TUS/KLYPVE Space Telescopes Simulation of Performance

Details TUS/KLYPVE Space Telescopes Simulation of Performance TUS/KLYPVE Space Telescopes Simulation of Performance

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....2.1105g&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

We started to simulate the performance of the TUS/KLYPVE telescopes a space based UHECR detectors measuring the fluorescent and Cherenkov signals from EAS, developed in atmosphere. The optical part of the telescope consists of a segmented Fresnel mirror, fo cusing light to a grid of PMTs. We studied effects of various atmosphere profiles, parametrizations of the fluorescent light and the atmosphere attenuation models. The electronics and triggering system are simulated. The detector trigger efficiency is also studied as a function of the EAS energy and its arrival direction.

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