Chinese Journal of Lasers, Volume. 51, Issue 8, 0804002(2024)

Atmospheric Wave‑Front Aberration Detection Using Sodium Laser Guide Star Under Strong Skylight Background

Xi Luo1,2、*, Xinyang Li1,2, Caixia Wang1, Xiaoyun Wang1, and Shijie Hu1
Author Affiliations
  • 1Key Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, Sichuan , China
  • 2University of Chinese Academy of Sciences, Beijing 100049, China
  • show less
    References(17)

    [1] Hardy J W[M]. Adaptive optics for astronomical telescopes(1998).

    [2] Humphreys R A, Primmerman C A, Bradley L C et al. Atmospheric-turbulence measurements using a synthetic beacon in the mesospheric sodium layer[J]. Optics Letters, 16, 1367-1369(1991).

    [3] Humphreys R A, Bradley L C, Herrmann J. Sodium-layer synthetic beacons for adaptive optics[J]. The Lincoln Laboratory Journal, 5, 45-66(1992).

    [4] Max C E, Olivier S S, Friedman H W et al. Image improvement from a sodium-layer laser guide star adaptive optics system[J]. Science, 277, 1649-1652(1997).

    [5] Wei K, Li M, Chen S Q et al. First light for the sodium laser guide star adaptive optics system on the Lijiang 1.8 m telescope[J]. Research in Astronomyand Astrophysics, 16, 183-189(2016).

    [6] Jin K. Research on wavefront detection of sodium beacon adaptive optical system[D], 10-13(2017).

    [7] Beckers J M, Cacciani A. Using laser beacons for daytime adaptive optics[J]. Experimental Astronomy, 11, 133-143(2001).

    [8] Beckers J M. The daytime use of adaptive optics for solar and stellar extremely large telescopes[C], 58, 83-89(2002).

    [9] Wilson K E, Wright M W, Lee S et al. Adaptive optics for daytime deep space laser communications from Mars[C], 19-20(2005).

    [10] Li C H. Research on the performance of field-of-view shifted Shack-Hartmann wavefront sensor in daytime[D], 79-89(2007).

    [11] Jiang W H. Adaptive optics techniques investigation in Institute of Optics and Electronics[J]. Opto-Electronic Engineering, 22, 1-13(1995).

    [12] Xu Z Y, Bo Y, Peng Q J et al. Progress on sodium laser guide star[J]. Infrared and Laser Engineering, 45, 0101001(2016).

    [13] Viard E, Delplancke F, Hubin N et al. Rayleigh scattering and laser spot elongation problems at ALFA[J]. Experimental Astronomy, 10, 123-133(2000).

    [14] Parenti R R. Adaptive optics for astronomy[J]. The Lincoln Laboratory Journal, 5, 93-114(1992).

    [15] Luo Q, Li X Y. Effects of beacons and wave-front detecting modes on control performance of adaptive optics systems[J]. Acta Optica Sinica, 35, 0801003(2015).

    [16] Bessell M S. UBVRI photometry. II - The cousins VRI system, its temperature and absolute flux calibration, and relevance for two-dimensional photometry[J]. Publications of the Astronomical Society of the Pacific, 91, 589-607(1979).

    [17] Lu G. Detection and recognition technology of small and weak targets in skylight background[D], 19-25(2008).

    Tools

    Get Citation

    Copy Citation Text

    Xi Luo, Xinyang Li, Caixia Wang, Xiaoyun Wang, Shijie Hu. Atmospheric Wave‑Front Aberration Detection Using Sodium Laser Guide Star Under Strong Skylight Background[J]. Chinese Journal of Lasers, 2024, 51(8): 0804002

    Download Citation

    EndNote(RIS)BibTexPlain Text
    Save article for my favorites
    Paper Information

    Category: Measurement and metrology

    Received: Jul. 17, 2023

    Accepted: Sep. 5, 2023

    Published Online: Mar. 29, 2024

    The Author Email: Luo Xi (luoxi@ioe.ac.cn)

    DOI:10.3788/CJL231028

    CSTR:32183.14.CJL231028

    Topics