Abstract <p>The scintillation experiment of the TAIGA astrophysical complex comprises two systems: Tunka-Grande and Taiga-Muon. The main objective of these systems is to study the energy spectrum and mass composition of cosmic rays in the energy range of <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="11450_2025_3560_Article_IEq1.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="71" /> </InlineMediaObject> <EquationSource Format="TEX">\(10^{15}{-}10^{18}\)</EquationSource> <!--NuclPhys2560049Kravchenko-m1--> </InlineEquation> eV, as well as to search for gamma radiation in the same energy range. An additional task of the experiments is to search for a signal from gamma quanta in the sub-PeV energy range in conjunction with wide angle Cherenkov detectors TAIGA-HiSCORE and Tunka-133. The report presents the objectives and status of the facility and a description of the design of scintillation counters and clusters. The results of the study of EAS with an unusual spatiotemporal structure are presented together with the results of a study of the joint operation of the Tunka-Grande and TAIGA-HiSCORE setups in order to search for sub-PeV gamma quanta. Estimates are made of the expected number of registered gamma quanta from the Crab Nebula.</p>

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Status of the Scintillation Experiment of the TAIGA Astrophysical Complex

  • E. A. Kravchenko,
  • I. I. Astapov,
  • P. A. Bezyazeekov,
  • E. A. Bonvech,
  • A. Blinov,
  • A. N. Borodin,
  • N. M. Budnev,
  • A. V. Bulan,
  • P. V. Busygin,
  • D. V. Chernov,
  • A. Chiavassa,
  • A. N. Dyachok,
  • V. A. Erofeeva,
  • A. R. Gafarov,
  • A. Yu. Garmash,
  • V. M. Grebenyuk,
  • E. O. Gress,
  • O. A. Gress,
  • T. I. Gress,
  • A. A. Grinyuk,
  • O. G. Grishin,
  • A. D. Ivanova,
  • A. L. Ivanova,
  • M. A. Iliushin,
  • I. A. Kabannik,
  • N. N. Kalmykov,
  • V. V. Kindin,
  • S. N. Kiryukhin,
  • N. I. Kolosov,
  • K. G. Kompaniets,
  • E. E. Korosteleva,
  • V. A. Kozhin,
  • A. P. Kryukov,
  • L. A. Kuzmichev,
  • A. A. Lagutin,
  • M. V. Lavrova,
  • Yu. E. Lemeshev,
  • B. K. Lubsandorzhiev,
  • N. Lubsandorzhiev,
  • A. Lukanov,
  • S. D. Malakhov,
  • R. R. Mirgazov,
  • R. D. Monkhoev,
  • E. A. Okuneva,
  • E. A. Osipova,
  • A. L. Pakhorukov,
  • L. V. Pankov,
  • A. Pan,
  • A. D. Panov,
  • A. A. Petrukhin,
  • D. A. Podgrudkov,
  • I. Poddubny,
  • V. A. Poleschuk,
  • E. G. Popova,
  • E. B. Postnikov,
  • V. V. Prosin,
  • A. A. Pushnin,
  • R. I. Raikin,
  • A. V. Razumov,
  • G. I. Rubtsov,
  • E. V. Ryabov,
  • V. S. Samoliga,
  • I. Satyshev,
  • A. A. Silaev,
  • A. A. Silaev,
  • A. Yu. Sidorenkov,
  • A. V. Skurikhin,
  • A. V. Sokolov,
  • L. G. Sveshnikova,
  • A. Shaikovsky,
  • M. V. Shulga,
  • V. A. Tabolenko,
  • L. G. Tkachev,
  • A. B. Tanaev,
  • M. Yu. Ternovoy,
  • N. A. Ushakov,
  • P. A. Volchugov,
  • N. V. Volkov,
  • D. M. Voronin,
  • V. Zirakashvili,
  • A. V. Zagorodnikov,
  • D. P. Zhurov,
  • I. I. Yashin

摘要

Abstract

The scintillation experiment of the TAIGA astrophysical complex comprises two systems: Tunka-Grande and Taiga-Muon. The main objective of these systems is to study the energy spectrum and mass composition of cosmic rays in the energy range of \(10^{15}{-}10^{18}\) eV, as well as to search for gamma radiation in the same energy range. An additional task of the experiments is to search for a signal from gamma quanta in the sub-PeV energy range in conjunction with wide angle Cherenkov detectors TAIGA-HiSCORE and Tunka-133. The report presents the objectives and status of the facility and a description of the design of scintillation counters and clusters. The results of the study of EAS with an unusual spatiotemporal structure are presented together with the results of a study of the joint operation of the Tunka-Grande and TAIGA-HiSCORE setups in order to search for sub-PeV gamma quanta. Estimates are made of the expected number of registered gamma quanta from the Crab Nebula.