• Acta Optica Sinica
  • Vol. 23, Issue 6, 662 (2003)
[in Chinese]*, [in Chinese], and [in Chinese]
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  • [in Chinese]
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    [in Chinese], [in Chinese], [in Chinese]. To Test the Convergence Process of Astronomical Iterative Shift-and-Add Technique by Bispectrum[J]. Acta Optica Sinica, 2003, 23(6): 662 Copy Citation Text show less
    References

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    [3] Lohmann A W, Weigelt G P, Wirnitzer B. Speckle masking in astronomy-trible correlation theory and application. Appl. Opt., 1983, 22(24):4028~4037

    [4] Bartelt H, Lohmann A W, Wirnitzer B. Phase and amplitude recovery from bispectra. Appl. Opt., 1984, 23(18):3121~3129

    [6] Labeyrie A. Attainment of diffraction limited resolution in large telescopes by Fourier analyzing speckle patterns in star images. Astron. Astrophs., 1970, 6(1):85~87

    [7] Bates R HT, Cady F W. Towards true imaging by wideband speckle interferometry. Opt. Commun., 1980, 32(3):365~369

    [8] Hunt B R, Fright W R, Bates R H T. Analysis of the shift and add method for imaging through turbulent media. J. Opt. Soc. Am., 1983, 73(4):456~465

    [in Chinese], [in Chinese], [in Chinese]. To Test the Convergence Process of Astronomical Iterative Shift-and-Add Technique by Bispectrum[J]. Acta Optica Sinica, 2003, 23(6): 662
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