[1] Labeyrie A. Attainment of diffraction limited resolution in large telescopes by Fourier analyzing speckle patterns in star images. Astron. Aatrophs., 1970, 6(1):85～87
[2] Lohmann A W, Weigelt G P, Wirnitzer B. Speckle masking in astronomy-trible correlation theory and application. Appl. Opt., 1983, 22(24):4028～4037
[3] Bartelt H, Lohmann A W, Wirnitzer B. Phase and amplitude recovery from bispectra. Appl. Opt., 1984, 23(18):3121～3129
[4] Meng J, Aitken G J M. Phase errors in near-axis bispectral stellar image reconstrucion. J. Opt. Soc. Am. (A), 1994, 11(6):1736～1747
[5] Haniff C A. Least-squares Fourier phase estimation from the modulo 2π bispectrum phase. J. Opt. Soc. Am. (A), 1991, 8(1):134～140
[6] Takajo H, Takahashi T. Least-squares phase recovery from the bispectrum phase: An algorithm for a two-dimensinal object. J. Opt. Soc. Am. (A), 1991, 8(7):1038～1047
[7] Hofmann K H, Weigelt G. Image reconstruction from the bispectrum using an iterative algrithm and applications of the method to astronomical objects. Proc. SPIE, 1990, 1351:522～525
[8] Hofmann K H, Weigelt G. Iterative image reconstruction from the bispectrum. Aston. Astrophys, 1993, 278(1):328～339
[9] Liu Zhing, Qiu Yaohui, Lu Ruwei. Reconstruction of video image through turbulent atmosphere. Proc. SPIE, 1998, 3561:326～331
[10] Wirnitzer B. Bispectra analysis at low light levels and astronomical speckle masking. J. Opt. Soc. Am. (A), 1985, 2(1):14～21
[11] Pehlemann E, Hofmann K H, Weigelt G. Photon bias compensation in triblecorrelation imaging and observation of R136. Astron. Aatrophs., 1992, 256(2):701～714
