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一种新型微小视频卫星光学系统设计
引用本文:韩培仙,金光,钟兴.一种新型微小视频卫星光学系统设计[J].应用光学,2015,36(5):691-697.
作者姓名:韩培仙  金光  钟兴
作者单位:1.中国科学院大学,北京 100039;
基金项目:国家863计划 (2012AA121502)
摘    要:基于Ritchey-Chretien (R-C)光学系统,采用Zemax软件设计次镜为类曼金反射镜的折反射式光学系统。系统的焦距为3 000 mm,视场角为1,相对孔径为1/8,工作谱段为450 nm~900 nm。结果表明,截止频率为50 lp/mm处的MTF值为0.55,接近衍射极限,畸变小于0.022%。类曼金镜的非球面反射面与主镜构成R-C光学系统,消除了系统的球差和彗差,折射面分担次镜的光焦度,减小了非球面的非球面偏心率。类曼金反射镜的加入,将次镜非球面偏心率的平方由4.356减小到1.940,而且系统总长度由600 mm减小到550 mm。

关 键 词:光学设计    微小型视频卫星光学系统    R-C光学系统    类曼金反射镜    场镜

Design of new type of micro video-capable satellite optical system
Institution:1.University of Chinese Academy of Sciences,Beijing 100039,China;2.Changchun Institute of Optics,Fine Mechanics and Physics,CAS,Changchun 130033,China
Abstract:Based on the Ritchey-Chretien(R-C) system, a refractive/reflective system with a Margin-like mirror and 3 correcting lenses in front of the focal plane was designed with the help of Zemax software. It has a focal length of 3000mm, F number of 8, waveband of 450nm~900nm, and the field of view reaches 1. It is shown that the value of modulation transfer function(MTF) is higher than 0.55 at 50 lp/mm, the image quality reaches the diffraction limit,and the distortion is less than 0.022%. An R-C optical system is made up of the aspheric mirror of the Margin-like mirror and the primary mirror of the system without the spherical aberration and the coma aberration. The refractive surface of the Margin-like mirror shares the optical power of the secondary mirror, reducing the asphericity of the aspheric mirror. Results show that the Margin-like mirror can lessen the square asphericity of the secondary mirror from 4.356 to 1.940, and reduce the length of the system from 600 mm to 550 mm.
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