PoS - Proceedings of Science
Volume 444 - 38th International Cosmic Ray Conference (ICRC2023) - Solar & Heliospheric Physics (SH)
Preliminary Simulation of the Scibar Cosmic Ray Telescope (SciCRT) at Sierra Negra
F. Monterde Andrade*, L.X. González, J.F. Valdés Galicia, J. Newton-Bosch, O.G. Morales Olivares, Y. Matsubara, Y. Itow, T. Sako, T. Kawabata, E. Ortiz, A. Hurtado, O. Musalem, R. Taylor, K. Munakata, C. Kato, W. Kihara, Y. Ko, S. Shibata, H. Takamaru, A. Oshima, T. Koi, H. Kojima, H. Tsuchiya, K. Watanabe, M. Kozai and Y. Nakamuraet al. (click to show)
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Pre-published on: July 25, 2023
Published on: —
Abstract
The Scibar Cosmic-Ray Telescope (SciCRT) is a brand new detector of the Sierra Negra Cosmic
Rays Observatory (SN-CRO). It is designed to observe solar neutrons and the muon background
produced by galactic cosmic rays. In this work we present a Geant4-based simulation of the muon
detection efficiency of the SciCRT; for this purpose we injected 10$^{5}$ muons, in an energy range
from 100 to 1000 MeV, impinging the SciCRT array. Our results provide new information about
the SciCRT performance and may be used to study variations in low energy galactic cosmic rays.
DOI: https://doi.org/10.22323/1.444.1273
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