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Cosmic Research, Vol. 42, No. 5, 2004, pp. 489­534. Translated from Kosmicheskie Issledovaniya, Vol. 42, No. 5, 2004, pp. 509­554. Original Russian Text Copyright © 2004 by Panasyuk, Kuznetsov, Lazutin, Avdyushi, Alexeev, Ammosov, Antonova, Baishev, Belenkaya, Beletsky, Belov, Benghin, Bobrovnikov, Bondarenko, Boyarchuk, Veselovsky, Vyushkova, Gavrilieva, Gaidash, Ginzburg, Denisov, Dmitriev, Zherebtsov, Zeleny, Ivanov-Kholodny, Kalegaev, Kanonidi, Kleimenova, Kozyreva, Kolomiitsev, Krasheninnikov,

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• http://www.kosmofizika.ru/buri/vesel2.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....

387. XX конференция Ломоносов (9-12 апреля 2013г.)

388. XX конференция Ломоносов (9-12 апреля 2013г.)

389. http://oc.cs.msu.su/smirnov/PPP/beameruserguide.pdf