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首页> 外文期刊>Journal of Modern Optics >A comparative study of standard and elegant Hermite-Gaussian beams propagating through turbulent atmosphere
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A comparative study of standard and elegant Hermite-Gaussian beams propagating through turbulent atmosphere

机译:标准和优雅的厄米-高斯光束在湍流中传播的比较研究

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摘要

Based on the extended Huygens-Fresnel principle and the definition of the second-order moments of the Wigner distribution function (WDF), the analytical expressions for the root-mean-square (rms) beam width and far-field divergence angle, curvature radius and M~2-factor of standard Hermite-Gaussian (SHG) and elegant Hermite-Gaussian (EHG) beams passing through turbulent atmosphere are derived and compared. It is shown that in turbulent atmosphere the far-field divergence angle of SHG and EHG beams is equal under the same conditions, but the rms beam width, curvature radius and the M ~2-factor of SHG and EHG beams are different except for beam orders m = 0 and m = 1. The relative rms beam width, relative curvature radius and relative M~2-factor of SHG beams are less than those of EHG beams. Therefore, the conclusion that SHG beams are less influenced by turbulence than EHG beams can be drawn if we examine one of the above three relative beam parameters.
机译:基于扩展的惠更斯-菲涅耳原理和维格纳分布函数(WDF)的二阶矩的定义,均方根光束宽度和远场发散角,曲率半径的解析表达式推导并比较了标准厄米-高斯光束(SHG)和优雅厄米-高斯光束(EHG)通过湍流的M〜2因子。结果表明,在相同条件下,SHG和EHG光束的远场发散角相等,但除光束外,均方根光束宽度,曲率半径和SHG和EHG光束的M〜2因子均不同。 m = 0和m = 1的阶数。SHG光束的相对均方根光束宽度,相对曲率半径和相对M〜2因子小于EHG光束。因此,如果我们检查以上三个相对光束参数之一,则可以得出SHG光束受湍流影响小于EHG光束的结论。

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