ИСТИНА |
Войти в систему Регистрация |
|
Интеллектуальная Система Тематического Исследования НАукометрических данных |
||
The EAS Cherenkov light array Tunka-133 with 3 km(2) area is taking data since 2009. In 2013-2014, scintillation stations for common operation with the Cherenkov light detectors are to be deployed. After a short description of the experiment and methods of EAS parameters reconstruction we present the all-particle energy spectrum in the energy range 10(15) - 10(18) eV and discuss possible astrophysical interpretations of the obtained results. The last part of the report is devoted to the future research based on the advantage of common work of Cherenkov light and scintillation detectors.