Scholarlink

Abstract <p>The Horizon-T facility at the Tien Shan station of the Lebedev Physical Institute records extensive air showers (EAS) with energies above <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(10^{16}\)</EquationSource> <!--NuclPhys2660012Beysembaeva-m3--> </InlineEquation> eV, while the central detector group can study cosmic rays of lower energies: <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(10^{15}\leq E\leq 10^{16}\)</EquationSource> <!--NuclPhys2660012Beysembaeva-m4--> </InlineEquation> eV. In this paper, the time characteristics of experimental EAS events and those simulated using CORSIKA-77500 are compared. The authors conclude that the QGSJETII-04 hadronic interaction model and the EAS development scenarios used in CORSIKA in the energy range under consideration contradict the time properties of EAS registered by the Horizon-T central detectors.</p>

错误：搜索内容不能为空，请输入英文关键词
错误：关键词超出字数限制，请精简
高级检索

Time Structure of Extensive Air Showers with Energies \({10^{15}{-}10^{16}}\) eV Based on Horizon-T Facility Data at the Tien Shan High-mountain LPI Station

  • 期刊论文

  • 发表日期：

    2026年2月1日

查看全文
  • E. A. Beisembaeva,
  • A. M. Anokhina,
  • V. S. Aseikin,
  • K. A. Baygarin,
  • Y. V. Verminskaya,
  • M. I. Vildanova,
  • V. V. Zhukov,
  • V. A. Ryabov,
  • M. A. Samoilov,
  • T. Kh. Sadykov,
  • A. L. Shepetov

摘要

Abstract

The Horizon-T facility at the Tien Shan station of the Lebedev Physical Institute records extensive air showers (EAS) with energies above \(10^{16}\) eV, while the central detector group can study cosmic rays of lower energies: \(10^{15}\leq E\leq 10^{16}\) eV. In this paper, the time characteristics of experimental EAS events and those simulated using CORSIKA-77500 are compared. The authors conclude that the QGSJETII-04 hadronic interaction model and the EAS development scenarios used in CORSIKA in the energy range under consideration contradict the time properties of EAS registered by the Horizon-T central detectors.