The TUS Fresnel mirror production and optical parameters measurementстатья
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Дата последнего поиска статьи во внешних источниках: 14 августа 2017 г.
Аннотация:The TUS space experiment is aimed to study energy spectrum, composition and angular distribution of the Ultra High Energy Cosmic Ray (UHECR) at E ~ 10^20 eV. The TUS mission is planned for operation at the end of 2011 at the dedicated “Mikhail Lomonosov” satellite. The TUS detector will measure the fluorescence and Cherenkov light radiated by EAS of the UHECR using the optical system - Fresnel mirror-concentrator of 7 modules of ~2 m^2 area in total. A production of the flight model of the optical system is in progress. Status of the Fresnel mirror production, the method and results of its optical parameters measurement are presented.