[1] Babcock H W. The possibility of compensating astronomical seeing[J]. Publications of the Astronomical Society of the Pacific, 1953, 65(386): 229–236.
[4] Van Noort M, Van Der Voort L R, L fdahl M G. Solar image restoration by use of multi-frame blind de-convolution with multiple objects and phase diversity[J]. Solar Physics, 2005, 228(1–2): 191–215.
[5] Ayers G R, Dainty J C. Iterative blind deconvolution method and its applications[J]. Optics Letters, 1988, 13(7): 547–549.
[6] Tian Y, Rao C H, Zhang X J. High frequency noise constraint in deconvolution from wavefront sensing[J]. High Power Laser and Particle Beams, 2007, 19(4): 593–597.
[7] Gonzalez R C, Woods R E. Digital image processing[M]. Reading, MA: Addison–Wesley, 1992.
[8] Kundur D, Hatzinakos D. Blind image deconvolution[J]. IEEE Signal Processing Magazine, 1996, 13(3): 43–64.
[9] Campisi P, Egiazarian K. Blind image deconvolution: theory and applications[M]. Boca Raton: CRC Press, 2016.
[10] Levin A, Weiss Y, Durand F, et al. Understanding and evaluating blind deconvolution algorithms[C]//Proceedings of 2009 IEEE Conference on Computer Vision and Pattern Recognition, 2009: 1964–1971.
[11] Perrone D, Favaro P. A clearer picture of total variation blind deconvolution[J]. IEEE Transactions on Pattern Analysis and Machine Intelligence, 2016, 38(6): 1041–1055.
[12] Levin A, Weiss Y, Durand F, et al. Efficient marginal likelihood optimization in blind deconvolution[C]//Proceedings of 2011 IEEE Conference on Computer Vision and Pattern Recognition, 2011: 2657–2664.
[13] Molina R, Mateos J, Katsaggelos A K. Blind deconvolution using a variational approach to parameter, image, and blur estimation[ J]. IEEE Transactions on Image Processing, 2006, 15(12): 3715–3727.
[14] Lofdahl M G. Multi–frame blind deconvolution with linear equality constraints[J]. Proceedings of SPIE, 2002, 4792: 146–155.
[15] Tian Y, Rao C H,Wei K. Adaptive optics image restoration based on frame selection and multi–frame blind deconvolution[J]. Chinese Astronomy and Astrophysics, 2009, 33(2): 223–230.
[16] Tian Y, Rao C H, Rao X J, et al. Hybrid deconvolution of adaptive optics retinal images from wavefront sensing[J]. Chinese Physics Letters, 2008, 25(1): 105–107.
[17] Li H, Lu J, Shi G H, et al. Deconvolution algorithm of retinal images[J]. Journal of Optoelectronics·Laser, 2010, 21(10): 1570–1573.
[18] Gonsalves R A. Phase retrieval and diversity in adaptive optics[ J]. Optical Engineering, 1982, 21(5): 829–832.
[19] Wang X, Zhao D Z, Mao H, et al. The development of phase diversity[J]. Optical Technique, 2009, 35(3): 454–460.
[20] L fdahl M G, Scharmer G B. Wavefront sensing and image restoration from focused and defocused solar images[J]. Astronomy and Astrophysics, 1994, 107: 243–264.
[21] Paxman R G, Schulz T J, Fienup J R. Phase–diverse speckle interferometry[C]// Topical Meeting on Signal Recovery and Synthesis IV, Technical Digest Series 11. Washington DC: Optical Society of America.
[22] Seldin J H, Paxman R G. Phase–diverse speckle reconstruction of solar data[J]. Proceedings of SPIE, 1994, 2302: 268–280.
[23] Paxman R G, Seldin J H, L fdahl M G, et al. Evaluation of phase–diversity techniques for solar–image restoration[J]. Astrophysical Journal, 1996, 466: 1087–1099.
[24] Vogel C R, Chan T F, Plemmons R J. Fast algorithms for phase–diversity–based blind deconvolution[J]. Proceedings of SPIE, 1998, 3353: 994 –1005.
[25] L fdahl M G, Scharmer G B. Diverse phase speckle inversion applied to data from the Swedish 1–meter solar telescope[J]. Proceedings of SPIE, 2003, 4853: 567–575.
[26] Kendrick R L, Acton D S, Duncan A L. Phase-diversity wave-front sensor for imaging systems[J]. Applied Optics, 1994, 33(27): 6533–6546.
[27] L fdahl M G, Kendrick R L, Harwit A, et al. Phase diversity experiment to measure piston misalignment on the segmented primary mirror of the Keck II telescope[J]. Proceedings of SPIE, 1998, 3356: 1190–1201.
[28] Yu X G, Liu Z, Jin Z Y, et al. Design of a phase diversity wavefront sensor[J]. Astronomical Research & Technology, 2010, 7(1): 55–59.
[29] Li F, Rao C H. Study on phase diversity wavefront sensor[J]. Acta Optica Sinica, 2011, 31(8): 0804001.
[30] Li F, Rao C H. Analysis and elimination of errors in phase diversity wavefront sensing system[J]. High Power Laser and Particle Beams, 2011, 23(3): 599–605.
[31] Li F, Rao C H. High resolution imaging technique based on phase diversity hybrid method[J]. Acta Physica Sinica, 2012, 61(2): 029502.
[32] Wang B, Wang Z Y, Wang J L, et al. Phase-diverse speckle imaging with two cameras[J]. Optics and Precision Engineering, 2011, 19(6): 1384–1390.
[33] Wang J L, Wang Z Y, Wang B, et al. Image restoration by phase–diverse speckle[J], Optics and Precision Engineering, 2011, 19(5): 1165–1170.
[34] Labeyrie A. Attainment of diffraction limited resolution in large telescopes by Fourier analysing speckle patterns in star images [J]. Astronomy and Astrophysics, 1970, 6: 85–87.
[35] Knox K T, Thompson B J. New methods of processing speckle pattern star images[J]. The Astrophysical Journal, 1973, 182: L133.
[36] Weigelt G, Wirnitzer B. Image reconstruction by the speckle– masking method[J]. Optics Letters, 1983, 8(7): 389–391.
[37] Weigelt G P. Modified astronomical speckle interferometry “speckle masking”[J]. Optics Communications, 1977, 21(1): 55–59.
[38] Von der Lühe O. Speckle imaging of solar small scale structure. I–Methods[J]. Astronomy and Astrophysics, 1993, 268(1): 374–390.
[39] Denker C, Mascarinas D, Xu Y, et al. High-spatial-resolution imaging combining high-order adaptive optics, frame selection, and speckle masking reconstruction[J]. Solar Physics, 2005, 227(2): 217–230.
[40] Denker C, Deng N, Rimmele T R, et al. Field-dependent adaptive optics correction derived with the spectral ratio technique[J]. Solar Physics, 2007, 241(2): 411–426.
[41] W ger F, von der Lühe O. Field dependent amplitude calibration of adaptive optics supported solar speckle imaging[J]. Applied Optics, 2007, 46(33): 8015–8026.
[42] Zhong L B, Tian Y, Rao C H. Influence of static aberrations on the accuracy of cross spectrum phase reconstruction and the compensated method[J]. Acta Optica Sinica, 2014, 34(7): 0701002.
[43] Zhong L B, Tian Y, Rao C H. Speckle image reconstruction of the adaptive optics solar images[J]. Optics Express, 2014, 22(23): 29249–29259.
[44] Zhong L B, Tian Y, Rao C H. Speckle transfer function for partial correction adaptive optics image reconstruction[J]. Optics Letters, 2014, 39(15): 4599–4602.
[45] Krishnan D, Bruna J, Fergus R. Blind deconvolution with nonlocal sparsity reweighting[J]. arXiv: 1311.4029, 2013.
[46] Yan R M, Shao L. Blind image blur estimation via deep learning [J]. IEEE Transactions on Image Processing, 2016, 25(4): 1910–1921.