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arXiv · 1507.03150

How to deal with PCR composition problem at $E_0 \gtrsim 10^{17}$ eV

V. I. Galkin·A. M. Anokhina·R. Bakhromzod·A. Mukumov
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Abstract

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.

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V. I. Galkin, A. M. Anokhina, R. Bakhromzod, A. Mukumov. 2015-07-11. How to deal with PCR composition problem at $E_0 \gtrsim 10^{17}$ eV. https://arxiv.org/abs/1507.03150

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