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Track detection of high-velocity resident space objects in Low Earth Orbit
Institution:1. Institute of Space Sciences and Astronomy (ISSA), University of Malta, Msida MSD 2080, Malta;2. Department of Physics, University of Oxford, Oxford OX1 3RH, United Kingdom;3. Istituto Nazionale di Astrofisica – Istituto di Radioastronomia (INAF), Via P. Gobetti, Bologna 101 - 40129, Italy
Abstract:The world’s economy has become heavily dependent on the services provided by satellites. With the exponential increase in satellite launches, the population of defunct or inactive hardware in space has grown substantially. This is especially true in sensitive orbits such as the Low Earth Orbit (LEO) and Geostationary Earth Orbit (GEO) regimes. These objects, collectively known as orbital debris, can reach speeds of up to 28 000km h?1 in LEO. At these orbital speeds, even the smallest of objects can pose a considerable threat to operational satellites or astronauts. This makes the monitoring, and detection, of these objects of the utmost importance. This work describes the latest detection strategy used in one of Europe’s largest Space Situational Awareness (SSA) installation; the BIstatic RAdar for LEo Survey (BIRALES) space debris radar. We present a novel bottom-up approach that makes use of single-linkage clustering to identify faint radar streaks in spectrogram data. Tests on synthetic data have shown that the detection strategy presented in this study obtains a higher detection rate when it is compared against existing methods. Unlike other approaches, this detection strategy, using the Multi-beam streak detection strategy (MSDS) algorithm, was still able to recall 90% of the track information at an Signal-to-Noise Ratio (SNR) of 2dB.
Keywords:Track detection  Space debris  Radar  Remote sensing
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