Acta Optica Sinica, Volume. 19, Issue 7, 935(1999)
Phase Recovery Methods in Speckle Masking and Image Reconstruction Experiment
[1] [1] Labeyrie A. Attainment of diffraction limited resolution in large telescopes by Fourier analyzing speckle patterns in star images. Astron. Astrophys., 1970, 6(1):85~97
[2] [2] Lohmann A W, Weigelt G P, Wirnitzer B. Speckle masking in astronomytrible correlation theory and application. Appl. Opt., 1983, 22(24):4028~4037
[3] [3] Bartelt H, Lohmann A W, Wirnitzer B. Phase and amplitude recovery from bispectra. Appl. Opt., 1984, 23(18):3121~3129
[4] [4] Korff D. Analysis of a method for obtaning near diffraction limited information in presence of atmospheric turbulence. J. Opt. Soc. Am., 1973, 63(8):971~980
[5] [5] Meng J, Aitken G J M. Phase errors in near-axis bispectral stellar image reconstruction. J. Opt. Soc. Am. (A), 1994, 11(6):1736~1747
[8] [8] Haniff C A. Least-squares Fourier phase estimation from the modulo 2π bispectrum phase. J. Opt. Am. (A), 1991, 8(1):134~140
[9] [9] Takajo H, Takahashi T. Least-squares phase recovery from the bispectrum phase: an algorithm for a two-dimensional object. J. Opt. Soc. Am. (A), 1991, 8(7):1038~1047
[10] [10] Hofmann K -H, Weight G. Iterative image reconstruction from the bispectrum. Astr on. Astrophys., 1993, 278(1):328~339
Get Citation
Copy Citation Text
[in Chinese], [in Chinese], [in Chinese], [in Chinese]. Phase Recovery Methods in Speckle Masking and Image Reconstruction Experiment[J]. Acta Optica Sinica, 1999, 19(7): 935