• Acta Optica Sinica
  • Vol. 24, Issue 3, 408 (2004)
[in Chinese]1、*, [in Chinese]2, [in Chinese]2, and [in Chinese]1
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  • 1[in Chinese]
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    [in Chinese], [in Chinese], [in Chinese], [in Chinese]. Research of Fourier Phase in Optical Synthetic-Aperture Imaging Technique[J]. Acta Optica Sinica, 2004, 24(3): 408 Copy Citation Text show less
    References

    [4] Ferwerda H A. The Phase Reconstruction Problem for Wave Amplitudes and Coherence Functions. Baltes H P. Inverse Problem in Optics, Springer-Verlag, 1978

    [6] Monnier J D. An introduction to Closure phases. Principle of Long Baseline Stellar Interferometry. NASA Report. 2000.Edited by Lawson P R, 2000. 202~230

    [7] Baldwin J E, Haniff C A, Mackay C D. Close phase in high resolution optical imaging.Nature,1986,320(6063):595~597

    [8] Edward B. Fomalont, Melvyn C. H. Wright, Interferometry and Aperture Synthesis. Galactic and Extra-Galactic Radio Astronomy, 1st edition. Verschuur G L, Kellermann K I ed. NewYork: Springer-Verlag, 1974. 256~290

    [9] Pearson T J, Readhead A C S. Image formation by self-calibration in radio astronomy. A&A, 1984, 22:97~130

    [10] Qiu Yaohui, Liu zhong, Lu Ruwei et al.. The application of clean algorithm to astronomical image reconstruction working in spatial domain. Publications of the Yunnan Observatory, 2000,(2):1~9

    [in Chinese], [in Chinese], [in Chinese], [in Chinese]. Research of Fourier Phase in Optical Synthetic-Aperture Imaging Technique[J]. Acta Optica Sinica, 2004, 24(3): 408
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