Zhou Junhe, Wu Jianjie, Hu Qinsong
Opt Express. 2018 Dec 10;26(25):33333-33348. doi: 10.1364/OE.26.033333.
In this paper, an optimal mode set is proposed to maximize the receiving power for free space transmission under atmosphere turbulence with transmitter/receiver aperture size constraint. The optimal beam profiles are evaluated through eigenmode analysis of the Fredholm integral equation, which is mathematically equivalent to the eigen vector analysis of an infinitely large matrix. The matrix is formed by orthonormal basis expansion, and its element is the overlap integral of the orthonormal basis functions and the Fredholm kernel. If circular aperture is implemented, then it is rigorously proven in this work that the eigenmodes possess certain topological charges (i.e., they are the OAM modes). These OAM modes have specific radial beam profiles, which have been optimized to minimize the power loss and the inter-mode crosstalk. While the traditional OAM beams, such as the Laguerre-Gauss (LG) beams, suffer significant energy loss and inter-radial-mode crosstalk, the optimized beam profiles will remarkably reduce the penalties.
本文提出了一种最优模式集,用于在存在发射机/接收机孔径尺寸约束的大气湍流条件下,最大化自由空间传输的接收功率。通过对弗雷德霍姆积分方程进行本征模分析来评估最优光束分布,这在数学上等同于对一个无限大矩阵进行特征向量分析。该矩阵由正交基展开形成,其元素是正交基函数与弗雷德霍姆核的重叠积分。如果采用圆形孔径,那么在本工作中严格证明了本征模具有特定的拓扑电荷(即它们是轨道角动量模式)。这些轨道角动量模式具有特定的径向光束分布,已对其进行优化以最小化功率损耗和模间串扰。虽然传统的轨道角动量光束,如拉盖尔 - 高斯(LG)光束,会遭受显著的能量损失和径向模间串扰,但优化后的光束分布将显著降低这些不利影响。