RODDIER F. The effects of atmospheric turbulence in optical astronomy[J]. Progress in optics., 1981,19:281-376.[2] BABCOCK H W. The possibility of compensating astronomical seeing[J]. Publ. Astron. Soc., 1953,65:229-236.[3] PLATT B. History and principles of Shack-Hartmann wavefront sensing[J]. Journal of Refractive Surgery, 2001,17(5):573-577.[4] RODDIER F. Adaptive Optics in Astronomy[M]. Cambridge: Cambridge University Press,1999.[5] FRIED D L. Time-delay-induced mean-square error in adaptive optics[J]. J. Opt. Soc. Am. A, 1990,7(7):1224-1225.[6] TYLER G A. Bandwidth considerations for tracking through turbulence[J]. J. Opt. Soc. Am. A, 1994,11(1):358-367.[7] GREENWOOD D P. Bandwidth specification for adaptive optics systems[J]. J. Opt. Soc. Am., 1977,67(3):390-393.[8] CONAN J M, ROUSSET G, MADEC P Y. Wave-front temporal spectra in high-resolution imaging through turbulence[J]. J. Opt. Soc. Am. A,1995,12(7):1559-1570.[9] RAO C H, JIANG W H, LING N. Spatial and temporal characterization of phase fluctuations in non-Kolmogorov atmospheric turbulence[J]. Journal of Modern Optics, 2000,47(6):1111-1126.[10] KIBBLEWHITE E, CHUN M. Design of tip-tilt and adaptive optics servos using measured angle-of-arrival and phase power spectra[J]. SPIE, 1998,3353:522-530.[11] MCGAUGHEY D, JM AITKEN G. Temporal analysis of stellar wave-front-tilt data[J]. Journal of the Optical Society of America A, 1997,14(8):19671974.[12] GREENWOOD D P, FRIED D L. Power spectra requirements for wave-front-compensative systems[J]. J. Opt. Soc. Am., 1976,66(3):193-206.[13] 李华强, 宋贺伦, 饶长辉,等. 增大夏克-哈特曼波前传感器动态测量范围的方法[J]. 光学 精密工程, 2008,16(7):1203-1206. LI H Q, SONG H L, RAO C H, et al.. Extrapolation method to extend dynamic range of Shack-Hartmann wave-front sensor[J]. Optics and Precision Engineering, 2008,16(7):1203-1206.(in Chinese)