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Design of the Simulation Scheme for SPHERE-3 Telescope for the \({10^{15}{-}10^{18}}\) eV Primary Cosmic Ray Studies Using Direct and Reflected Cherenkov Light from the Extensive Air Showers

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Abstract

Paper contains the first results on the development of a SPHERE-3 telescope for the primary cosmic ray studies in 1–1000 PeV energy range using reflected and direct Cherenkov light generated by extensive air showers. It also sheds some light on the development of our new approach to the design of the new telescope.

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Funding

The part of this work dedicated to the analysis of the SPHERE-2 experiment was supported by the Interdisciplinary Scientific and Educational School of Moscow University ‘‘Fundamental and Applied Space Research’’.

The work was supported by the Russian Science Foundation no. 23-72-00006, https://rscf.ru/project/23-72-00006/.

The research is carried out using the equipment of the shared research facilities of HPC computing resources at Lomonosov Moscow State University [23].

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Correspondence to E. A. Bonvech.

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Bonvech, E.A., Azra, C.J., Chernov, D.V. et al. Design of the Simulation Scheme for SPHERE-3 Telescope for the \({10^{15}{-}10^{18}}\) eV Primary Cosmic Ray Studies Using Direct and Reflected Cherenkov Light from the Extensive Air Showers. Phys. Atom. Nuclei 86, 1048–1055 (2023). https://doi.org/10.1134/S1063778824010149

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