[1] [1] Sheppard D G, Hunt B R, Marcellin M W. Iterative multiframe super-resolution algorithms for atmospheric turbulence-degraded imagery ［J］. IEEE Trans. Image Proc., 1998, 4: 2857-2860.

[2] [2] Green J J, Hunt B R. Improved restoration of space imagery ［J］. J. Opt. Soc. Am. A, 1999, 16(12): 2859-2865.

[3] [3] Tyson R K. Principles of Adaptive Optics ［M］. 3rd ed., Florida: CRC Press, 2011.

[4] [4] Hardy J W, Lefebvre J E, Koliopoulos C L. Real-time atmospheric compensation ［J］. J. Opt. Soc. Am., 1977, 67: 360-369.

[5] [5] van Iersel M, van Eijk A M J. Estimating turbulence in images ［C］. Free-Space Laser Communications X, Proc. SPIE, 2010, 7814: 78140Q.

[6] [6] Roddier F, ed. Adaptive Optics in Astronomy ［M］. Cambridge: Cambridge University Press, 1999.

[7] [7] Hart M. Recent advances in astronomical adaptive optics ［J］. Appl. Opt. 2010, 49(16): D17-D29.

[8] [8] Hardy J W. Adaptive Optics for Astronomical Telescopes ［M］. New York: Oxford University Press, 1998.

[9] [9] Niu S S, Shen J X, Liang C, et al. High-resolution retinal imaging with micro adaptive optics system ［J］. Appl. Opt., 2011, 50(22): 4365-4375.

[10] [10] Loktev M, Soloviev O, Vdovin G. Adaptive Optics Guide ［M］. 3rd ed., 2008, Flexible Optical BV (OKOr Technologies).

[11] [11] Chen C, Fei J D, Yi S H, et al. Study on the temporal and spatial characteristics of high-speed turbulent flow field and its optical transmission effects ［C］. Proc. SPIE, 2011, 8193: 819303.

[12] [12] Mi Q, Fei J D, Chen C. A real-time restoring method for infrared images degraded by high speed airflow ［C］. Proc. SPIE, 2011, 8193: 81934R.