Digital Tracking Cloud Distributed Architecture for Detection of Faint NEAs

Roxana E. Sichitiu, M. Frîncu, Ovidiu Vaduvescu
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引用次数: 0

Abstract

There is an exponential volume of captured images, millions of captures taken every night being processed and scrutinized. Big Data analysis has become essential for the study of the solar system, discovery and orbital knowledge of the asteroids. This analysis often requires more advanced algorithms capable of processing the available data and solve the essential problems in almost real time. One such problem that needs very rapid investigation involves the detection of Near Earth Asteroids(NEAs) and their orbit refinement which should answer the question "will the Earth collide in the future with any hazardous asteroid?". This paper proposes a cloud distributed architecture meant to render near real-time results, focusing on the image stacking techniques aimed to detect very faint moving objects, and pairing of unknown objects with known orbits for asteroid discovery and identification.
微弱近地天体探测的数字跟踪云分布式架构
被捕获的图像呈指数级增长,每天晚上都有数百万张被处理和审查的图像。大数据分析对于太阳系的研究、小行星的发现和轨道知识已经变得至关重要。这种分析通常需要更先进的算法,能够处理可用数据并几乎实时地解决基本问题。其中一个需要迅速调查的问题涉及到探测近地小行星(NEAs)及其轨道修正,这应该回答“地球将来会与任何危险的小行星相撞吗?”这个问题。本文提出了一种旨在呈现近实时结果的云分布式架构,重点关注旨在检测非常微弱的运动物体的图像堆叠技术,以及用于小行星发现和识别的未知物体与已知轨道的配对。
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