• Acta Optica Sinica
  • Vol. 22, Issue 7, 829 (2002)
[in Chinese]1、2、*, [in Chinese]1、2, [in Chinese]1、2, and [in Chinese]1、2
Author Affiliations
  • 1[in Chinese]
  • 2[in Chinese]
  • show less
    DOI: Cite this Article Set citation alerts
    [in Chinese], [in Chinese], [in Chinese], [in Chinese]. Noise Bias Compensation in the Iterative Shift-and-Add Method for Astronomical Image Reconstruction[J]. Acta Optica Sinica, 2002, 22(7): 829 Copy Citation Text show less
    References

    [1] 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

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

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

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

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

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

    [10] Korff D. Analysis of a method for obtaining near-diffraction-limited information in the presence of atmospheric turbulence. J. Opt. Soc. Am., 1973,63(8):971~980

    [in Chinese], [in Chinese], [in Chinese], [in Chinese]. Noise Bias Compensation in the Iterative Shift-and-Add Method for Astronomical Image Reconstruction[J]. Acta Optica Sinica, 2002, 22(7): 829
    Download Citation