Zhu Kaicheng, Li Shaoxin, Tang Ying, Yu Yan, Tang Huiqin
School of Physical Science and Technology, Central South University, Changsha, Hunan, China.
J Opt Soc Am A Opt Image Sci Vis. 2012 Mar 1;29(3):251-7. doi: 10.1364/JOSAA.29.000251.
Based on the integral representation of Bessel function and the extended Huygens-Fresnel principle, an integral expression of the Wigner distribution function (WDF) for partially coherent Bessel-Gaussian beams (PBGBs) propagating through turbulent atmosphere has been obtained. Also, the analytical formulas of the M2-factor for PBGB propagation in such a medium have been derived, which can be applied to cases of different spatial power spectra of the refractive index fluctuations. The performed numerical results reveal that the M2-factor of a PBGB in turbulent atmosphere depends on the beam parameters of the initial input beam, the structure constants of the turbulent atmosphere, and the propagation distance. These results may be useful in long-distance optical communications in free space or in turbulent atmosphere.
基于贝塞尔函数的积分表示和扩展的惠更斯-菲涅耳原理,得到了部分相干贝塞尔-高斯光束(PBGBs)在湍流大气中传播时维格纳分布函数(WDF)的积分表达式。此外,还推导了PBGB在这种介质中传播时M²因子的解析公式,该公式可应用于折射率起伏具有不同空间功率谱的情况。所进行的数值结果表明,湍流大气中PBGB的M²因子取决于初始输入光束的光束参数、湍流大气的结构常数和传播距离。这些结果可能在自由空间或湍流大气中的长距离光通信中有用。