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Simulation of resident space objects detection from space-based optical imaging

机译:基于天基光学成像的常驻空间物体检测的仿真

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The United States Space Surveillance Network catalogs around 23,000 Resident Space Objects (RSOs). The completeness of their coverage of the true RSO population decreases gradually with object size and radar reflectivity. While the population of cm level space debris is poorly represented in the catalogs these space bullets can cause severe damage to satellites and spacecrafts in addition to being likely much more numerous than larger pieces. This research project focuses on the ability to peek into this debris population using space-based high sensitivity, fast frame rate, wide field visible imaging from low Earth orbit.The simulator developed focuses on a LEO to LEO (sensor to RSO) scenario and the capacity to constrain their orbit trajectory. In the Matlab simulator, a simple specular/diffuse sphere model is used for the debris in order to generate the object's apparent magnitude for any sun-debris-observer arrangement. Satellite and debris relative velocities and orbits are also considered in order to determine the length of the streak left by the debris on any given exposure sequence and the number of photons per pixel. The exact timing, position, length and orientation of the streak contains information constraining the object's orbit. The generation of representative star backgrounds matched to the sensor high sensitivity is also an important part of the simulator since it affects the effective limiting sensitivity to faint transiting source. This simulator allows us to trade various sensor parameters in order to optimize the camera design. The conclusion from this work contribute to the global effort in Space Situational Awareness (SSA) by assessing the impact of including space based optical imagery in the detection mix.
机译:美国太空监视网络对大约23,000个常驻空间物体(RSO)进行了编目。随着目标尺寸和雷达反射率的提高,它们对真实RSO总体覆盖的完整性会逐渐降低。尽管目录中厘米级空间碎片的数量很少,但是这些空间子弹除了可能比大型碎片数量更多外,还会对卫星和航天器造成严重破坏。该研究项目的重点是使用基于空间的高灵敏度,快速帧频,低地球轨道的宽视场可见成像来窥视这些碎片群的能力。模拟器的开发重点是LEO到LEO(传感器到RSO)的场景以及约束其轨道轨迹的能力。在Matlab仿真器中,将简单的镜面/漫射球体模型用于碎片,以便为任何太阳碎片观察者布置生成对象的视在大小。还应考虑卫星和碎片的相对速度和轨道,以便确定在任何给定的曝光序列上碎片留下的条纹的长度以及每个像素的光子数。条纹的确切时间,位置,长度和方向包含约束对象轨道的信息。与传感器高灵敏度相匹配的代表性恒星背景的生成也是模拟器的重要组成部分,因为它会影响对微弱过渡源的有效极限灵敏度。该模拟器使我们可以交易各种传感器参数,以优化相机设计。这项工作得出的结论是,通过评估在探测混合物中包括基于空间的光学图像的影响,有助于全球空间态势感知(SSA)方面的工作。

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