[1] [1] Fiete R D, Tantalo T A, Calus J R, et al.. Image quality of sparse- aperture designs for remote sensing[J]. Optical Engineering, 2002, 41(8): 1957-1969.

[2] [2] Gonsalves R A. Phase retrieval and diversity in adaptive optics[J]. Optical Engineering, 1982, 21(5): 829-829.

[3] [3] Zhang S, Wang B, Zhao J. High resolution optical image restoration for ground based large telescope using phase diversity speckle[J]. Optik-International Journal for Light and Electron Optics, 2014, 125(2): 861-864.

[4] [4] Lofdahl M G, Scharmer G B. Wavefront sensing and image restoration from focused and defocused solar images[J]. Astronomy and Astrophysics Supplement Series, 1994, 107: 243-264.

[5] [5] Vogel C R, Chan T, Plemmons R. Fast Algorithms for phase diversity- based blind deconvolution[C]. Astronomical Telescopes & Instrumentation, 1998: 994-1005.

[6] [6] Wang Xin, Zhao Dazun. Influence of noise to phase diversity wavefront sensing[J]. Acta Optica Sinica, 2009, 29(8): 2142-2146.

[7] [7] Smith C S, Marinica R, Verhaegen M. Real- time wavefront reconstruction from intensity measurements[C]. Third AO4EL7 Conference Adaptive Optics for the Extremely Large Telescopes, 2013.

[8] [8] Luo Q, Huang L, Gu N, et al.. Experimental study of a modified phase diversity with a diffraction grating[J]. Opt Express, 2012, 20(11): 12059-12066.

[9] [9] Paxman R G, Fienup J R. Optical misalignment sensing and image reconstruction using phase diversity[J]. JOSA A, 1988, 5(6): 914-923.

[10] [10] Gonzalez R C, Woods R E. Digital Picture Processing: 2nd[M]. Bei Jing: Electronic Industry Press, 2007.

[11] [11] Fan Junliu, Wu Quanying, Wang Fuliang, et al.. Design of Golay 3telescope system[J]. Optics and Precision Engineering, 2011, 19(12): 2677-2683.

[12] [12] Chen Qihai, Wang Zhile, Zhang Wei. Study on subaperture aberration of optical synthetic aperture imaging system[J]. Journal of Applied Optics, 2006, 27(2): 112-115.

[13] [13] Wu Q, Fan J, Wu F, et al.. Error analysis of the Golay3 optical imaging system[J]. Applied Optics, 2013, 52(13): 2966-2973.