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Contribution Poster
R&D of the Fresnel optical system for the TUS space detector
Speakers
- Dr. LEONID TKACHEV
Primary authors
- Dr. LEONID TKACHEV (JOINT INSTITUTE FOR NUCLEAR RESEARCH, Dubna)
Co-authors
- G. GARIPOV (D.V. Skobeltsyn Institute of Nuclear Physics of Moscow State University, Moscow, Russia)
- A. GONGADZE (Joint Institute for Nuclear Research, Dubna, Moscow region, Russia)
- A. GRINYUK (Joint Institute for Nuclear Research, Dubna, Moscow region, Russia)
- B. KHRENOV (D.V. Skobeltsyn Institute of Nuclear Physics of Moscow State University, Moscow, Russia)
- O. KLIMOV (Joint Institute for Nuclear Research, Dubna, Moscow region, Russia)
- D. NAUMOV (Joint Institute for Nuclear Research, Dubna, Moscow region, Russia)
- A. PUCHKOV (Rocket Space Corporation "Energia", Consortium "Space Regatta, Korolev, Moscow region, Russia.)
- B. SABIROV (Joint Institute for Nuclear Research, Dubna, Moscow region, Russia)
- O. SAPRYKIN (Rocket Space Corporation "Energia", Consortium "Space Regatta, Korolev, Moscow region, Russia.)
- I. YASHIN (D.V. Skobeltsyn Institute of Nuclear Physics of Moscow State University, Moscow, Russia)
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Abstract content
The space TUS detector of UV fluorescence light radiated by EAS of Ultra High Energy Cosmic Rays (UHECR) is under preparation. The TUS optical system will consist of the Fresnel mirror-concentrator of ~2 sq. m. and 256 PMT pixels as the photo receiver at the mirror focal surface. The 2 PMT pixel prototypes were tested and used for data taken at the “Universitetsky-Tatiana” and Compass-2 satellites. The R&D study of the Fresnel mirror production is presented.
If this papers is presented for a collaboration, please specify the collaboration
TUS collaboration
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 5 (HE part 2), pages 881-884