Response time structure of electrons and muons recorded by scintillation detectors in showers with energies higher than 5 × 1018 eV at the Yakutsk EAS array: The search for neutrinos
- Авторы: Knurenko S.P.1, Egorov Y.A.1, Petrov Z.E.1, Petrov I.S.1, Sleptsov I.Y.1
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Учреждения:
- Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
- Выпуск: Том 81, № 4 (2017)
- Страницы: 474-477
- Раздел: Proceedings of the 34th National Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/185046
- DOI: https://doi.org/10.3103/S1062873817040268
- ID: 185046
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Аннотация
The procedure for and results from a search for showers generated by such neutral particles as high energy gamma rays and astroneutrinos are presented. A comprehensive analysis of data on electrons, muons, and EAS Cherenkov light, and their response time in scintillation and Cherenkov detectors, is performed.
Об авторах
S. Knurenko
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.sbras.ru
Россия, Yakutsk, 677980
Yu. Egorov
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.sbras.ru
Россия, Yakutsk, 677980
Z. Petrov
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.sbras.ru
Россия, Yakutsk, 677980
I. Petrov
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Автор, ответственный за переписку.
Email: igor.petrov@ikfia.sbras.ru
Россия, Yakutsk, 677980
I. Sleptsov
Shafer Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: igor.petrov@ikfia.sbras.ru
Россия, Yakutsk, 677980
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