Autor:	Galkin, V. I., Anokhina, A. M., Bakhromzod, R., Mukumov, A.
Rok vydání:	2015
Předmět:	Astrophysics - High Energy Astrophysical Phenomena
Druh dokumentu:	Working Paper
Popis:	Basic ideas of muon tracker technique for the solution of primary cosmic ray (PCR) composition problem in the energy range $10^{17}-10^{18}$ eV are presented. The approach uses MC simulation data made with CORSIKA6.990 for "Pamir-XXI" site conditions. Similar technology can certainly be developed for other observation levels and interaction models. One can probably extend it to much higher primary energies. Comment: 13 pages, 12 figures, 4 references
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/1507.03150 Zobrazit plný text záznamu View this record from Arxiv