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一种具有低F数和宽视场的制冷中波红外离轴三镜系统的光学设计。

Optical design of a cooled mid-wave infrared off-axis three-mirror system with a low F-number and wide field of view.

作者信息

Xie Yunqiang, Liu Chunyu, Liu Shuai, Xu Minglin, Fan Xinghao, Rao Qilong

出版信息

Appl Opt. 2022 Mar 1;61(7):1652-1659. doi: 10.1364/AO.449841.

DOI:10.1364/AO.449841
PMID:35297841
Abstract

Infrared imaging systems with a wide detection scale, excellent precision, and high resolution are playing an increasingly important role in many fields. Compared with uncooled infrared detectors, the cooled infrared detectors have the advantages of high precision, long detection distance, and a high signal-to-noise ratio due to the low working temperature. In this paper, a cooled off-axis three-mirror mid-wave infrared (MWIR) optical system with a wide field of view (FOV), long focal length, and large relative aperture is designed. We first establish the initial coaxial three-mirror system based on the third-order Seidel aberration theory and then make the aperture stop offset to eliminate central obscuration. During the process of optimization, the FOV of the system is expanded stepwise, and it is not biased to avoid the extra aberration. In order to increase the optimizing degrees of freedom to improve the aberration elimination ability of the system, we apply the polynomial surface on the tertiary mirror (TM). After optimization, we finally obtain a cooled off-axis three-mirror MWIR optical system with a FOV of 5.3×4.4, a focal length of 500 mm, and a relative aperture of 1/2. The image quality of our system is excellent, and the aperture stop is between the focal plane and the TM, and coaxial with the focal plane, meeting the conditions of matching with the cold stop of the infrared detector. The tolerance analysis is also carried out, and the result shows that the system meets the requirements of practical fabrication and alignment.

摘要

具有宽探测范围、优异精度和高分辨率的红外成像系统在许多领域发挥着越来越重要的作用。与非制冷红外探测器相比,制冷红外探测器由于工作温度低,具有高精度、长探测距离和高信噪比的优点。本文设计了一种具有宽视场(FOV)、长焦距和大相对孔径的制冷离轴三镜中波红外(MWIR)光学系统。我们首先基于三阶赛德尔像差理论建立初始同轴三镜系统,然后使孔径光阑偏移以消除中心遮拦。在优化过程中,逐步扩大系统的视场,且不产生偏差以避免额外像差。为了增加优化自由度以提高系统的像差消除能力,我们在第三镜(TM)上应用多项式面。优化后,最终得到了一个视场为5.3×4.4、焦距为500mm且相对孔径为1/2的制冷离轴三镜MWIR光学系统。我们系统的成像质量优异,孔径光阑位于焦平面和第三镜之间,并与焦平面同轴,满足与红外探测器冷光阑匹配的条件。还进行了公差分析,结果表明该系统满足实际制造和装调的要求。

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