Physics – Nuclear Physics
Scientific paper
Dec 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009nuphs.196..173m&link_type=abstract
Nuclear Physics B Proceedings Supplements, Volume 196, p. 173-178.
Physics
Nuclear Physics
Scientific paper
The all-particle energy spectrum of the primary cosmic rays at energies 1-200 PeV has been obtained on the basis of the GAMMA experimental data using the event-by-event method of the primary energy evaluation from the measured N, N and shower age (s) parameters. The energy estimation method was developed using the CORSIKA simulation code in the frames of the SIBYLL interaction model taking into account the response of the GAMMA detectors and the reconstruction uncertainties of the EAS parameters. The observed ‘bump’ at ˜7.4ṡ107 GeV can be described by a two-component model of primary cosmic ray origin.
Erlykin Anatoly D.
Gallant Yves A.
Garyaka Alexandr P.
Jones Linwood W.
Martirosov Romen M.
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