ИСТИНА |
Войти в систему Регистрация |
|
ФНКЦ РР |
||
The EAS Cherenkov light array Tunka-133, with ∼ 3 km2 geometric area, is taking date since 2009.The array permits a detailed study of energy spectrum and mass composition of cosmic rays in the energy range from 6 · 1015 to 1018 eV. We describe the methods of time and amplitude calibration of the array, methods of EAS parameter reconstruction and present the all-particle energy spectrum, based on 7 seasons of operation.