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Primary aberrations of a thin lens with standard aspheres

机译:具有标准非球面的薄透镜的主要像差

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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:本文的本文是扩展关于薄镜头的主要像差的结果。从两个折射球面的贡献开始,我们已经增加了将每个作为旋转对称多项式购物中心的效果。作为之前的研究,我们已经使用了弯曲变量(B)和共轭变量(C)。另外,两个不同的介质围绕透镜,并且它没有孔停止接触,以便在轴外像差上获得非球面表面的效果。结果,Seidel像差是变量B和C中的第三阶多项式,除了场曲率和色差,它们保持其形状,因为它们是用于球形表面的形状。表达式可用于在不仅简单但复杂的光学系统的预测中加入这些表面的增加使用,甚至可以在最近提出的模型轴流镜片。此外,现代代数系统可以利用它们来获得初始设计以进一步优化。

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