• Acta Optica Sinica
  • Vol. 21, Issue 2, 186 (2001)
[in Chinese], [in Chinese], [in Chinese], and [in Chinese]
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  • [in Chinese]
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    [in Chinese], [in Chinese], [in Chinese], [in Chinese]. A New Method for Astronomical Image Reconstruction in Spatial Region: Iterative Shift-and-Add Technique[J]. Acta Optica Sinica, 2001, 21(2): 186 Copy Citation Text show less
    References

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

    [5] Fienup J R. Reconstruction of an object from the modulus of its Fourier transform. Opt. Lett., 1978, 3(1):27~29

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

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

    [9] Bates R H T, Cady F M. Towards true imaging by wideband speckle interferometry. Opt. Commun., 1980, 32(3):365~369

    [10] Ribak E. Astronomical images by filtered weighted shift-and-add technique. J. Opt. Soc. Am. (A), 1986, 3(12):2069~2076

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

    CLP Journals

    [1] Jin Zhenyu, Liu Zhong, Qiu Yaohui. Improvement of Iterative Shift-and-Add Image Reconstruction Method[J]. Acta Optica Sinica, 2009, 29(5): 1205

    [in Chinese], [in Chinese], [in Chinese], [in Chinese]. A New Method for Astronomical Image Reconstruction in Spatial Region: Iterative Shift-and-Add Technique[J]. Acta Optica Sinica, 2001, 21(2): 186
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