Analysis of influence of long back focal length on athermal design based on infrared multispectral camera
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Published:2021
Issue:18
Volume:70
Page:184201
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ISSN:1000-3290
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Container-title:Acta Physica Sinica
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language:
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Short-container-title:Acta Phys. Sin.
Author:
Xu Huan-Yao,Xu Liang,Shen Xian-Chun,Xu Han-Yang,Sun Yong-Feng,Liu Wen-Qing,Liu Jian-Guo, ,
Abstract
Under different ambient temperatures, the thermal aberration certainly affects the imaging quality of infrared multi-spectral camera. Therefore, an athermalized model of infrared multi-spectral cameras is established, and in this model the ambient infrared multispectral camera is equivalent to a separated dual-lens optical system. In the case of the fixed focal length, the influence of the back focal length on the change of the focal power of the front lens and back lens is analyzed. Now, the variation range of the front and rear lens interval is assumed to be restricted. When the back focal length is smaller than the focal length, the ratio of the absolute value of the focal power of the front lens to the absolute value of the focal power of the back lens decreases with the back focal length increasing. The material of the front lens and the back lens have a longer interval on the thermogram. When the back focal length is greater than the focal length, the scenario becomes exactly opposite. Combined with the judgment method of the positive value and negative value of the focal power on the thermogram, the selection range of materials is constrained by the positive value, negative value, and absolute value of focal power, thus realizing the rapid selection of the optical materials. This method is used to design an athermalized infrared multispectral camera with a waveband of 8–14 μm, a focal length of 50 mm, and an <i>F</i> number of 1.4 in a range from –40 ℃ to +60 ℃. Through the simulation analysis, the value of the athermalized infrared multispectral camera, at the Nyquist frequency of 30 lp/mm reaches 0.39, which is close to the diffraction limit; the root mean square radius of the diffuse spot is smaller than the Airy spot radius of 19.17 μm; the axial aberration is less than 0.02 mm, and the design results show that this method can make the long back-focus infrared optical system maintain stable imaging quality in a large temperature range. The SF<sub>6</sub> gas is detected experimentally, and the experimental results demonstrate the excellent optical performance of the system.
Publisher
Acta Physica Sinica, Chinese Physical Society and Institute of Physics, Chinese Academy of Sciences
Subject
General Physics and Astronomy
Reference22 articles.
1. Xu L, Gao M G, Liu J G, Jiao Y, Feng M C, Tong J J, Li S 2013 Remote Sensing of Clouds and the Atmosphere XVII; and Lidar Technologies, Techniques, and Measurements for Atmospheric Remote Sensing VIII Edinburgh, United Kingdom, September 24–27, 2012 p85340M 2. Yin H, Sun Y W, Liu C, Zhang L, Lu X, Wang W, Shan C G, Hu Q H, Tian Y, Zhang C X, Su W J, Zhang H F, Palm M A, Notholt J, Liu J G 2019 Opt. Express 27 A1225 3. Yin H, Sun Y W, Liu C, Lu X, Smale D, Blumenstock T, Nagahama T, Wang W, Tian Y, Hu Q H, Shan C G, Zhang H F, Liu J G 2020 Opt. Express 28 8041 4. Yin H, Sun Y, Song Z, Liu C, Wang W, Shan C, Zha L 2021 Remote Sens. 13 791 5. Gay L, Alazarine A, Favier S, Blanchard S 2018 19th Meeting of the Chemical, Biological, Radiological, Nuclear, and Explosives (CBRNE) Sensing as part of the SPIE Defense and Commercial Sensing (DCS) Symposiμm Orlando, United States of America, April 16–18, 2018 p106290X
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