Abstract
Techniques for measuring helium nuclei and proton energy spectra in circumterrestrial space were developed on the basis of simulated data and data from the position-sensitive silicon-tungsten calorimeter in the PAMELA satellite experiment. The thickness of the calorimeter is 0.6 nuclear interaction lengths. In this work, the experimental results for the measured energy spectra of the protons and helium nuclei of cosmic rays with energies above 50 GeV are presented.
Original language | English |
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Pages (from-to) | 327-330 |
Number of pages | 4 |
Journal | Bulletin of the Russian Academy of Sciences: Physics |
Volume | 75 |
Issue number | 3 |
DOIs | |
State | Published - Mar 2011 |
Externally published | Yes |
Bibliographical note
Funding Information:This work was supported by the Russian Founda tion for Basic Research, project no. 10 02 01301a, and performed as part of the program Scientific and Pedagogical Personnel of an Innovative Russia, 2009– 2013.
Funding
This work was supported by the Russian Founda tion for Basic Research, project no. 10 02 01301a, and performed as part of the program Scientific and Pedagogical Personnel of an Innovative Russia, 2009– 2013.
Funders | Funder number |
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Russian Founda tion for Basic Research | 10 02 01301a |