How to deal with PCR composition problem at eV
arXiv:1507.03150
Abstract
Basic ideas of muon tracker technique for the solution of primary cosmic ray (PCR) composition problem in the energy range 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.
arXiv comment13 pages, 12 figures, 4 references