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Primary aberrations of a thin lens with standard aspheres

机译:具有标准非球面镜的薄透镜的主像差

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Essence of this paper is to expand the results published concerning the primary aberrations of a thin lens. Starting with the contributions of the two refracting spherical surface, we have added the effects of considering each one as a rotationally symmetric polynomial asphere. As previous studies, we have worked with the bending variable (B) and the conjugate variable (C). In addition, two different media surround the lens and it has not the aperture stop in contact in order to get the effect of the aspherical surfaces on off-axis aberrations. As a result, the Seidel aberrations are third order polynomials in the variables B and C, except for the field curvature and chromatic aberrations, which preserve their form as they are obtained for spherical surfaces. The expressions can be used to incorporate the increase use of these surfaces in the predesign of not only simple but complex optical systems too, even to model axial GRIN lenses as it has been proposed recently. Moreover, modern algebra systems can make use of them to get an initial design for further optimisation.
机译:本文的实质是扩大有关薄透镜的基本像差发表的结果。从两个折射球面的贡献开始,我们添加了将每个视作旋转对称多项式非球面的效果。作为以前的研究,我们研究了弯曲变量(B)和共轭变量(C)。另外,两种不同的介质包围着镜头,并且没有使光圈挡块接触,以便获得非球面表面对离轴像差的影响。结果,Seidel像差是变量B和C中的三阶多项式,除了像场曲率和色差之外,它们在球形表面上获得时都保持其形式。这些表达式不仅可以用于简单,复杂的光学系统的预设计中,还可以用于增加这些表面的使用,甚至可以建模轴向GRIN透镜,如最近已经提出的那样。此外,现代代数系统可以利用它们来进行初步设计以进一步优化。

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