[1] JIANG Wenhan. Adaptive optics technology[J]. Chinese Journal of Nature, 28, 7(2006).

[2] SALTER P S, BOOTH M J. Adaptive optics in laser processing[J]. Light-Science & Applications, 8, 16(2019).

[3] SUN L C, GUO Y D, SHAO C F et al. 10.8 kW, 2.6 times diffraction limited laser based on a continuous wave Nd∶YAG oscillator and an extra-cavity adaptive optics system[J]. Optics Letters, 43, 4160-4163(2018).

[4] AZIMIPOUR M, JONNAL R S, WERNER J S et al. Coextensive synchronized SLO-OCT with adaptive optics for human retinal imaging[J]. Optics Letters, 44, 4219-4222(2019).

[5] LI C H, XIAN H, JIANG W H et al. Performance analysis of field-of-view shifted Shack–Hartmann wavefront sensor based on splitter[J]. Applied Physics B, 88, 367-372(2007).

[6] LI C H, XIAN H, JIANG W H et al. Analysis of wavefront measuring method for daytime adaptive optics[J]. Acta Physica Sinica, 56, 4289-4296(2007).

[7] LI C H, XIAN H, RAO C et al. Field-of-view shifted Shack-Hartmann wavefront sensor for daytime adaptive optics system[J]. Optics Letters, 31, 2821-2823(2006).

[8] LI Chaohong. Research on performance of Hartmann wavefront sensor based on field shift in daytime conditions[D](2007).

[9] GONGLEWSKI J D, HIGHLAND R G, DAYTON D C et al. ADONIS: daylight imaging through atmospheric turbulence[C], 2827, 152-161(1996).

[10] ZHU M, SHEN X H, WU C. Study of star image detecting technology in daytime strong background[C], 1, 745-748(2004).

[11] LI Z Q, LI X Y. Centroid computation for Shack-Hartmann wavefront sensor in extreme situations based on artificial neural networks[J]. Optics Express, 26, 31675-31692(2018).

[12] LIU Yu. Infrared image background estimation based on adaptive surface fitting[J]. Science and Technology Innovation Review, 38-40(2012).

[13] LI Kun, LI Hui, LIU Yunjie et al. B-spline surface fitting background suppression of LCD Mura defects[J]. Opto-electronic Engineering, 41, 33-39(2014).

[14] GAO Yang, LI Yanjun, ZHANG Ke. Surface fitting segmentation of infrared image under heterogeneous background[J]. Opto-electronic Engineering, 33, 83-87(2006).

[15] LIFTON J J, LIU T, MCBRIDE J. Non-linear least squares fitting of Bézier surfaces to unstructured point clouds[J]. AIMS Mathematics, 6, 3142-3159(2021).

[16] WAHAB A F, ZULKIFLY M I E. 3-Tuple Bézier surface interpolation model for data visualization[J]. IAENG International Journal of Applied Mathematics, 50, 1-7(2020).

[17] SONG Tao, QI Jihui, HOU Peiguo et al. Geometric optimization method of projection image based on Bezier surface[J]. Journal of Yanshan University, 45, 449-455(2021).

[18] LI Xuxu. Research on sub-spot location Algorithm of point source target Hartmann sensor with low signal-to-noise ratio[D](2018).

[19] BAKER K L, MOALLEM M M. Iteratively weighted centroiding for Shack-Hartmann wave-front sensors[J]. Optics Express, 15, 5147-5159(2007).

[20] FEST E C[M]. Stray light analysis and control(2013).

[21] FORTES M A, MEDINA E. Fitting missing data by means of adaptive meshes of Bézier curves[J]. Mathematics and Computers in Simulation, 191, 33-48(2022).

[22] ZHU Xinxiong[M]. Free curve and surface modeling technology(2000).

[23] SING J K, KHAN K, BASU D K et al. Polynomial surface fitting based method for retrospective correction of intensity inhomogeneity in MR images[C], 405-409(2011).

[24] CHEN Dongren, WANG Guojin. Developable Bezier function surface[J]. Progress in Natural Science, 5, 65-69(2002).

[26] LIU Yu, HUANG Jianhua, ZHAO Chuanjiang et al. Experimental study on background noise suppression when focusing through scattering medium[J]. Acta Photonica Sinica, 52, 0129001(2023).

[27] LIU Xiang, ZHANG Lihua, DAI Zeyuan et al. A parameter-free denoising method for ICESat-2 point cloud under strong noise[J]. Acta Photonica Sinica, 51, 1110002(2022).