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Primary cosmic ray energy spectrum in terms of the GAMMA muon data

โœ Scribed by A.P. Garyaka; R.M. Martirosov; S.V. Ter-Antonyan; A.D. Erlykin; N.M. Nikolskaya; Y.A. Gallant; L.W. Jones; J. Procureur

Publisher
Elsevier Science
Year
2009
Tongue
English
Weight
237 KB
Volume
196
Category
Article
ISSN
0920-5632

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โœฆ Synopsis

The energy spectrum of the primary cosmic rays is obtained by conversion from the truncated muon size spectrum of EAS studied with the GAMMA array. The previously observed dependence of E0 on N tr ยต at various zenith angles is used. It is shown that the present spectrum has the same structure ("bump") as the spectrum determined by another independent multi-parametric energy estimation method confirming that the "bump" structure is not produced by uncertainties in our methods.

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## Abstract In a recent paper BHATTACHARYYA has derived the pion and kaon production spectra in the atmosphere using a form of the primary nucleon energy spectrum of the measurements of GRIGOROV et al. and the interaction model of BUGAEV et al. The sea level muon spectrum derived from these meson s