Test of primary model predictions by EAS size spectra

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

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Astrophysics

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https://dspace.dare.co.zw/handle/123456789/53963

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