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Beam propagation factor of radial Gaussian-Schell model beam array in non-Kolmogorov turbulence

机译:非Kolmogorov湍流中径向高斯-谢尔模型光束阵列的光束传播因子

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摘要

The analytical expression for the beam propagation factor (M ~2-factor) of a radial Gaussian-Schell model (GSM) beam array propagating in non-Kolmogorov turbulence is derived. The influences of beam number, ring radius and generalized exponent on the M~2-factor are investigated. The results indicate that the M~2-factor has great dependence on the generalized exponent and the beam number. Moreover, there is an optimum ring radius, which leads to a minimum M~2-factor and increases with increase in beam number. Further, the M~2-factor for the superposition of the intensity is larger than that for the superposition of the cross-spectral density function (CSDF). However, the M~2-factor for the superposition of the intensity is less sensitive to the turbulence than that for the superposition of the CSDF.
机译:推导了在非Kolmogorov湍流中传播的径向高斯-谢尔模型(GSM)波束阵列的波束传播因子(M〜2因子)的解析表达式。研究了束数,环半径和广义指数对M〜2因子的影响。结果表明,M〜2因子对广义指数和束数有很大的依赖性。而且,存在最佳的环形半径,这导致最小的M〜2因数,并随着光束数量的增加而增大。此外,用于强度叠加的M〜2因子大于用于交叉谱密度函数(CSDF)的叠加的M〜2因子。但是,强度叠加的M〜2因子对湍流的敏感度比CSDF叠加的M〜2因子小。

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