基于广义惠更斯-菲涅耳原理、修正von Karman湍谱、贝塞耳权重函数的高斯函数近似和误差小于4%的波结构函数平方近似,研究得出了包含湍流尺度影响的湍流大气中传输高斯光束的平均光强新关系和包含湍流外尺度影响的光束短期扩展因子.研究了高斯光束等效半径与传输距离、初始光束束径和光波波长间的关系,结果表明,在给定折射率结构参量和传输距离情况下,存在极小短期光束扩展对应的特征初始束径和特征光波波长.

文章给出了多包层标准单模光纤的宏弯曲损耗模型，这一损耗模型不仅适用于多包层单模光纤的宏弯曲损耗的计算，也适用于单包层单模光纤的宏弯曲损耗的计算。文章还讨论了弯曲半径及工作波长与单模光纤弯曲损耗之间的关系，并把这种关系与传统的弯曲损耗模型进行了比较，比较结果表明，单模光纤包层对弯曲损耗有很大的影响。此外，文章还运用模式耦合理论详细解释了廊(Whispering-gallery，WG)模对损耗振荡的影响。

The average intensity of finite laser beam propagating through turbulent atmosphere is calculated from the extended Huygens Fresnel principle. Formulas are presented for the slant path average intensity from an arbitrarily truncated Gaussian beam. The new expressions are derived from the modified von Karman spectrum for refractive-index fluctuations, quadratic approximation of the structure function, and Gaussian approximation for the product of Gaussian function and Bessel function. It is shown that the form of average intensity is not a Gaussian function but a polynomial of the power of the binomial function, Gaussian function, and the incomplete gamma function. The results also show that the mean irradiance of a finite optical beam propagating in slant path turbulent atmosphere not only depends on the effective beam radius at the transmitting aperture plane, propagation distance, and long-term lateral coherence length of spherical wave, but also on the radius of emit aperture.

为了数值求解平面光波导的弯曲损耗,首先给出了平面弯曲光波导的传输模型。基于这种模型,使用基于求解贝塞尔函数的方法数值求解出平面光波导的弯曲损耗。为了验证该方法的准确性,将计算得到的弯曲损耗结果与以往的实验结果相比较,结果表明,在弯曲半径较大的情况下两者基本吻合。