Отправить статью по E-mail A way of observing Cherenkov light at the Yakutsk EAS array
- Авторы: Timofeev L.V.1, Ivanov A.A.1
-
Учреждения:
- Shafer Institute of Cosmophysical Research and Aeronomy
- Выпуск: Том 81, № 4 (2017)
- Страницы: 471-473
- Раздел: 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
Цитировать
Открытый доступ
Доступ предоставлен
Только для подписчиков
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.
Об авторах
L. Timofeev
Shafer Institute of Cosmophysical Research and Aeronomy
Автор, ответственный за переписку.
Email: timofeevlev@ikfia.sbras.ru
Россия, Siberian Branch, Yakutsk, 677980
A. Ivanov
Shafer Institute of Cosmophysical Research and Aeronomy
Email: timofeevlev@ikfia.sbras.ru
Россия, Siberian Branch, Yakutsk, 677980
Дополнительные файлы
