Air Cherenkov Methods in Cosmic Rays: A Review and Some History
arXiv:astro-ph/0504269 · doi:10.1016/j.radphyschem.2005.12.019
Abstract
The history of application of the Cherenkov light emission in the atmosphere to cosmic ray and gamma-ray astronomy studies is briefly outlined with an emphasis on the pioneering activity of A.E. Chudakov. The present-day situation and some new ideas are also discussed.
11 pages, 5 figures, invited talk presented at the conference P.A. Cherenkov and Modern Physics (Moscow, June 22-25, 2004) commemorating P.A. Cherenkov centenary. Submitted for publication to Journal of Radiation Physics and Chemistry
References in corpus (4)
- The optical system of the H.E.S.S. imaging atmospheric Cherenkov telescopes, Part I: layout and components of the system
- The Technical Performance of the HEGRA System of Imaging Air Cherenkov Telescopes
- Development of an atmospheric Cherenkov imaging camera for the CANGAROO-III experiment
- The energy spectrum of cosmic rays above 10^15 eV as derived from air Cherenkov light measurements in Yakutsk
Cited by in corpus (5)
- Ultrahigh Energy Cosmic Rays
- Imaging Very High Energy Gamma-Ray Telescopes
- The Discovery of Cherenkov Radiation and its use in the detection of extensive air showers
- Ground-based gamma-ray astronomy: history and development of techniques
- Technological Novelties of Ground-Based Very High Energy Gamma-Ray Astrophysics with the Imaging Atmospheric Cherenkov Telescopes