$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 de...

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Bibliographische Detailangaben
Hauptverfasser:	Galkin, V. I, Anokhina, A. M, Bakhromzod, R, Mukumov, A
Format:	Artikel
Sprache:	eng
Schlagworte:	Physics - High Energy Astrophysical Phenomena
Online-Zugang:	Volltext bestellen
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Beschreibung
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.
DOI:	10.48550/arxiv.1507.03150