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Test of primary model predictions by EAS size spectra

2001/06/06 by Samvel Ter-Antonyan, Ter-Antonyan, Samvel, Peter Biermann +1
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0106091

4 pages, 4 figures, to appear in proceedings of 27th ICRC (Hamburg, August 7-15, 2001)

arxiv created 2001/06/29 · arxiv updated 2009/12/01

Abstract

High statistical accuracy of experiments KASCADE and ANI allowed to obtain approximations of primary energy spectra and elemental composition in the "knee" region. Obtained results point out to the correctness of QGSJET interaction model and 2-component model of primary cosmic ray origin up to 100 PeV energies.

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