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Telescope Array Project



Millard,


Utah,United-states - 84624

Detailed description is 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 1400m above sea level.OverviewThe Telescope Array observatory is a hybrid detector system consisting of both an array of 507 scintillation surface detectors 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.
Each fluorescence station is also accompanied by a LIDAR system for atmospheric monitoring.
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.Surface detectorThe surface detectors that make up the ground array are activated when ionizing particles from an extensive air shower pass through them.
When these particles pass through the plastic scintillator within the detector, it induces photo electrons which are then gathered by wavelength-shifting fibers and sent to a photomultiplier tube.
The electronic components within the detectors then filter the results, giving the detectors comparable accuracy to the AGASA experiment.


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Ans: Latitude of the location is 39.296944444444 Longtitude of the location is - -112.90861111111

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