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Computer-aided Alignment of off-axis three-mirror imaging spectrometer system

机译:轴外三镜像谱仪系统的计算机辅助对准

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The space camera is one of the most advanced optical equipments in obtaining earth surface information from space. With the development of the optical design, manufacture and alignment technology, the performance of the optical camera is moving forward quickly. In space-to-ground remote sensing field, the resolution of ground remote sensing images have become higher and higher. Off-axis three-mirror system becomes an advanced optical system structure of space camera at present, because of its merits of large field, long focal length, no obstruction, high modulated transfer function, wide spectrum, good image quality, small cubage and light weight, etc. As it is difficult to align and test, the alignment of off-axis three mirror system is time-consuming, so it is important and necessary of studying the computer-aided alignment of the complex optical system. Aiming at cutting the time of alignment, Computer-aided alignment technology is applied to this system. According to relation between fringe Zernike coefficient and Seidel aberration, wavefront aberration in the exit pupil of optical system is instead with fringe Zernike coefficient. A series of Zernike coefficient expressing the incorrect parameters of system are obtained by using multi-fields ZYGO interferometer auto-collimating interference test, which are transformed into geometric aberrations as the corrected object. Incorrect parameters of the system are determined by sensitivity matrix resulted from optical design software. These incorrect parameters are defined to be variables; the Zernike coefficient are defined to be the optimized target in merit function. The system is optimized by applying optical design software to receive the incorrect parameters result. Consequently, the adjusted result is brought into the optical design software to verify the right selection of incorrect parameters. The practical experiments are also given, result with RMS value lower than 0.04λ is acquired by using this alignment technology which has proved the effectiveness of above methodology of guiding-alignment.
机译:空间照相机是从空间获得地球表面信息中最先进的光学设备之一。随着光学设计,制造和对准技术的发展,光学相机的性能快速向前移动。在空对地遥感场中,地面遥感图像的分辨率变得越来越高。轴外三镜系统成为目前太空摄像机的先进光学系统结构,由于其大场,焦距长,无阻塞,高调制传递函数,宽度,良好的图像质量,小立方和光线重量等。由于难以对准和测试,偏离轴三镜系统的对准是耗时的,因此研究复杂光学系统的计算机辅助对准是重要的,需要的。旨在减少对准时间,计算机辅助对准技术应用于该系统。根据条纹Zernike系数和Seidel像差之间的关系,光学系统出口瞳孔中的波前像差是与边缘Zernike系数的。通过使用多场Zygo干涉仪自组合干扰测试获得了一种表达系统不正确的系统参数的Zernike系数,其作为校正对象转换成几何像差。系统的参数不正确通过光学设计软件引起的灵敏度矩阵来确定。这些不正确的参数被定义为变量; Zernike系数被定义为优选函数中的优化目标。通过应用光学设计软件来接收不正确的参数结果来优化系统。因此,调整后的结果被引入光学设计软件,以验证正确的参数选择。还给出了实际实验,通过使用该对准技术获得了低于0.04λ的RMS值的结果,这已经证明了引导对准方法的高度方法的有效性。

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