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Experimental determination of paraxial ray transfer matrices and cardinal points of complex optical systems by means of finite conjugate imaging

机译:有限共轭成像实验确定复杂光学系统近轴射线传递矩阵和基点

摘要

The Lineate Imaging Near-ultraviolet Spectrometer (LINUS) uses three complex lens systems to focus an image from distances on the order of several kilometers onto the image intensifier of an ultraviolet camera. These images can then be analyzed to characterize the atmospheric distribution and concentration of sulfur dioxide (SO2). The lenses purchased for LINUS were corrected for spherical aberrations but due to the lack of detailed knowledge about the lenses their chromatic aberrations could not be readily predicted. The project presented in this thesis was performed with the goal of experimentally quantifying the chromatic aberrations of each of LINUSαs lens systems. The matrix method of representing paraxial optical systems was used to determine relationships between object and image distances for different lens systems. These relationships were manipulated to give equations for the matrix elements of the lens system in terms of readily measurable parameters. Once the matrix elements are known, all of the cardinal points can be readily predicted. This method will, in theory, quantify the chromatic aberrations of each lens system. The method was validated with simulations and measurements taken on a lens of known focal length. Finally, the LINUS lens systems were characterized at 220, 300, 334, and 370 nm.
机译:线性成像近紫外光谱仪(LINUS)使用三个复杂的透镜系统,可将几千米距离的图像聚焦到紫外相机的图像增强器上。然后可以分析这些图像以表征大气分布和二氧化硫(SO2)的浓度。为LINUS购买的镜头已针对球差进行了校正,但是由于缺乏有关镜头的详细知识,因此无法轻松预测其色差。本论文中提出的项目的目的是通过实验量化每个LINUS镜头系统的色差。代表近轴光学系统的矩阵方法用于确定不同透镜系统的物距和像距之间的关系。对这些关系进行操作,以根据易于测量的参数给出镜头系统矩阵元素的方程式。一旦知道了矩阵元素,就可以容易地预测所有基点。从理论上讲,该方法将量化每个镜头系统的色差。通过在已知焦距的镜头上进行的仿真和测量验证了该方法的有效性。最后,LINUS透镜系统的特征是220、300、334和370 nm。

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    Blackwell Jerry S.;

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  • 年度 2001
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