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Thermal imager non-uniformity sources modeling

机译:热成像仪非均匀性资源建模

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摘要

The raw output of a generic infrared vision system, based on staring arrays, is spatially not uniform. This spatial noise can be much greater than the system NETD, and determines a strong drop in system performance. Therefore we need to model all system non-uniformity (NU) sources to highlight the parameters that should be controlled by optical and mechanical design, the ones depending on the focal plane array and those that can be corrected in post-processing. In this paper, we identify the main NU sources (optical relative irradiance, housing straylight, detector pixel-pixel differences and non linearity), we show how to model these sources and how they are related to the design and physical parameters of the system. We then describe the total signal due to these sources at the detector output. Applying different NUC algorithms to this signal, the final results on the image can be simulated finding a proper correction algorithm. At the end we show the agreement between the model with the experimental data taken on a real system. Changing a limited set of parameters, this model can be applied to many third generation thermal imager configurations.
机译:基于凝视阵列的通用红外视觉系统的原始输出在空间上不均匀。这种空间噪声可以大于系统NetD,并确定系统性能的强大下降。因此,我们需要建模所有系统不均匀性(NU)源以突出显示应由光学和机械设计控制的参数,根据焦平面阵列和可以在后处理中校正的那些。在本文中,我们识别主元源(光学相对辐照度,外壳串行灯,探测器像素 - 像素差异和非线性),我们展示了如何建模这些来源以及它们与系统的设计和物理参数有关。然后,我们描述了由于探测器输出的这些源导致的总信号。将不同的NUC算法应用于该信号,可以模拟图像上的最终结果可以确定找到适当的校正算法。最后,我们展示了模型与实际系统上的实验数据之间的协议。更改有限的参数集,该模型可以应用于许多第三代热成像器配置。

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