Primary Energy Spectra and Elemental Composition. GAMMA Experiment

Details Primary Energy Spectra and Elemental Composition. GAMMA Experiment Primary Energy Spectra and Elemental Composition. GAMMA Experiment

2005-06-24

arxiv.org/abs/astro-ph/0506588v1

Astronomy and Astrophysics

Astrophysics

11 pages, 14 figures, submitted to 29th International Cosmic Ray Conference, Pune

Scientific paper

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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