. V. Karelin1, S. V. Borisov1,2, A. M. Galper1, and S. A. Voronov for PAMELA collaboration1
1NRNU MEPhI, Moscow, Russia
2INFN, Structure of Rome "or Vergata" and Physics Department of University of Rome "Tor Vergata", Italy

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.

Citation: Karelin, A. V., Borisov, S. V., Galper, A. M., and S. A. Voronov for PAMELA collaboration: The Proton and Helium cosmic ray spectra from 50 GeV to 15 TeV, Astrophys. Space Sci. Trans., 7, 235-238, doi:10.5194/astra-7-235-2011, 2011.
 
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