PyBIRALES: A Radar Data Processing Backend for the Real-Time Detection of Space Debris

Author:

Cutajar D.1ORCID,Magro A.1,Borg J.1,Adami K. Z.12,Bianchi G.3,Pupillo G.3,Mattana A.3,Naldi G.3,Bortolotti C.3,Perini F.3,Lama L.3,Schiaffino M.3,Roma M.3,Maccaferri A.3,Lizia P. Di4,Massari M.4,Losacco M.4

Affiliation:

1. Institute of Space Sciences and Astronomy (ISSA), University of Malta, Malta

2. Department of Physics, University of Oxford, Oxford, OX1 3RH, UK

3. Istituto Nazionale di Astrofisica, Istituto di Radioastronomia, Via P. Gobetti 101, 40129 Bologna, Italy

4. Department of Aerospace Science and Technology, Politecnico di Milano, Via G. La Masa 34, 20156 Milano, Italy

Abstract

The growing population of artificial satellites in near-Earth orbit has made the monitoring of orbital debris objects ever more important. Orbital debris objects pose a threat to these satellites as their orbit cannot be changed in order to avoid a collision. In recent years, the European Space Agency (ESA)’s Space Surveillance and Tracking (SST) programme has been assisting national institutions in the upgrading of their space debris detection and monitoring capabilities. One of the latest such systems within this programme is the BIRALES space surveillance system based in Italy. The receiving antenna is a radio telescope that is made up of 32 receivers which are placed on eight parabolic cylindrical reflectors of the North–South arm of the Istituto Nazionale di Astrofisica (INAF)’s Northern Cross. This work introduces a new software backend which was developed for this novel space debris sensor. The system was designed to be a fast, highly configurable software backend for the radio telescope’s acquisition and processing system and whose monitoring and control can be realized by a simple front-end web-based application. The real-time detection of Resident Space Object (RSO) is an important prerequisite for such a system as it gives the operator an immediate feedback loop on any detections whilst keeping the storage requirements at a minimum given that there is no need to save the raw data. The detection of high-velocity objects is achieved by means of a specially developed data processing pipeline that uses the received raw antenna voltages to generate a number of beams, collectively known as a multipixel, that cover the Field of View (FoV) of the instrument. The trajectory of the detected objects is determined by considering the illumination sequence within this multipixel. The initial results on known objects represent the first steps in extending the growing network of European SST systems.

Funder

European Commission Framework Programme H2020 and Copernicus, SST Space Surveillance and Tracking

Publisher

World Scientific Pub Co Pte Lt

Subject

Astronomy and Astrophysics,Instrumentation

Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Track detection of high-velocity resident space objects in Low Earth Orbit;Advances in Space Research;2023-02

2. Digitizing MEXART — System Overview and Verification;Journal of Astronomical Instrumentation;2021-12

3. The Design and Development of a GPU-accelerated Radar Simulator for Space Debris Monitoring;2021 5th High Performance Computing and Cluster Technologies Conference;2021-07-02

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