Tang Yi, Zheng Cheng, Jia Huiping, Nan Yibing, Li Fei, Xue Wei
Appl Opt. 2015 Mar 20;54(9):2507-13. doi: 10.1364/AO.54.002507.
The structure of an astigmatism-corrected Czerny-Turner imaging spectrometer will produce the focal length difference between sagittal rays and tangential rays, which contributes to the magnification difference in the spectral and spatial dimensions of the images. In this paper, the common characteristics of two optical path structures based on the Czerny-Turner imaging spectrometer to correct astigmatism (using a cylindrical and a toroidal mirror) are discussed. The magnification differences in the spectral and spatial dimensions of the image when the gratings are at zero-order and first-order diffraction and the influence of image magnification of different wavelengths are analyzed. The correction formula, methods of anamorphosis, and their common characteristics are given as well. The validity of the correction formula of anamorphosis is verified with theoretical calculation, ray tracing simulation, and experimental measurements with the imaging spectrometers. Meanwhile, this method is useful for the anamorphosis correction of an off-axis dispersion imaging spectrometer in other operating conditions of collimated light.
像散校正 Czerny-Turner 成像光谱仪的结构会产生弧矢光线和子午光线之间的焦距差,这导致了图像在光谱和空间维度上的放大率差异。本文讨论了基于 Czerny-Turner 成像光谱仪校正像散的两种光路结构(使用柱面镜和 toroidal 镜)的共同特性。分析了光栅处于零阶和一阶衍射时图像在光谱和空间维度上的放大率差异以及不同波长图像放大率的影响。还给出了变形校正公式、变形方法及其共同特性。通过理论计算、光线追迹模拟以及成像光谱仪的实验测量验证了变形校正公式的有效性。同时,该方法对于其他准直光工作条件下的离轴色散成像光谱仪的变形校正也很有用。