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Aberration considerations in lens tolerancing

机译:镜头公差中的像差注意事项

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Often the tolerancing of an optical system is performed by treating the optical system as a black box in which the designer sets tolerances for perturbations and then runs a Monte Carlo analysis to determine the as-built performance. When the effects of the perturbations are not considered, the tolerances might result tighter than necessary, proper compensation might be missed, and manufacturing cost can be increased. By acquiring aberration sensitivity for each type of perturbation, an optical engineer can increase tolerances by ad hoc compensation. An aberration sensitivity evaluation can be performed quickly and can be incorporated into the initial lens design phase. A lens designer can find what surfaces or elements within the optical system will be problematic before any time-consuming Monte Carlo run is performed. In this paper we use aberration theory of plane symmetric systems to remove, to some useful extent, the black-box tolerancing approach and to provide some insights into tolerancing. The tolerance sensitivities that are analyzed are with respect to surface tilt, center thickness, index value, and radius. To analyze these perturbations, exact wavefront calculations are performed for the following aberrations: uniform astigmatism, uniform coma, linear astigmatism, distortion I, distortion II, spherical aberration, linear coma, quadratic astigmatism, and cubic distortion. We provide a discussion about how the aberration tolerancing analysis is useful.
机译:通常,光学系统的公差是通过将光学系统视为黑匣子来执行的,设计人员在该黑匣子中设置了摄动公差,然后运行蒙特卡洛分析来确定其实际性能。如果不考虑扰动的影响,公差可能会变得比必要的更严格,可能会丢失适当的补偿,并且会增加制造成本。通过获取每种摄动的像差灵敏度,光学工程师可以通过临时补偿来增加公差。像差灵敏度评估可以快速执行,并且可以合并到初始镜头设计阶段。镜片设计人员可以在执行任何耗时的蒙特卡洛测试之前,找出光学系统中哪些表面或元件会出现问题。在本文中,我们使用平面对称系统的像差理论在一定程度上消除了黑匣子容差方法,并提供了一些有关容差的见解。分析的公差灵敏度是关于表面倾斜度,中心厚度,折射率值和半径的。为了分析这些扰动,对以下像差执行精确的波前计算:均匀像散,均匀彗差,线性像散,畸变I,畸变II,球差,线性彗形,二次像散和三次畸变。我们提供有关像差公差分析如何有用的讨论。

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