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

Autor:	J. Procureur, R. M. Martirosov, A.P. Garyaka, L. W. Jones, Y. A. Gallant, N. M. Nikolskaya, S.V. Ter-Antonyan, A.D. Erlykin
Rok vydání:	2009
Předmět:	Physics Nuclear and High Energy Physics Energy estimation Muon Primary (astronomy) Astrophysics::High Energy Astrophysical Phenomena Spectrum (functional analysis) Energy spectrum Cosmic ray Astrophysics Atomic and Molecular Physics and Optics Zenith
Zdroj:	Nuclear Physics B - Proceedings Supplements. 196:387-390
ISSN:	0920-5632
DOI:	10.1016/j.nuclphysbps.2009.09.073
Popis:	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 E 0 on N μ tr 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.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_________::44f093ee24f4d87438863230184f8a2d https://doi.org/10.1016/j.nuclphysbps.2009.09.073 Zobrazit plný text záznamu Full Text from ScienceDirect