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宏-微脉冲激光激发钠信标回波光子数的数值计算与探讨

刘向远 钱仙妹 张穗萌 崔朝龙

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宏-微脉冲激光激发钠信标回波光子数的数值计算与探讨

刘向远, 钱仙妹, 张穗萌, 崔朝龙

Numerical calculation and discussion on the return photon number of sodium laser beacon excited by a macro-micro pulse laser

Liu Xiang-Yuan, Qian Xian-Mei, Zhang Sui-Meng, Cui Chao-Long
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  • 当采用低功率的宏-微脉冲激光激发钠信标时, 尽管激光传输和钠信标光斑大小受到大气湍流影响, 但是钠信标具有回波光子数无起伏且激发品质因数高的优点. 除此之外, 宏-微脉冲激光激发钠信标还与激光的宏脉冲线型有关. 对于高斯线型的宏脉冲, 增大微脉冲的宽度有利于提高激发钠信标的品质因数和激发态概率. 为了获得更多的钠信标回波光子和较小的钠信标半径, 增大激光功率的同时要考虑良好的光束质量、适当的激光发射口径以及光谱宽度等影响因素. 因此, 优选宏-微脉冲激光的参数、发射口径、发射方式等对于激发优良特性的钠信标有着重要的现实意义.
    Sodium laser beacon (SLB) excited by a macro-micro pulse laser with low power has the following advantages: the return photons without fluctuations and the high merit quantity, although the laser beam propagation and the size of SLB suffer form the atmospheric turbulence. In addition, the macro-pulse profile may influence the interaction of laser and sodium atoms. For the macro-pulse with a Gaussian profile, it is useful to enhance the merit quantity and the excitation probability of the SLB to increase the width of micropulse. In order to obtain more of the return photons in the SLB, while increasing the laser power, the fine beam quality, the appropriate launch diameter, and the spectral width of the laser etc. must be considered. Therefore, it is of practical significance for the SLB with fine characteristics to optimize the laser parameters, the launch diameter and launch pattern.
    • 基金项目: 安徽省高校自然科学基金(批准号: KJ2013A260, KJ2013B331)和国家自然科学基金(批准号: 61107066) 资助的课题.
    • Funds: Project supported by the College Natural Science Foundation of Anhui Province, China (Grant Nos. KJ2013A260, KJ2013B331), and the National Natural Science Foundation of China (Grant No. 61107066).
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    Bradley L C 1992 J. Opt. Soc. Am. B 9 1931

    [2]

    Telle J M, Milonni P W, Hiliman P D 1998 Proc. SPIE 3264 37

    [3]

    Kibllewhite E, Shi F 1998 Proc. SPIE 3353 300

    [4]

    Milonni P W, Thode L E 1992 Applied Optics 31 785

    [5]

    Stephen C R 2010 Nonlinear and Quantum Optics using the Density Matrix (British: Oxford University Press) p43

    [6]

    Temkin R J 1993 J. Opt. Soc. B 10 830

    [7]

    Jelonek M P, Fugate R Q, Lange W J, Slavin A C, Ruane R E, Cleis R A 1994 J. Opt. Soc. Am. A 11 806

    [8]

    Rao R Z 2012 Modern Atmospheric Optics (Beijing: Science Press) p428 (in Chinese)[饶瑞中 2012 现代大气光学(北京: 科学出版社)第428页]

    [9]

    Telle J M, Milonni P W, Hiliman P D 1998 Proc. SPIE 3264 37

    [10]

    Humphreys R A, Bradley L C, Herrmann J 1992 The Lincoln Laboratory Journal 6 45

    [11]

    Zhu W Y, Huang Y B, Qian X M, Rao R Z, Wang Y J 2007 Journal of atmospheric and Eenvironmental Optics 2 451 (in Chinese) [朱文越, 黄印博, 钱仙妹, 饶瑞中, 王英俭 2007 大气与环境光学学报2 451]

    [12]

    Cai D M, Wang K, Jia P, Wang D, Liu J X 2014 Acta Phys. Sin. 63 104217 (in Chinese) [蔡冬梅, 王昆, 贾鹏, 王东, 刘建霞 2014 63 104217]

    [13]

    Shi F 2001 Publications of the Astronomical Society of the Pacific 113 366

    [14]

    Ageorges N, Dainty C 2000 Laser Guide Star Adaptive Optics for Astronomy (London: Kluwer Academic Publishers) p59

    [15]

    Qian X M, Zhu W Y, Rao R Z 2008 Acta Photonica Sinica 37 1525

    [16]

    Holzlöhner R, Rochester S M, Calia D B, Budker D, Higbie J M, Hackenberg W 2010 Astronomy & Astrophysics 50 1

    [17]

    Liu X Y, Qian X M, Li Y J, Rao R Z 2014 Chin. Phys. B 23 124213

    [18]

    Rochester S M, Otarola A, Boyer C, Budker D, Ellerbroek B, Holzlöhner R, Wang L 2012 J. Opt. Soc. Am. A 6 832

    [19]

    Strohben J W 1978 Laser beam Propagation in the atmosphere (Berlin: Springer-Verlag) p129

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出版历程
  • 收稿日期:  2014-10-05
  • 修回日期:  2014-11-06
  • 刊出日期:  2015-05-05

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