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Approach to investigating the spherical aberration variation with the object position in an aplanatic system

机译:研究非球面系统中物体位置的球差变化的方法

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In a general optical system, spherical aberration will arise when the on-axis position of an object is changed from its optimum position to another point. Induced spherical aberration can be used to compensate the aberration caused by inserting or removing a medium plate with any thickness that has a refractive index that differs from that of the original. To generate a degree of adequate aberration to balance the aberration from a thin layer, it is necessary to estimate the amount of arising aberration correctly when a point object deviates from its aberration-free position. We analytically induce the exact form of an arising spherical aberration with an on-axis object position for general optical systems that satisfy the Abbe sine condition and express a fourth-order approximation of that form using simple parameters that are conventionally used for the aberration of a thin lens. To verify the correctness of the proposed formula, a comparison between this analysis and simulation results is applied to several sample optical systems using commercial lens-design software.
机译:在一般的光学系统中,当物体的轴上位置从其最佳位置改变到另一个点时,就会出现球差。诱导的球差可用于补偿由于插入或卸下折射率不同于原始折射率的任何厚度的介质板而引起的像差。为了产生足够的像差度以平衡来自薄层的像差,当点物体偏离其无像差位置时,必须正确地估计产生的像差量。对于通常满足阿贝正弦条件的光学系统,我们通过分析得出具有轴上物体位置的球面像差的精确形式,并使用常规用于像差的简单参数来表示该形式的四阶近似。薄镜。为了验证所提出公式的正确性,使用商业镜头设计软件将这种分析结果与模拟结果之间的比较应用于多个示例光学系统。

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