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Status of the Tunka Advanced Instrument for Cosmic Ray Physics and Gamma Astronomy (TAIGA)статья
- Авторы: Kalmykov N., Korosteleva E., Kozhin V., Kuzmichev L., Lubsandorzhiev N., Osipova Eleonora A., Panasyuk M., Popova Elena G., Postnikov E., Prosin V., Silaev A.A., Silaev Alexey A., Skurikhin A., Sveshnikova L.G., TAIGA collaboration
- Сборник: Proceedings of 2016 International Conference on Ultra-High Energy Cosmic Rays (UHECR2016)
- Серия: JPS Conference Proceedings
- Том: 19
- Год издания: 2018
- Место издания: Journal of the Physical Society of Japan
- Первая страница: 011027
- DOI: 10.7566/jpscp.19.011027
- Аннотация: The new TAIGA project is proposed to solve a number of fundamental problems of high- energy gamma astronomy, cosmic-ray and particle physics. The array will be located in the Tunka valley at the site of the Tunka-133 array. TAIGA will consist of wide-angle (FOV ~ 0.6 sr) non-imaging Cherenkov optical detectors (TAIGA-HiSCORE) covering an area of up to 5 km2, and up to 16 IACTs (Imaging Atmospheric Cherenkov Telescopes) (FOV ~ 10 × 10°) based on ~9 m2 mirrors and muon detectors with a total sensitive area of 2000 m2. The current TAIGA status is presented.
- Добавил в систему: Постников Евгений Борисович