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Optimization of three and four-element lens systems by minimizing the caustic merit function.

机译:通过最小化苛性函数来优化三元和四元镜片系统。

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摘要

For an imaging optical system, it is, in general, desirable to transform a collection of point sources of light into point images distributed over the focal plane with the appropriate magnification. In practice, this is achieved by varying the lens system parameters (radii of curvature, lens spacings, and indicies of refraction) such that the spread of a bundle of rays from each object point over the image plane has been minimized. Traditionally, optical design is performed by minimizing a merit function based on the spread of rays over the image plane or the deviation of the image wavefront from a reference spherical wavefront. In this study, the caustic surfaces, which are the loci of the wavefront centers of curvature, are used to construct a merit function that describe the spread of the caustic surfaces from an ideal image point. A generalized ray tracing algorithm has been used to calculate the principal radii of curvature of the wavefront for a bundle of rays passing through the optical system. From the generalized ray tracing algorithm, the caustic surfaces can be determined and provide important information about the structure of the image which is used in this study for lens design and analysis.; The caustic merit function has been used to optimize a large collection of three and four-element lenses. The performance of the optimized systems has been evaluated for different field angles by comparing the RMS blur circle radii with systems designed by conventional techniques. Results indicate that minimizing the caustic merit function reduces the RMS blur radii over the field of view and the total aberrations of the lens system when a few rays are traced through the system. During the optimization process, the caustic merit function has been minimized by varying the system parameters subject to the constraint of constant total focal length for the lens. A quasi-Newton algorithm has been used as the optimization technique.
机译:对于成像光学系统,通常期望以适当的放大倍数将点光源的集合转换成分布在焦平面上的点图像。实际上,这是通过改变透镜系统参数(曲率半径,透镜间距和折射指数)来实现的,从而使来自每个物点的一束光束的散布在图像平面上达到最小。传统上,光学设计是通过基于图像平面上的光线散布或图像波阵面与参考球面波阵面的偏差最小化优值函数来执行的。在这项研究中,苛性表面是波前曲率中心的位点,用于构建评价函数,该函数描述了理想表面上苛性表面的扩散。对于通过光学系统的一束光线,已使用通用的光线跟踪算法来计算波前的主曲率半径。从广义射线追踪算法,可以确定苛性表面,并提供有关图像结构的重要信息,该信息可用于本研究中的镜片设计和分析。苛性功函数已用于优化三元素和四元素镜片的大集合。通过将RMS模糊圆半径与通过常规技术设计的系统进行比较,已针对不同的视场角评估了优化系统的性能。结果表明,当通过系统跟踪少量光线时,将苛性函数最小化可减小整个视场的RMS模糊半径和透镜系统的总像差。在优化过程中,通过改变系统参数(在恒定的总焦距镜头的约束下),可以将苛性函数最小化。拟牛顿算法已用作优化技术。

著录项

  • 作者

    AL-Ahdali, Issam Hamed.;

  • 作者单位

    The University of Alabama at Birmingham.;

  • 授予单位 The University of Alabama at Birmingham.;
  • 学科 Physics Optics.
  • 学位 Ph.D.
  • 年度 1989
  • 页码 196 p.
  • 总页数 196
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 光学;
  • 关键词

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