Test of primary model predictions by EAS size spectra

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dc.creatorTer-Antonyan, Samvel
dc.creatorBiermann, Peter
dc.date2001-06-06
dc.date2001-06-29
dc.date.accessioned2026-07-25T18:09:39Z
dc.descriptionHigh 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.
dc.description4 pages, 4 figures, to appear in proceedings of 27th ICRC (Hamburg, August 7-15, 2001)
dc.identifierhttps://arxiv.org/abs/astro-ph/0106091
dc.identifierhttp://arxiv.org/abs/astro-ph/0106091
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/53963
dc.subjectAstrophysics
dc.titleTest of primary model predictions by EAS size spectra
dc.typetext

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