Acta Optica Sinica, Volume. 19, Issue 2, 151(1999)

An Experiment in Astronomical High Resolution Image Reconstruction with Speckle Holography

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

    [2] [2] D. L. Fried. Optical resolution through a random1y inhomogeneous mediumfor very long and very short exposures. J. Opt. Soc. Am., 1966, 56(10):1372~1379

    [3] [3] A. Labeyrie. Attainment of diffraction limited resolution in large telescopes by Fourier analyzing speckle patterns in star images. Astron. Astrophs., 1970. 6(1):85~87

    [4] [4] C. Y. C. Liu, A. W. Lohmann. High resolution image formation through the turbulent atmosphere. Opt. Commun., 1973, 8(3):372~377

    [5] [5] R. H. T. Bates, P. T. Gough, P. J. Napier. Speckle interferometry gives holograms of multiple star systems. Astron. Asrtrophys., 1973, 22(2):319~320

    [6] [6] D. Korff. Analysis of a method for obtaining near diffrection limited information in presence of atmospherie turbulence. J. Opt. Soc. Am., 1973, 63(8):971~980

    [9] [9] Sky Catalogue 2000.0 Vo1.2 Double Stars. Variable Stars and Nonstellar Ojects, Edited by Alan Hirshfeld, Roger W. Sinnott, New York: Press Syndicate of the Univers ity of Cambridge, 1985.

    CLP Journals

    [1] Li Fei, Rao Changhui. Least Square Phase Retrieval Algorithm Based on Defocusing Grating[J]. Chinese Journal of Lasers, 2010, 37(11): 2813

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    [in Chinese], [in Chinese], [in Chinese], [in Chinese], [in Chinese]. An Experiment in Astronomical High Resolution Image Reconstruction with Speckle Holography[J]. Acta Optica Sinica, 1999, 19(2): 151

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    Paper Information

    Category: Holography

    Received: Nov. 18, 1997

    Accepted: --

    Published Online: Aug. 9, 2006

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