Journal of Atmospheric and Environmental Optics, Volume. 13, Issue 3, 178(2018)

Influence of Signal to Noise Ratio on Atmospheric Coherence Length Measured by DIMM

Yang SHA1,2, Xu JING1、*, Yi WU1, and Zaihong HOU1
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  • 1[in Chinese]
  • 2[in Chinese]
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    References(9)

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    [5] [5] Tan Huisong, Cen Xuefen, Qian Tonglin. The factors influencing the seeing measurement by the DIMM[J].Publication of Yunnan Observator, 2002, 1: 38-4(in Chinese).

    [6] [6] SarazinM, Roddier F. The ESO differential image motion monitor[J].Astronomy and Astrophysics, 1990, 227: 294-300.

    [7] [7] MaX Y, Rao C H, Zheng H Q. Error analysis of CCD-based point source centroid computation under the background light[J].Optics Express, 2009, 17(10): 8525-8541.

    [8] [8] Lu Qianian, Hou Zaihong, Jing Xu,et al. Influence of sky background on data of day-night atmospheric coherence length monitor[J]. Laser & Infrared, 2012, 42(8): 921-924.

    [9] [9] Tokovinin A. From differential image motion to seeing[J].Publications of the Astronomical Society of the Pacific, 2002, 114: 1156-1166.

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    SHA Yang, JING Xu, WU Yi, HOU Zaihong. Influence of Signal to Noise Ratio on Atmospheric Coherence Length Measured by DIMM[J]. Journal of Atmospheric and Environmental Optics, 2018, 13(3): 178

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    Paper Information

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    Received: Jan. 5, 2017

    Accepted: --

    Published Online: Jun. 1, 2018

    The Author Email: Xu JING (xujing@aiofm.ac.cn)

    DOI:10.3969/j.issn.1673-6141.2018.03.003

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