在实验室模拟厚大气湍流及其在轨道角动量通信中的应用
光学
2014-03-21 v3
摘要
我们描述了一种程序，可通过该程序在受控条件下实验模拟穿过大气湍流的长距离（）光路，并将其缩放至实验室环境中易于实现的距离。随后，该程序被用于模拟一个 1 公里长的自由空间通信链路，其中信息编码在轨道角动量 (OAM) 空间模式中。我们还证明了标准自适应光学方法可用于减轻厚大气湍流的许多影响。
引用
@article{arxiv.1301.7454,
title = {Simulating thick atmospheric turbulence in the lab with application to orbital angular momentum communication},
author = {Brandon Rodenburg and Mohammad Mirhosseini and Mehul Malik and Omar S. Magaña-Loaiza and Michael Yanakas and Laura Maher and Nicholas K. Steinhoff and Glenn A. Tyler and Robert W. Boyd},
journal= {arXiv preprint arXiv:1301.7454},
year = {2014}
}
备注
Rewritten abstract and introductory section to emphasize the importance of the work and to make it accessible to a more general audience. Section 2 was expanded to include some background on the physics of turbulence to allow the paper to be self-contained and understood by nonspecialists