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Photo receiver of the orbital ultra high energy cosmic rays detector TUS

机译:轨道超高能宇宙射线探测器TUS的光电接收器

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The TUS space experiment is aimed to study energy spectrum, composition and angular distribut distribution of the Ultra High ion Ene Energy Cosmic Ray (UHECR) at E rgy ~ 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 r ra- adiated by EAS o diated of the UHECR using the optical system f - Fresnel mirror mirror-concentrator of 7 modules of ~2 m 2 area in total. A production of the flight model of the photo receiver is in progress. Status of the photo receiver production and tests are presented.
机译:TUS空间实验旨在研究E rgy〜10 20 eV时超高能离子能宇宙射线(UHECR)的能谱,组成和角度分布。 TUS任务计划于2011年底在专用的“米哈伊尔·罗蒙诺索夫”卫星上运行。 TUS检测器将使用光学系统f-菲涅耳镜反射镜集中器,共7个模块,总面积约2 m 2,测量UHECR对EAS辐射的荧光和Cherenkov光。光接收器的飞行模型的制作正在进行中。介绍了光接收器生产和测试的状态。

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