Liu Dajun, Yin Hongming, Wang Guiqiu, Wang Yaochuan
Appl Opt. 2017 Nov 1;56(31):8785-8792. doi: 10.1364/AO.56.008785.
The partially coherent Lorentz-Gauss vortex beam generated by a Schell-model source has been introduced. Based on the extended Huygens-Fresnel principle, the cross-spectral density function of a partially coherent Lorentz-Gauss vortex beam propagating in oceanic turbulence is derived. The influences of coherence length, topological charge M, and oceanic turbulence on the spreading properties and position of the coherence vortex for a partially coherent Lorentz-Gauss vortex beam are analyzed in detail. The results show that a partially coherent Lorentz-Gauss vortex beam propagating in stronger oceanic turbulence will evolve into a Gaussian-like beam more rapidly as the propagation distance increases, and the number of coherent vortices will change.
介绍了由谢尔模型源产生的部分相干洛伦兹 - 高斯涡旋光束。基于扩展的惠更斯 - 菲涅耳原理,推导了部分相干洛伦兹 - 高斯涡旋光束在海洋湍流中传播时的交叉谱密度函数。详细分析了相干长度、拓扑电荷M和海洋湍流对部分相干洛伦兹 - 高斯涡旋光束的扩展特性和相干涡旋位置的影响。结果表明,在较强海洋湍流中传播的部分相干洛伦兹 - 高斯涡旋光束随着传播距离的增加将更快地演化为类高斯光束,并且相干涡旋的数量会发生变化。