http://arxiv.org/abs/1507.03150
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.
V. Galkin, A. Anokhina, R. Bakhromzod, et. al.
Tue, 14 Jul 15
38/64
Comments: 13 pages, 12 figures, 4 references