• Acta Optica Sinica
  • Vol. 17, Issue 2, 175 (1997)
[in Chinese], [in Chinese], and [in Chinese]
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  • [in Chinese]
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    [in Chinese], [in Chinese], [in Chinese]. Noise Analysis of an Adaptive Optics System Using Photon Counting Shearing Interferometer as Wavefront Sensor[J]. Acta Optica Sinica, 1997, 17(2): 175 Copy Citation Text show less
    References

    [2] Wenhan Jiang, Mingquan Li, Guomao Tang et al.. Adaptive optics image compensation experiments for star objects. Opt. Engng., 1995, 34(1): 15~20

    [4] R. R. Parenti, R. J. Sasiela. Laser-guide-star systems for astronomical applications. J. Opt. Soc. Am. (A), 1994, 11(1): 288~309

    [5] J. C. Wyant. Use of an heterodyne lateral shear interferometer with real-time wavefront correction systems. Applied Optics, 1975, 14(11): 2622~2626

    [6] J. Herrmann. Least-square wave front errors of minimumnorm. J. Opt. Soc. Am., 1980, 70(1): 28~35

    [in Chinese], [in Chinese], [in Chinese]. Noise Analysis of an Adaptive Optics System Using Photon Counting Shearing Interferometer as Wavefront Sensor[J]. Acta Optica Sinica, 1997, 17(2): 175
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