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An analytical method of vector diffraction for focusing optical systems with Seidel aberrations II: Astigmatism and coma

机译:具有Seidel像差的聚焦光学系统的矢量衍射分析方法II:像散和彗差

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In this paper, a method developed by the author is used to study the image formation in various aplanntio systems of high Fresnel numbers and circular pupils with Seidel (fourth order) aberrations, particularly the astigmatic and comatic aberrations. The theory developed here is based on Richards and Wolf's formulation of the vector diffraction theory of focusing systems. The electric and magnetic vectors are derived to reflect the asymmetry of the surface of the wavefront with respect to the optical axis. The unit normal to the surface of an aberrated wavefront is expressed as the sum of two vectors. One vector is in the direction of the unit normal to the ideal Gaussian sphere, while the other, after a suitable normalization, characterizes the unit normal's deviation from the unit normal to the ideal Gaussian sphere. The components of the electric and magnetic vectors are then expressed in integral form. In the end, the integrals are evaluated in terms of the products of Gegenbauer polynomials of the first kind and spherical Besael functions; both of these functions are evaluated by summing finite series. We present results for systems with ustigmatic and comatic aberrations and provide information about the location of the diffraction foci and Strehl intensity. We also show that in the limit, the theory presented here provides solutions to aberration-free systems and systems with the Seidel aberrations of the first kind, and in cases when the numerical aperture is small, the results are in agreement with the scalar theory for large Fresnel numbers.
机译:在本文中,作者开发了一种方法,用于研究各种菲涅尔数高的圆形透镜和具有Seidel(四阶)像差(特别是像散和彗差)的圆形瞳孔在各种平面系统中的成像。这里发展的理论是基于理查兹和沃尔夫对聚焦系统矢量衍射理论的表述。推导出电和磁矢量以反映波前表面相对于光轴的不对称性。垂直于像差波前表面的单位表示为两个向量的总和。一个向量是在垂直于理想高斯球体的单位法线方向上,而另一向量在经过适当的归一化后,可以表征单位法向与从单位法向到理想高斯球体的偏差。电和磁矢量的分量然后以整数形式表示。最后,根据第一类Gegenbauer多项式与球形Besael函数的乘积评估积分。这两个函数都是通过对有限序列求和而求出的。我们介绍了具有散光和彗形像差的系统的结果,并提供了有关衍射焦点和Strehl强度的信息。我们还表明,在极限条件下,此处介绍的理论为无像差系统和第一类塞德尔像差的系统提供了解决方案,并且在数值孔径较小的情况下,结果与标量理论相符。大菲涅耳数。

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