Acta Optica Sinica, Volume. 23, Issue 6, 662(2003)

To Test the Convergence Process of Astronomical Iterative Shift-and-Add Technique by Bispectrum

[in Chinese]*, [in Chinese], and [in Chinese]
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    References(6)

    [1] [1] Liu Zhong, Qiu Yaohui, Lu Ruwei. Reconstruction of video image through turbulent atmosphere. Proc. SPIE, 1998, 3561:326~331

    [3] [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] [4] Bartelt H, Lohmann A W, Wirnitzer B. Phase and amplitude recovery from bispectra. Appl. Opt., 1984, 23(18):3121~3129

    [6] [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] [7] Bates R HT, Cady F W. Towards true imaging by wideband speckle interferometry. Opt. Commun., 1980, 32(3):365~369

    [8] [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

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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

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    Paper Information

    Category: Fourier optics and signal processing

    Received: Apr. 1, 2002

    Accepted: --

    Published Online: Jun. 27, 2006

    The Author Email: (gfb@public.km.yn.cn)

    DOI:

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