What question did this study set out to answer?

To report on the development and performance of the SPHERE-3 Detector for studying cosmic rays.

April 3, 2026

Results of the Development of the SPHERE-3 Detector for Studying the PCR Mass Composition in the 1–1000 PeV Energy Range. The Status of 2025

DCD. V. ChernovLomonosov Moscow State University EBE. A. BonvechLomonosov Moscow State University OCO. V. CherkesovaLomonosov Moscow State University

Key Points

To report on the development and performance of the SPHERE-3 Detector for studying cosmic rays.
Developed a setup to register Cherenkov light from extensive air showers (EAS)
Implemented new measurement techniques for enhanced accuracy
Modelled detector performance and project status updates
Significant progress made in primary cosmic ray composition research
Current detector setup shows improved measurement capabilities
Projection of performance enhancements through 2025

Abstract

The SPHERE-3 setup is destined to register the EAS Cherenkov light (CL), both the direct and the reflected from the snow surface. A set of methods and new approaches in the measurement technique enable substantial progress in the study of the primary cosmic ray composition in the energy range 1–1000 PeV. The present work reveals the current status of the project development and detector performance modelling.

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Cite This Study

Chernov et al. (Mon,) studied this question.

synapsesocial.com/papers/69cf5e115a333a821460c370 https://doi.org/https://doi.org/10.1134/s1063778825602239

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