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Intensity distribution and spectral degree of coherence for array beams in non-Kolmogorov atmospheric turbulence

机译:非Kolmogorov大气湍流中阵列光束的强度分布和相干度

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The propagation expressions of the intensity distribution and the spectral degree of coherence for radial array Gaussian Schell-model beams in non-Kolmogorov atmospheric turbulence have been derived. There exists a maximum of the on-axis intensity for radial array beams on propagation. The optimal propagation distance where the maximum appears has been analyzed in detail. The influence of the generalized structure constant and the initial spatial coherence parameter for the correlated superposition beam is different from the uncorrelated one. In particular, the on-axis intensity maximum exhibits a minimum when the generalized exponent alpha = 3.1. The spectral degree of coherence for the correlated superposition beam is larger than the uncorrelated one, and the difference between the two superposition styles becomes larger when the spatial coherence parameter becomes larger and the turbulence becomes weaker. Moreover, when alpha = 3.1 the spectral degree of coherence exhibits a minimum.
机译:推导了非柯尔莫哥罗夫大气湍流中径向阵列高斯谢尔模型光束的强度分布和相干谱度的传播表达式。传播时,径向阵列光束的轴上强度最大。已对出现最大值的最佳传播距离进行了详细分析。广义结构常数和初始空间相干参数对相关叠加光束的影响与不相关光束的影响不同。特别是,当广义指数alpha = 3.1时,轴向强度最大值呈现最小值。相关的叠加光束的光谱相干度大于不相关的光束,并且当空间相干参数变大且湍流变弱时,两种叠加样式之间的差异变大。此外,当α= 3.1时,光谱的相干度显示为最小值。

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