Zhai Yanwang, Fu Shiyao, Zhang Jianqiang, Liu Xueting, Zhou Heng, Gao Chunqing
Opt Express. 2020 Mar 2;28(5):7515-7527. doi: 10.1364/OE.388526.
The vector vortex beams (VVB) possessing non-separable states of light, in which polarization and orbital angular momentum (OAM) are coupled, have attracted more and more attentions in science and technology, due to the unique nature of the light field. However, atmospheric transmission distortion is a recurring challenge hampering the practical application, such as communication and imaging. In this work, we built a deep learning based adaptive optics system to compensate the turbulence aberrations of the vector vortex mode in terms of phase distribution and mode purity. A turbulence aberration correction convolutional neural network (TACCNN) model, which can learn the mapping relationship of intensity profile of the distorted vector vortex modes and the turbulence phase generated by first 20 Zernike modes, is well designed. After supervised learning plentiful experimental samples, the TACCNN model compensates turbulence aberration for VVB quickly and accurately. For the first time, experimental results show that through correction, the mode purity of the distorted VVB improves from 19% to 70% under the turbulence strength of D/r0 = 5.28 with correction time 100 ms. Furthermore, both spatial modes and the light intensity distribution can be well compensated in different atmospheric turbulence.
具有光的不可分离态的矢量涡旋光束(VVB),其中偏振和轨道角动量(OAM)相互耦合,由于光场的独特性质,在科学技术领域受到越来越多的关注。然而,大气传输畸变是阻碍其在通信和成像等实际应用中的一个反复出现的挑战。在这项工作中,我们构建了一个基于深度学习的自适应光学系统,以根据相位分布和模式纯度来补偿矢量涡旋模式的湍流像差。精心设计了一个湍流像差校正卷积神经网络(TACCNN)模型,该模型可以学习失真矢量涡旋模式的强度分布与前20个泽尼克模式产生的湍流相位之间的映射关系。在对大量实验样本进行监督学习后,TACCNN模型能够快速准确地补偿VVB的湍流像差。实验结果首次表明,通过校正,在D/r0 = 5.28的湍流强度下,失真VVB的模式纯度从19%提高到70%,校正时间为100 ms。此外,在不同的大气湍流中,空间模式和光强分布都能得到很好的补偿。