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

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

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...

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Veröffentlicht in:arXiv.org 2015-07
Hauptverfasser: Galkin, V I, Anokhina, A M, Bakhromzod, R, Mukumov, A
Format: Artikel
Sprache:eng
Schlagworte:
Composition
Computer simulation
Cosmic rays
Interaction models
Primary cosmic rays
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Zusammenfassung: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.
ISSN:2331-8422