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Tunka-133: result of 5 year observation and future experiments - HiSCORE, Grande, IACTдоклад на конференции
- Авторы: Бережнев С.Ф., TAIGA collaboration, Калмыков Н.Н., 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.
- Конференция : RICAP 2014
- Даты проведения конференции: 2014
- Тип доклада: не указан
- Докладчик: не указан
- Место проведения: Noto, Sicily, Italy, 30 Sept. – 3 Oct. 2014, Italy
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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. 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