A Space Debris-Dedicated Channel for the P-Band Receiver of the Sardinia Radio Telescope: A Detailed Description and Characterization

• Published in: IEEE antennas & propagation magazine Vol. 62; no. 3; pp. 45 - 57
• Main Authors: Muntoni, Giacomo, Schirru, Luca, Montisci, Giorgio, Pisanu, Tonino, Valente, Giuseppe, Ortu, Pierluigi, Concu, Raimondo, Melis, Andrea, Urru, Enrico, Saba, Andrea, Gaudiomonte, Francesco, Bianchi, Germano
• Format: Magazine Article
• Language: English
• Published: New York IEEE 01-06-2020; The Institute of Electrical and Electronics Engineers, Inc. (IEEE)
• Subjects: Antennas; Atmospheric entry; Echoes; Monitoring; Planetary orbits; Radar; Radio astronomy; Radio telescopes; Space debris; Space stations; Space surveillance; Space vehicles
• ISSN: 1045-9243; 1558-4143
• DOI: 10.1109/MAP.2019.2943274

Space debris (SD) is an important problem for space operations and a hot topic for space surveillance research. A structured network of radar sensors is available worldwide, offering vital information about debris status. Recently, the Sardinia Radio Telescope (SRT), a 64-m dish located in Sardinia, Italy, was introduced in the European plan for SD monitoring. Because the SRT is devoted to radio astronomy applications and is not optimized for SD echo detection, the need for an SD-dedicated channel has emerged. In this article, we present a detailed description and characterization of the new P-band receiving chain for SRT's space debris-monitoring purposes. As a test of its capabilities, the new channel was used to detect the echoes that emanated from the Chinese space station Tiangong-1 when it reentered Earth's atmosphere on its latest mission.