本文介绍一种光学/数字混合图像处理方法,它可用于星体斑点干涉术,以克服大气扰动的影响,使天文望远镜达到理论衍射极限.混合处理系统包括相干光傅里叶交换装置、光学输出数字化的显微密度计和微计算机三部分。在简单分析星体斑点干涉术数据处理的要求之后,本文将叙述系统各部分的组成和设计,介绍处理模拟星体图像的结果,讨论今后的发展和其它可能的应用。 This paper presents an optical / digital hybrid image processing method that can be used in speckle speckle interferometry to overcome the effects of atmospheric perturbations to achieve the theoretical diffraction limit of telescopes. Hybrid processing systems include coherent optical Fourier switching devices, digital optical output Micro-density meter and microcomputer three parts. After a brief analysis of the data processing requirements for astral speckle interferometry, this article describes the composition and design of each part of the system, describes the results of dealing with simulated astral images, discusses future developments and other possible applications.