• Acta Optica Sinica
  • Vol. 19, Issue 7, 975 (1999)
[in Chinese], [in Chinese], and [in Chinese]
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  • [in Chinese]
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    [in Chinese], [in Chinese], [in Chinese]. Performance Analysis and Comparison of ICCD and CCD Types of Hartmann-Shack Wavefront Sensor Operated with Faint Object[J]. Acta Optica Sinica, 1999, 19(7): 975 Copy Citation Text show less
    References

    [1] Noll R J. Zernike polinomials and atmospheric turbulence. J. Opt. Soc. Am., 1976, 66(3):207~211

    [2] Yura H T. Short-term average optical beam spread in a turbulent medium. J. Opt. Soc. Am., 1973, 63(5):567~572

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

    [5] Morgan J S, Slater D C, Timothy J G et al.. Centroid position measurements and subpixel sensitivity variations with the MAMA detector. Appl. Opt., 1989, 28(6):1178~1192

    [6] Cao G, Cao Genrui, Yu Xin et al.. Accuracy analysis of a Hartmann-Shack wavefront sensor oprated with a faint object. Opt. Engng., 1994, 33(7):2331~2335

    [in Chinese], [in Chinese], [in Chinese]. Performance Analysis and Comparison of ICCD and CCD Types of Hartmann-Shack Wavefront Sensor Operated with Faint Object[J]. Acta Optica Sinica, 1999, 19(7): 975
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