Acta Photonica Sinica, Volume. 46, Issue 3, 311004(2017)

The Design and Implementation of CCD Refrigeration System of Imaging Spectrometer

ZHANG Quan1,2、*, HUANG Shu-hua1, ZHAO Xin1, SI Fu-qi1, ZHOU Hai-jin1, WANG Yu1, and LIU Wen-qing1
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  • 2[in Chinese]
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    To decrease CCD dark current noise and improve the signal to noise ratio in airborne ultraviolet imaging spectrograph, CCD working temperature should be decreased as CCD is temperature sensitive device. So CCD cooling circuit was designed by adoping analog PID algorithm, and its parameters were determined by Ziegler-Nicholas method. The max cooling rate is less than 5℃/min and its temperature stability is about ±0.05℃, satisfing the requirements of maximum cooling temperature difference.The cooling circuit has been tested on airborne system. The experimental results show that change of temeperature could not affect the cooling results. And after reaching the target refrigeration temperature of -20℃, dark background noise of spectral dimension CCD detector is 1 702 on average and dark signal response non-uniform decreases to 0.5%. The results meet the requirements of spectral data.

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    ZHANG Quan, HUANG Shu-hua, ZHAO Xin, SI Fu-qi, ZHOU Hai-jin, WANG Yu, LIU Wen-qing. The Design and Implementation of CCD Refrigeration System of Imaging Spectrometer[J]. Acta Photonica Sinica, 2017, 46(3): 311004

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    Paper Information

    Received: Aug. 3, 2016

    Accepted: --

    Published Online: Apr. 10, 2017

    The Author Email: Quan ZHANG (qzhang@aiofm.cas.cn)

    DOI:10.3788/gzxb20174603.0311004

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