Primary Energy Spectra and Elemental Composition. GAMMA Experiment
Ter-Antonyan, S. V. · Martirosov, R. M. · Garyaka, A. P. · Eganov, V. · Nikolskaya, N. · Episkoposyan, T. · Procureur, J. · Gallant, Y. · Jones, L.
Original · EN
On the basis of the Extensive Air Shower data observed by the GAMMA experiment the energy spectra and elemental composition of the primary cosmic rays have been derived in the 1-100 PeV energy range. Reconstruction of the primary energy spectra is carried out in the framework of the SIBYLL and QGSJET interaction models and the hypothesis of the power-law steepening primary energy spectra. All presented results are derived taking into account the detector response, reconstruction uncertainties of EAS parameters and fluctuation of EAS development.
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