A way of observing Cherenkov light at the Yakutsk EAS array
- Авторлар: Timofeev L.V.1, Ivanov A.A.1
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Мекемелер:
- Shafer Institute of Cosmophysical Research and Aeronomy
- Шығарылым: Том 81, № 4 (2017)
- Беттер: 471-473
- Бөлім: Proceedings of the 34th National Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/185045
- DOI: https://doi.org/10.3103/S1062873817040402
- ID: 185045
Дәйексөз келтіру
Аннотация
A way of observing the Cherenkov light from extensive air showers (EAS) generated by cosmic rays (CRs) with energies above 1016 eV is presented, along with preliminary results from observations. The detector is a wide-angle Cherenkov telescope working in coincidence with scintillation detectors and the integral and differential Cherenkov detectors of the Yakutsk EAS array. The detector is positioned about 2 m away from one of the integral Cherenkov detectors.
Авторлар туралы
L. Timofeev
Shafer Institute of Cosmophysical Research and Aeronomy
Хат алмасуға жауапты Автор.
Email: timofeevlev@ikfia.sbras.ru
Ресей, Siberian Branch, Yakutsk, 677980
A. Ivanov
Shafer Institute of Cosmophysical Research and Aeronomy
Email: timofeevlev@ikfia.sbras.ru
Ресей, Siberian Branch, Yakutsk, 677980
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