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Telescope Array Project : ウィキペディア英語版
Telescope Array Project


The Telescope Array project is an international collaboration involving research and educational institutions in Japan, The United States, Russia, South Korea, and Belgium. The experiment is designed to observe air showers induced by ultra-high-energy cosmic ray using a combination of ground array and air-fluorescence techniques. It is located in the high desert in Millard County, Utah (USA) at about above sea level.
==Overview==

The Telescope Array observatory is a hybrid detector system consisting of both an array of 507 scintillation surface detectors (SD) which measure the distribution of charged particles at the Earth's surface, and three fluorescence stations which observe the night sky above the SD array.〔T. AbuZayyad et al., "(The surface detector array of the Telescope Array experiment )" Nuclear Instruments and Methods in Physics Research Section A: (2012) vol. 689〕 Each fluorescence station is also accompanied by a LIDAR system for atmospheric monitoring.〔M. Chikawa et al., Proceedings of 29th ICRC (2005) 137〕 The SD array is much like that of the AGASA group, but covers an area that is nine times larger. The hybrid setup of the Telescope Array project allows for simultaneous observation of both the longitudinal development and the lateral distribution of the air showers. When a cosmic ray passes through the earth's atmosphere and triggers an air shower, the fluorescence telescopes measure the scintillation light generated as the shower passes through the gas of the atmosphere, while the array of scintillator surface detectors samples the footprint of the shower when it reaches the Earth's surface.
At the center of the ground array is the Central Laser Facility which is used for atmospheric monitoring and calibrations.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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