[1] Sandler D G, Stahl S, Angel J R P, et al. Adaptive optics for diffraction-limited infrared imaging with 8-m telescopes[J]. J. Opt. Soc. Am. A, 1994, 11: 925-945.
[2] Parenti R R, Sasiela R J. Laser-guide-star systems for astronomical applications[J]. J. Opt. Soc. Am. A, 1994, 11(1): 288-309.
[3] Ge J, Jacobsena B D, Angela J R P, et. al. Sodium laser guide star brightness, spot size, and sodium layer abundance[C]. Proc. SPIE, 1998, 3353: 242-253.
[4] Thomas S, Fusco T, Tokovinin A, et al. Comparison of centroid computation algorithms in a Shack-Hartmann sensor[J]. Mon. Not. R. Astron. Soc., 2006, 371: 323-336.
[5] Cao G, Yu X. Accuracy analysis of a Hartmann-Shack wavefront sensor operated with a faint object[J]. Opt. Eng., 1994, 33(7): 2331-2335.
[6] Rao Ruizhong. Modern Atmospheric Optics[M]. Beijing: Science Press, 2012: 463-473(in Chinese).
[8] Jelonek M P, Fugate R Q, Lange W J, et al. Characterization of artificial guide stars generated in the mesospheric sodium layer with a sum-frequency laser[J]. J. Opt. Soc. Am. A, 1994, 11(2): 806-812.
[9] McGuigan R J, Schmidt J D. Effect of Coudè pupil rotation on sodium laser beacon perspective elongation[C]. IEEE AC paper, 2010, 1: 26
[10] Liu Xiangyuan, Qian Xianmei, Liu Dandan, et al. Influencing factors and numerical simulations for the number of return photons from Sodium Laser Beacon[J]. Chinese Journal of Lasers, 2013, 40(6): 0613001-1-10(in Chinese).