Detection Performance Analysis of the Telescope considering Pointing Angle Command Error

Hojin Lee, Sang-Wook Lee
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Abstract

In this paper, the detection performance of the electro-optical telescopes which observes and surveils space objects including artificial satellites, is analyzed. To perform the Modeling & Simulation(M&S) based analysis, satellite orbit model, telescope model, and the atmospheric model are constructed and a detection scenario observing the satellite is organized. Based on the organized scenario, pointing accuracy is analyzed according to the Field of View(FOV), which is one of the key factors of the telescope, considering pointing angle command error. In accordance with the preceding result, detection possibility according to the pixel-count of the detector and the FOV of the telescope is analyzed by discerning detection by Signal-to-Noise Ratio(SNR). The result shows that pointing accuracy increases with larger FOV, whereas the detection probability increases with smaller FOV and higher pixel-count. Therefore, major specification of the telescope such as FOV and pixel-count should be determined considering the result of M&S based analysis performed in this paper and the operational circumstances.
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考虑指向角指令误差的望远镜探测性能分析
本文分析了用于观测和监视包括人造卫星在内的空间物体的光电望远镜的探测性能。为进行基于建模与仿真(M&S)的分析,构建了卫星轨道模型、望远镜模型和大气模型,并组织了观测卫星的探测场景。在组织场景的基础上,考虑指向角指令误差,根据望远镜的关键因素之一视场对指向精度进行了分析。根据上述结果,通过信噪比判别检测,分析了探测器像素数和望远镜视场的检测可能性。结果表明:视场越大,指向精度越高;视场越小,像素数越多,检测概率越高;因此,应结合本文基于M&S的分析结果和实际使用情况,确定望远镜的视场、像素数等主要指标。
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