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Propagation properties of radially polarized partially coherent beam in the oceanic turbulence

机译:径向偏振部分相干光束在海洋湍流中的传播特性

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Based on the extended Huygens–Fresnel principle and the second-order moments of the Wigner distribution function,propagation properties of radially polarized partially coherent beam in the oceanic turbulence are investigated. Ananalytical formula for the propagation factors (M~2-factors) of partially coherent one-dimensional radially polarized beamsin turbulent ocean is derived. The intensity distribution, degree of polarization and beam characteristic parameters ofradially polarized partially coherent beam in turbulent ocean are numerically described in detail. It is shown that theoceanic turbulence parameters and the initial coherence length have significant influence on the degree of polarization andcoherence for radially polarized partially coherent beams, and such beam is depolarized on propagation. As the value of theoceanic turbulence parameters (χT or w) increases and the coherence length of the beam decreases, the normalizedM2-factor increases more rapidly. The results will be useful in long-distance free-space optical communications.
机译:基于扩展的惠更斯-菲涅耳原理和维格纳分布函数的二阶矩, 研究了径向偏振的部分相干光束在海洋湍流中的传播特性。一个 部分相干一维径向偏振光束的传播因子(M〜2因子)的解析公式 在动荡的海洋中衍生而来。激光的强度分布,偏振度和光束特性参数。 详细描述了湍流海洋中径向极化的部分相干光束。结果表明 海洋湍流参数和初始相干长度对极化程度和 径向偏振的部分相干光束具有相同的相干性,并且这种光束在传播时会被去极化。作为价值 海洋湍流参数(χT或w)增加而波束的相干长度减少,归一化 M2因子增加更快。该结果将对长距离自由空间光通信有用。

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