Test of primary model predictions by EAS size spectra

(2) Max-Plank-Institute fur Radioastronomie; Armenia; Bonn; Germany); Peter Biermann (2) ((1) Yerevan Physics Institute; Samvel Ter-Antonyan (1); Yerevan

arxiv: astro-ph/0106091 · v4 · submitted 2001-06-06 · 🌌 astro-ph

Test of primary model predictions by EAS size spectra

Samvel Ter-Antonyan (1) , Peter Biermann (2) ((1) Yerevan Physics Institute , Yerevan , Armenia , (2) Max-Plank-Institute fur Radioastronomie , Bonn , Germany) This is my paper

classification 🌌 astro-ph

keywords modelprimaryspectraaccuracyallowedapproximationscomponentcomposition

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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.

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Test of primary model predictions by EAS size spectra

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