|
ИСТИНА |
Войти в систему Регистрация |
ИСТИНА ИНХС РАН |
||
Primary CR energy spectrum and mass composition by the data of Tunka-133 arrayдоклад на конференции
- Авторы: Калмыков Н.Н., TAIGA collaboration, Бережнев С.Ф., Карпов Н.И., Коростелева Е.Е., Кожин В.А., Кузьмичев Л.А., Лубсандоржиев Н.Б., Осипова Э.А., Панасюк М.И., Попова Е.Г., Свешникова Л.Г., Силаев А.А., (мл) Силаев А.А., Скурихин А.В., Просин В.В.
- Международная Конференция (Симпозиум) : 18th International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI 2014)
- Даты проведения конференции: 2014
- Дата доклада: 18 августа 2014
- Тип доклада: Стендовый
- Докладчик: не указан
- Место проведения: Geneva, Switzerland, Switzerland
-
Аннотация доклада:
The EAS Cherenkov light array Tunka-133 with ~3 km2 geometric area operates since 2009. Five winter seasons of data acquisition (~107 triggers) permitted us to reconstruct primary energy spectrum and mass composition in the energy range 6•1015 to 1018 eV. The further experiments in Tunka Valley will be: scintillation stations (Tunka-Grande), Tunka radio extension (Tunka-REX), Tunka-HiSCORE, Tunka-IACT. To start gamma-astronomy experiments in Tunka Valley researchers from a number of Russian and European Institutes arranged a Collaboration TAIGA (Tunka Advanced Instrument for cosmic ray and Gamma-Astronomy). The complex installation will consists of the net of wide-angle (1 sr. field of view) Cherenkov light optical stations (Tunka-HiSCORE ), several (~ 5) IACT telescopes based on spherical mirrors of 10 m2 area (Tunka-IACT) and muon scintillation detectors of the total area ~2000 m2.
- Добавил в систему: Кузьмичев Леонид Александрович