Acta Optica Sinica, Volume. 20, Issue 4, 501(2000)

Fourier Modulus Recovery in Astronomical Speckle Imaging and the Experiments of Image Reconstruction

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

    [1] [1] Fried D L. Optical resolution through a randomly inhomogeneous medium for very long and very short exposures. J. Opt. Soc. Am., 1966, 56(10):1372~1379

    [2] [2] 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

    [3] [3] Knox K T, Thompson B J. Recovery of images from atmospherically-degraded short-exposure photographs. Astrophys. J., 1974, 193(1):L45~L48

    [4] [4] Lohmann A W, Weigelt G P, Wirnitzer B. Speckle masking in astronomy-trible correlation theory and application. Appl. Opt., 1983, 22(24):4028~4037

    [5] [5] Korff D. Analysis of a method for obtaining near diffrection limited informtion in presence of atmospheric turbulence. J. Opt. Soc. Am., 1973, 63(8):971~980

    [6] [6] von der Luhe O. Estimating Fried′s parameter from a time series of an arbitrary resolved object imaged through atmospheric turbulence. J. Opt. Soc. Am. (A), 1984, 1(5):510~519

    CLP Journals

    [1] MA Xue-lian. Effect of Atmospheric Turbulence on Resolution and Spot Radius of Long-term Exposure and Short-term Exposure[J]. Acta Photonica Sinica, 2015, 44(6): 601003

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    [in Chinese], [in Chinese], [in Chinese], [in Chinese]. Fourier Modulus Recovery in Astronomical Speckle Imaging and the Experiments of Image Reconstruction[J]. Acta Optica Sinica, 2000, 20(4): 501

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    Paper Information

    Category: Fourier optics and signal processing

    Received: Oct. 5, 1998

    Accepted: --

    Published Online: Aug. 9, 2006

    The Author Email:

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