Acta Optica Sinica, Volume. 17, Issue 2, 175(1997)

Noise Analysis of an Adaptive Optics System Using Photon Counting Shearing Interferometer as Wavefront Sensor

[in Chinese], [in Chinese], and [in Chinese]
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    References(4)

    [2] [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] [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] [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] [6] J. Herrmann. Least-square wave front errors of minimumnorm. J. Opt. Soc. Am., 1980, 70(1): 28~35

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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

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    Paper Information

    Category: Atmospheric Optics and Oceanic Optics

    Received: Sep. 7, 1995

    Accepted: --

    Published Online: Oct. 31, 2006

    The Author Email:

    DOI:

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