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Abstract <p>Some plans on further development of the SPHERE experiment are presented. Namely, reasons for the introduction of an additional detector of the angular distribution of Cherenkov light, pointed at zenith, are given. It can only work together with the main telescope but can yield important information on the primary particle direction and mass. Construction and capabilities of the detector are discussed, draft algorithms for direction definition are revealed, and sensitivity to the primary mass is shown.</p>

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Estimation of Extensive Air Shower Primary Parameters Using Cherenkov Light Angular Distribution in the SPHERE-3 Experiment

  • 期刊论文

  • 发表日期：

    2025年6月1日

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  • E. A. Bonvech,
  • N. O. Ovcharenko,
  • O. V. Cherkesova,
  • E. L. Entina,
  • V. I. Galkin,
  • C. G. Azra,
  • D. V. Chernov,
  • V. A. Ivanov,
  • T. A. Kolodkin,
  • D. A. Podgrudkov,
  • T. M. Roganova,
  • M. D. Ziva

摘要

Abstract

Some plans on further development of the SPHERE experiment are presented. Namely, reasons for the introduction of an additional detector of the angular distribution of Cherenkov light, pointed at zenith, are given. It can only work together with the main telescope but can yield important information on the primary particle direction and mass. Construction and capabilities of the detector are discussed, draft algorithms for direction definition are revealed, and sensitivity to the primary mass is shown.