Paper
8 January 2008 The device for observing the solar on moon in multispectrum
Gang Huang, Qirong Xiao, Chao Zheng, Kaili Chu, Zhe Jin
Author Affiliations +
Abstract
In the thesis we introduce the basic design of the solar multi-spectrum telescope and imaging system. The whole system consists of Cassegrainian reflecting telescope, light-splitting system, light-filtering system, photo emissive detector group, calibration spectroscopy system and solar UV light source Simulated in order to image solar UV radiation, visible light and infrared band respectively and get video. The catadioptric parts of our system guarantee to image the three spectrums at the same time. There are turntable filter group before the detectors to achieve visible and ultraviolet band of more specific band imaging. Spectrophotometry system uses germanium spectroscope and spectrophotometry plane mirror to let the infrared and visible light through. And we coat spectroscope and spectrophotometry plane mirror UV-reflective film to achieve UV reflectance spectrophotometry. At last, we get real-time video image in three specific spectrums in a coaxial optical system. Since working in space for some time, the external factors will lead to our system to produce the spectrum of radiation drift. Therefore we add radiation calibration spectra to the system which provide a standard spectral radiation parameters to provide the detected result with a reliable reference data standard.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gang Huang, Qirong Xiao, Chao Zheng, Kaili Chu, and Zhe Jin "The device for observing the solar on moon in multispectrum", Proc. SPIE 6835, Infrared Materials, Devices, and Applications, 68350K (8 January 2008); https://doi.org/10.1117/12.758258
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KEYWORDS
Imaging systems

Visible radiation

Ultraviolet radiation

Mirrors

Infrared imaging

Sensors

Optical filters

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