Enviar artigo por via de e-mail A way of observing Cherenkov light at the Yakutsk EAS array
- Autores: Timofeev L.V.1, Ivanov A.A.1
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Afiliações:
- Shafer Institute of Cosmophysical Research and Aeronomy
- Edição: Volume 81, Nº 4 (2017)
- Páginas: 471-473
- Seção: 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
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Resumo
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.
Sobre autores
L. Timofeev
Shafer Institute of Cosmophysical Research and Aeronomy
Autor responsável pela correspondência
Email: timofeevlev@ikfia.sbras.ru
Rússia, Siberian Branch, Yakutsk, 677980
A. Ivanov
Shafer Institute of Cosmophysical Research and Aeronomy
Email: timofeevlev@ikfia.sbras.ru
Rússia, Siberian Branch, Yakutsk, 677980
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