[1] Hou W L, Lee Z, Weidemann A D. Why does the Secchi disk disappear An imaging perspective［J］. Opt. Express., 2007, 15(6): 2791-2802.

[2] Hou W L, Gray D J, Weigemann A D, et al. Automated underwater image restoration and retrieval of related optical properties［C］. IEEE International Geosciences and Remote Sensing Symposium. IGARSS, 2007: 1889-1892.

[3] Wells W H. Theory of small angle scattering［R］. AGARD Lec. Series No. 61. NATO, 1973.

[4] Fan F, Yang K, Xia M, et al. Underwater image restoration by means of blind deconvolution approach［J］. Front. Optoelectron. China., 2010, 3(2): 169-178.

[5] 范泛, 杨克成, 夏珉, 等. 盲反卷积方法在水下激光图像复原中的应用［J］. 光学与光电技术, 2010, 8(3): 13-17.

[6] Fan F, Yang K, Xia M, et al. Comparative study on several blind deconvolution algorithms applied to underwater image restoration［J］. Opt. Review., 2010, 17(3): 123-129.

[7] Fish D A, Brinicombe A M, Pike E R, et al. Blind deconvolution by means of the Richardson-Lucy algorithm［J］. J. Opt. Soc. Am. A., 1995, 12: 58-65.

[8] Richardson W H. Bayesian-based iterative method of image restoration［J］. Journal of the Optical Society of America, 1972, 62(1): 55-59.

[9] Lcuy L B. An iterative technique for the rectification of observed distributions［J］. Astron. J., 1974, 79(6): 745-754.

[10] Vio R, Bardsley J, Wamsteker W. Least-squares methods with Poissonian noise: Analysis and comparison with the Richardson-Lucy algorithm［J］. Astronomy & Astrophysics, 2005, 435: 741-755.

[11] Lanteri H, Soummer R, Aime C. Comparison between ISRA and RLA algorithms. Use of a Wiener Filter based stopping criterion［J］. Astronomy & Astrophysics Supplement Series, 1999, 140(5): 235-246.

[12] Zhang J, Zhang Q, He G. Blind deconvolution: multiplicative iterative algorithm［J］. Optics Letters, 2008, 33(1): 25-27.

[13] Marziliano P, Dufaux F, Winkler S, et al. Perceptual blur and ringing metrics: application to JPEG2000［J］. Signal Processing: Image Communication, 2004, 19(6): 163-172.