Zoom lens with large aperture and long focal length in the integration system of detection and recognition

Rui Yao, Xu-yang Li, Zixuan Ma, Zhi-guang Ren, Nanqing Chu
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Abstract

This paper designs an integrated optical system for detection and recognition. The system combines the R-C (Ritchey-Chretien optics) system and the zoom structure. The R-C mirror design of the initial structure of the system is completed by calculation of theory. Then, use the zoom theory to complete the design of the two zoom positions. The two zoom positions respectively realize the detection and identification of space debris. The F numbers are 5.86 and 11. The field of view angles are 2.83°and 0.6°. It works in band of 400-750nm. The system has an entrance pupil diameter of 300mm. The detection position can detect space debris with a brightness of 13 magnitude stars, with focal length of 1760mm; the recognition position’s modulation transfer function is greater than 0.6 at the Nyquist frequency of 33.33lp/mm, with the focal length of 3300mm. The zoom theory is well applied in the integrated detection and recognition system.
在检测识别集成系统中采用大光圈长焦距变焦镜头
本文设计了一种用于检测和识别的综合光学系统。该系统结合了R-C(里奇-克雷蒂安光学)系统和变焦结构。通过理论计算完成了系统初始结构的R-C反射镜设计。然后,运用变焦理论完成了两个变焦位置的设计。这两个变焦位置分别实现了空间碎片的检测与识别。F值是5.86和11。视场角度分别为2.83°和0.6°。它工作在400-750nm波段。该系统的入口瞳孔直径为300毫米。探测位置可探测亮度为13等恒星的空间碎片,焦距为1760mm;在奈奎斯特频率为33.33lp/mm时,识别位置的调制传递函数大于0.6,焦距为3300mm。变焦理论在综合检测识别系统中得到了很好的应用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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