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This is a Quantitative Study study.

October 17, 2025Open Access

Estimation of the capabilities of the SPHERE-3 Cherenkov telescope for determining the parameters of the primary cosmic particle

ЕБЕ. А. БонвечLomonosov Moscow State University OCO. V. CherkesovaLomonosov Moscow State University ДЧД. В. ЧерновKrasnodar University of Ministry of Internal Affairs of Russia

Key Points

The SPHERE-3 Cherenkov telescope can accurately determine cosmic particle parameters through direct and reflected Cherenkov light.
Results indicate improved precision in measuring the energy and type of primary cosmic particles using Cherenkov light.
Modeling was based on the EAS Cherenkov light data from the Lomonosov-2 supercomputer's distribution dataset.
Accurate assessments of cosmic particle detection are critical for advancing astrophysics and cosmic research.

Abstract

New results of modeling the operation of the new SPHERE-3 Cherenkov telescope are presented. The telescope will be able to detect cosmic particles by direct and reflected Cherenkov light of the extensive air showers (EAS). Dual detection improves the accuracy of determining the parameters of the primary particle. The study is based on the data bank of distributions of the EAS Cherenkov light obtained on the Lomonosov-2 supercomputer. The accuracy of determining the energy and type of the primary particle from the reflected and direct flux of Cherenkov light is estimated.

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