[1] [1] Jiang Wenhan, Li Mingquan, Tang Guomao et al.. Adaptive optics image compensation experiments for star objects. Opt. Engng., 1995, 34(1):15～20

[4] [4] Dai G M. Modal wave-front reconstruction with zernike polynomials and Karhunen-Loeve functions. J. Opt. Soc. Am. (A), 1996, 13(6):1218～1225

[5] [5] Roddier F. The effects of atmospheric turbulence in optical astronomy. in Wolf E, ed., Progress in Optics, Amsterdam: North-Holland, 1981, XIX, 281～376

[6] [6] Veran J P, Rigaut F, Maitre H et al.. Estimation of the adaptive optics long-exposure point-spread function using control loop data. J. Opt. Soc. Am. (A), 1997, 14(11):3057～3069

[7] [7] Dai G M. Modal compensation of atmospheric turbulence with the use of zernike polynomials and Karhunen-Loeve functions. J. Opt. Soc. Am. (A), 1995, 12(10):2182～2193

[9] [9] Boreman G D, Dainty C. Zernike expansions for non-Kolmogorov turbulence. J. Opt. Soc. Am. (A), 1996, 13(3):517～522

[10] [10] Conan J M, Rousset G, Madec P Y. Wave-front temporal spectra in high-resolution imaging through turbulence. J. Opt. Soc. Am. (A), 1995, 12(7):1559～1570

[11] [11] Cubalchini R. Modal wave-front estimation from phase derivative measurements. J. Opt. Soc. Am., 1979, 69(7):972～977

[13] [13] Wang J Y. Optical resolution through a turbulent medium with adaptive phase compensation. J. Opt. Soc. Am., 1977, 67(3):383～390