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A Probabilistic Approach of Space Objects Detection from Non-resolved Optical Observation

机译:非分辨光学观察空间对象检测的概率方法

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Non-resolved optical space imagery is usually heavily noisy with many field stars clutter. Both phenomena may impair the success of detecting space objects. There is hence often a need for efficient and robust preprocessing techniques to filter the objects of interest. In this paper, we propose a novel probabilistic approach for denoising, filtering and detecting space objects by using non-resolved optical images. In particular, as pixels of background and foreground in an image obey different probabilistic distributions, we propose a corresponding clustering algorithm to distinguish foreground objects from background noises. Furthermore, a near real-time finer classification for foreground objects is achieved by further exploring the metric on the filtered pixel set. Various modes (sidereal tracking/stationary) and different types of objects (GEO/LEO) are unified into this general framework. We verify the effectiveness and robustness of our algorithm by detecting and filtering space objects in CCD telescopic sequential imageries under different experimental conditions.
机译:非分辨光学空间图像通常严重嘈杂,许多田间恒星杂乱无章。这两种现象都可能损害检测空间物体的成功。因此,需要有效地过滤感兴趣的对象的高效和鲁棒预处理技术。在本文中,我们提出了一种新的概率方法,用于通过使用不分辨的光学图像去噪,过滤和检测空间物体。特别是,作为图像遵循不同概率分布的背景和前景的像素,我们提出了一种相应的聚类算法来区分从背景噪声中的前景对象。此外,通过进一步探索过滤的像素集的度量来实现前景对象的近实时较好分类。各种模式(恒星跟踪/静止)和不同类型的物体(Geo / Leo)统一到这一总体框架中。我们通过在不同实验条件下检测和过滤和过滤CCD伸缩顺序成像中的空间对象来验证算法的有效性和鲁棒性。

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