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1. http://cosrad.sinp.msu.ru/experiments/tus/doc/HO2COSPAR2006.pdf
... The data on UV glow of the atmosphere obtained in operation of one pixel of the TUS detector on board the Moscow State University "Universitetsky-Tatiana" satellite was taken into account in design of the updated TUS detector. ... The main feature of the design is use of MEMS technology scanning mirror controlled by the TUS computer, analyzing the recorded EAS data and directing the laser to the atmosphere spot, where back scattered Cherenkov light came from. ... Monitoring of UV intensity on-route....
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Ссылки http://cosrad.sinp.msu.ru/experiments/tus/doc/HO2COSPAR2006.pdf -- 237.2 Кб -- 19.03.2008
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2. http://cosrad.sinp.msu.ru/experiments/tus/doc/Ponce2007fin.pdf
... For full UV energy Euv (erg) radiated in TLE the corresponding number of photons of wavelength =300-400 nm (with average energy 3.5 eV) is: Nph=Euv/3.5в1.6 10-12 (1) We considered 2 options of the pinhole camera focal distance: 1. focal distance is short so that the circle of diameter 40 km is observed by one pixel and 2. focal distance is long so that the 40 km circle is observed in many camera pixels. ... Full energy released in UV in the atmosphere is determined by the pixel signal. ...
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Ссылки http://cosrad.sinp.msu.ru/experiments/tus/doc/Ponce2007fin.pdf -- 115.3 Кб -- 19.03.2008
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3. http://cosrad.sinp.msu.ru/experiments/tus/doc/global2007.pdf
30 TH I NT E R N AT I ON AL C OSMIC R AY C O N F ER EN C E Search for global asymmetry of UHECR arrival directions with the TUS space detector P. K LI M OV 1 ,O. K AL ASHE V 2 , B . ... Introduction Space-based ultra-high-energy cosmic-ray detectors such as TUS or JEM/EUSO are best suited for searches of the global anisotropies in the distribution of arrival directions of cosmic-ray particles because they provide full-sky coverage with a single experiment. ... Phys. 12, 25 (1999). ... Phys. Lett. ...
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Ссылки http://cosrad.sinp.msu.ru/experiments/tus/doc/global2007.pdf -- 136.8 Кб -- 19.03.2008
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