A new method to estimate the absorption coefficient for uncooled infrared detectors

M. Y. Tanrikulu, F. Çivitci, T. Akin
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引用次数: 5

Abstract

This paper introduces a new method to estimate the total absorption coefficient of uncooled infrared detectors. Current approaches in the literature model the infrared detectors as cascaded transmission lines representing the detector layers, and this model can easily be used to estimate the absorption coefficient if the detector has the same structure at every point. However, the state of the art uncooled infrared detectors do not have same structure at every point, making it not feasible to use this simple model. According to the proposed method, the detector structure is divided into subregions having different layer combinations, and the absorption coefficient of each subregion is calculated separately. Then, the area ratios of the subregions together with these coefficients are used in order to calculate the total absorption coefficient of the detector. As the estimation of the absorption coefficient for complex detector structures can easily be done, the absorption in the required part of the infrared spectrum can be optimized by adjusting the layer properties and layer thicknesses. This approach can be used both for single and double layer uncooled infrared detector structures.
一种估算非制冷红外探测器吸收系数的新方法
本文介绍了一种估算非制冷红外探测器总吸收系数的新方法。目前文献中的方法将红外探测器建模为级联传输线,表示探测器层,如果探测器在每个点具有相同的结构,则该模型可以很容易地用于估计吸收系数。然而,最先进的非冷却红外探测器在每个点上都没有相同的结构,使得使用这个简单的模型是不可行的。根据提出的方法,将探测器结构划分为具有不同层组合的子区域,并分别计算每个子区域的吸收系数。然后,利用子区域的面积比和这些系数计算探测器的总吸收系数。由于复杂探测器结构的吸收系数易于估计,因此可以通过调整层的性质和层的厚度来优化红外光谱中所需部分的吸收。该方法可用于单层和双层非冷却红外探测器结构。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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