[1] Rao Ruizhong.Light Propagation in the Atmospheric Turbulence[M]. Hefei: Anhui Science and Technology Press, 2005(in Chinese).
[2] Fried D L. Statistics of a geometric representation of wavefront distortion[J].Journal of the Optical Society of America, 1965, 55(11): 1427-1435.
[3] Liu Zhong, Qian Yaohui, Qian Ping. Two problems on the principle of the measurement of seeing by using the differential image motion method[J].Publication of Yunnan Observator, 1993, 2: 54-60(in Chinese).
[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] SarazinM, Roddier F. The ESO differential image motion monitor[J].Astronomy and Astrophysics, 1990, 227: 294-300.
[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] 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] Tokovinin A. From differential image motion to seeing[J].Publications of the Astronomical Society of the Pacific, 2002, 114: 1156-1166.