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Optical design of diffractive telescope system based on off-axis three mirror

机译:基于离轴三镜的衍射望远镜系统的光学设计

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Diffractive telescope has the advantages of lightweight and loose tolerance, so it can become the next generation spacetelescope. In order to realize no central obscuration, compact structure and large field of view (FOV), the off-axis threemirror is used as eyepiece in diffractive telescope system. According to the Schupmann’s achromatic theory, an opticaldesign example of diffractive telescope with 0.8m aperture of objective lens, 0.46~0.54μm spectral bandwidth and 0.08°FOV is presented. By using the function of coordinate break in optical design software ZEMAX, an unobscureddiffractive telescope system based on off-axis three mirror eyepiece is realized. After optimized original structureparameters, the diffractive telescope system has a good performance with 39.1m short total length. Here, at the spatialfrequency of 50lp/mm, the values of modulation transfer function (MTF) within full FOV are greater than 0.574.Furthermore, the values of RMS radius are less than airy radius diameter. The optimized results clearly show that thesystem is achromatic and near diffraction limited imaging quality.
机译:衍射望远镜具有轻质和宽松耐受性的优点,因此它可以成为下一代空间望远镜。为了实现没有中央遮挡,结构紧凑和大视野(FOV),轴外三镜子用作衍射望远镜系统的目镜。根据Schupmann的消色氛理论,光学衍射望远镜的设计实例,物镜0.8M光圈,0.46〜0.54μm光谱带宽和0.08°举办了FOV。通过使用光学设计软件zemax的坐标中断的功能,一个视野开阔实现了基于轴外轴三镜像仪的衍射望远镜系统。优化原始结构后参数,衍射望远镜系统的性能良好,总长度39.1米。在这里,在空间50LP / mm的频率,全FOV内的调制传递函数(MTF)的值大于0.574。此外,RMS半径的值小于通风半径直径。优化的结果清楚地表明了系统是消色差,近衍射有限的成像质量。

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