[1] [1] Mao Wei, Ji Kaifan, Li Binhua et al.. Celestial Measuring Based on CCD ［M］. Kunming: Yunnan Technology Press, 2003. 60～75

[2] [2] Ding Xiaohua, Li You, Yu Qifeng et al.. CCD noise calibration and its application in edge location［J］. Acta Optica Sinica, 2008, 28(1): 99～104

[3] [3] J. Arines, J. Ares. Minimum variance centroid thresholding ［J］. Opt. Lett., 2002, 27(7): 497～499

[4] [4] Li Zhan, Peng Qingyu, Han guoqiang. Comparison of digital centering algorithms based on CCD images ［J］. Acta Astronomica Sinca, 2009, 50(3): 340～348

[5] [5] Hu Keliang. Research on the Application of Guide System with Area CCD Camera and Embedded System in High Temporal and Spatial Resolution Observation of Solar Magnetic Field ［D］. Beijing: Graduate University of Chinese Academy of Sciences, 2004

[6] [6] B. H. Tatarskii. Wave Propagation in a Turbulent Mdium［M］. Wen Jingsong, Song Zhengfang, Zeng Zongyong et al. Transl.. Beijing: Science Press, 1978

[7] [7] M. C. Roggemann, B. Welsh. Imaging Through Turbulence［M］. Boca Raton, FL: CRC Press, 1996

[8] [8] F. Roddier. The Effects of Atmospheric Turbulence in Optical Astronomy［M］. E. Wolf, ed., Progress in Optics XIX, 1981

[9] [9] J. W. Goodman. Statistical Optics ［M］. New York: Wiley Classics Library Edition, 2000. 361～457

[10] [10] D. L. Fried. Statistics of a geometric representation of wave-front distortion [J]. J. Opt. Soc. Am., 1965, 55(11): 1427～1435

[11] [11] Liu Zhong, Dai Yichun, Jin Zhenyu et al.. The centroid of speckle image and the wavefront tilt［J］. Astronomical Reseanch & TechonolgyPulications of National Astronomical Observatories of China, 2009, 6(2): 119～124

[12] [12] M. A. Kallistratova, A. I. Kon. Fluctuations in the angle of arrival of light waves from an extended source in a turbulent atmosphere［J］. Radiophysics and Quantum Electronics, 1966, 9(6): 636～639

[13] [13] L. C. Andress, R. L. Phillips. Laser Beam Propagation Through Random Media［M］. Bellingham: SPIE Press, 2005. 492～493

[14] [14] G. B. Scharmer, T. I. M. VanWerkhoven. S-DIMM+ height characterization of day-time seeing using solar granulation［J］. Astron. & Astrojphys., 2010, 513(A25): 1～12

[15] [15] M. Sarazin, F. Roddier. The ESO differential image motion monitor ［J］. Astron. & Astrophys., 1990, 227(1): 294～300

[16] [16] J. M. Beckers. Increasing the size of the isoplanatic patch with multi-conjugate adaptive optics［C］. ESO Conference and Workshop Proceedings, 1988. 693～703

[17] [17] Chang Xiang, Li Rongwang, Xiong Yaoheng. Predicted space-varying point spread function model for anisoplanatic adaptive optics imaging［J］. Acta Optica Sinica, 2011, 31(12): 1201001

[18] [18] Liu Yunqing, Jiang Huilin, Tong Shoufeng. Study on stabilizational racking technology for atmospheric laser communication system［J］. Chinese J. Lasers, 2011, 38(5): 0505005

[19] [19] Chen Jingyuan. Geometric anisoplanatism of adaptive optics system［J］. Acta Optica Sinica, 2010, 30(4): 922～927

[20] [20] M. Warner, V. Riot, J. Sebag. LSST telescope guider loop requirements analysis and predicted performance ［C］. SPIE, 2010, 7738: 77381U

[21] [21] Li Rongwang, Chang Xiang, Xiong Yaoheng. Numerical simulation of wander of ranging laser beam［J］. Acta Optica Sinica, 2011, 31(11): 1101001

[22] [22] A. J. Jankevics, A. Wirth. Wide field of view adaptive optics［C］. SPIE, 1991, 1534: 438～448

[23] [23] E. P. Waliner. Optimizing the locations of multiconjugate wavefront correctors［C］. SPIE, 1994, 2201: 110～116

[24] [24] R. J. Noll. Zernike polynomials and atmospheric turbulence［J］. J. Opt. Soc. Am., 1976, 66(3): 207～211

[25] [25] N. Roddier. Atmospheric wavefront simulation and Zernike polynomials［C］. SPIE, 1990, 1237: 670～678

[26] [26] B. M. Welsh, C. Dainty. Fourier series based atmospheric phase screen generator for simulating anisoplantic geometries and temporalevolution［C］ . SPIE, 1997, 3125: 327～338

[27] [27] R. G. Lane, A. Glindemann, J. Dainty. Simulation of Kolmogorov phase screen［J］. Waves in Random Media, 1992, 2(3): 209～224