A Tri-Band Cooled Receiver for Geodetic VLBI
This paper shows a simultaneous tri-band (S: 2.2-2.7 GHz, X: 7.5-9 GHz and Ka: 28-33 GHz) low-noise cryogenic receiver for geodetic Very Long Baseline Interferometry (geo-VLBI) which has been developed at Yebes Observatory laboratories in Spain. A special feature is that the whole receiver front-end...
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Published in | Sensors (Basel, Switzerland) Vol. 21; no. 8; p. 2662 |
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Main Authors | , , , , , , , , , , , , , , , , |
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10.04.2021
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Abstract | This paper shows a simultaneous tri-band (S: 2.2-2.7 GHz, X: 7.5-9 GHz and Ka: 28-33 GHz) low-noise cryogenic receiver for geodetic Very Long Baseline Interferometry (geo-VLBI) which has been developed at Yebes Observatory laboratories in Spain. A special feature is that the whole receiver front-end is fully coolable down to cryogenic temperatures to minimize receiver noise. It was installed in the first radio telescope of the
(RAEGE) project, which is located in Yebes Observatory, in the frame of the VLBI Global Observing System (VGOS). After this, the receiver was borrowed by the Norwegian Mapping Autorithy (NMA) for the commissioning of two VGOS radiotelescopes in Svalbard (Norway). A second identical receiver was built for the Ishioka VGOS station of the Geospatial Information Authority (GSI) of Japan, and a third one for the second RAEGE VGOS station, located in Santa María (Açores Archipelago, Portugal). The average receiver noise temperatures are 21, 23, and 25 Kelvin and the measured antenna efficiencies are 70%, 75%, and 60% in S-band, X-band, and Ka-band, respectively. |
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AbstractList | This paper shows a simultaneous tri-band (S: 2.2-2.7 GHz, X: 7.5-9 GHz and Ka: 28-33 GHz) low-noise cryogenic receiver for geodetic Very Long Baseline Interferometry (geo-VLBI) which has been developed at Yebes Observatory laboratories in Spain. A special feature is that the whole receiver front-end is fully coolable down to cryogenic temperatures to minimize receiver noise. It was installed in the first radio telescope of the
(RAEGE) project, which is located in Yebes Observatory, in the frame of the VLBI Global Observing System (VGOS). After this, the receiver was borrowed by the Norwegian Mapping Autorithy (NMA) for the commissioning of two VGOS radiotelescopes in Svalbard (Norway). A second identical receiver was built for the Ishioka VGOS station of the Geospatial Information Authority (GSI) of Japan, and a third one for the second RAEGE VGOS station, located in Santa María (Açores Archipelago, Portugal). The average receiver noise temperatures are 21, 23, and 25 Kelvin and the measured antenna efficiencies are 70%, 75%, and 60% in S-band, X-band, and Ka-band, respectively. This paper shows a simultaneous tri-band (S: 2.2–2.7 GHz, X: 7.5–9 GHz and Ka: 28–33 GHz) low-noise cryogenic receiver for geodetic Very Long Baseline Interferometry (geo-VLBI) which has been developed at Yebes Observatory laboratories in Spain. A special feature is that the whole receiver front-end is fully coolable down to cryogenic temperatures to minimize receiver noise. It was installed in the first radio telescope of the Red Atlántica de Estaciones Geodinámicas y Espaciales (RAEGE) project, which is located in Yebes Observatory, in the frame of the VLBI Global Observing System (VGOS). After this, the receiver was borrowed by the Norwegian Mapping Autorithy (NMA) for the commissioning of two VGOS radiotelescopes in Svalbard (Norway). A second identical receiver was built for the Ishioka VGOS station of the Geospatial Information Authority (GSI) of Japan, and a third one for the second RAEGE VGOS station, located in Santa María (Açores Archipelago, Portugal). The average receiver noise temperatures are 21, 23, and 25 Kelvin and the measured antenna efficiencies are 70%, 75%, and 60% in S-band, X-band, and Ka-band, respectively. This paper shows a simultaneous tri-band (S: 2.2–2.7 GHz, X: 7.5–9 GHz and Ka: 28–33 GHz) low-noise cryogenic receiver for geodetic Very Long Baseline Interferometry (geo-VLBI) which has been developed at Yebes Observatory laboratories in Spain. A special feature is that the whole receiver front-end is fully coolable down to cryogenic temperatures to minimize receiver noise. It was installed in the first radio telescope of the Red Atlántica de Estaciones Geodinámicas y Espaciales (RAEGE) project, which is located in Yebes Observatory, in the frame of the VLBI Global Observing System (VGOS). After this, the receiver was borrowed by the Norwegian Mapping Autorithy (NMA) for the commissioning of two VGOS radiotelescopes in Svalbard (Norway). A second identical receiver was built for the Ishioka VGOS station of the Geospatial Information Authority (GSI) of Japan, and a third one for the second RAEGE VGOS station, located in Santa María (Açores Archipelago, Portugal). The average receiver noise temperatures are 21, 23, and 25 Kelvin and the measured antenna efficiencies are 70%, 75%, and 60% in S-band, X-band, and Ka-band, respectively. |
Author | Malo-Gómez, Inmaculada Beltrán-Martínez, Francisco J Vaquero-Jiménez, Beatriz Tercero-Martínez, Félix Patino-Esteban, María Díez-González, Carmen González-García, Javier López-Pérez, José A Serna-Puente, José M López-Fernández, José A García-Pérez, Óscar Gallego-Puyol, Juan D Barbas-Calvo, Laura García-Carreño, Pablo Albo-Castaño, Carlos López-Fernández, Isaac de Vicente-Abad, Pablo |
AuthorAffiliation | Yebes Observatory, Centro de Desarrollos Tecnológicos, Instituto Geográfico Nacional, Ministerio de Transportes, Movilidad y Agenda Urbana, Cerro de la Palera s.n., Yebes, E-19141 Guadalajara, Spain; f.tercero@oan.es (F.T.-M.); jm.serna@oan.es (J.M.S.-P.); b.vaquero@oan.es (B.V.-J.); m.patino@oan.es (M.P.-E.); pablo.garcia@oan.es (P.G.-C.); j.gonzalez@oan.es (J.G.-G.); ogarcia@oan.es (Ó.G.-P.); francisco.beltran@oan.es (F.J.B.-M.); c.albo@oan.es (C.A.-C.); jd.gallego@oan.es (J.D.G.-P.); i.lopez@oan.es (I.L.-F.); c.diez@oan.es (C.D.-G.); i.malo@oan.es (I.M.-G.); l.barbas@oan.es (L.B.-C.); p.devicente@oan.es (P.d.V.-A.); jalfernandez@mitma.es (J.A.L.-F.) |
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Snippet | This paper shows a simultaneous tri-band (S: 2.2-2.7 GHz, X: 7.5-9 GHz and Ka: 28-33 GHz) low-noise cryogenic receiver for geodetic Very Long Baseline... This paper shows a simultaneous tri-band (S: 2.2–2.7 GHz, X: 7.5–9 GHz and Ka: 28–33 GHz) low-noise cryogenic receiver for geodetic Very Long Baseline... |
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StartPage | 2662 |
SubjectTerms | Antennas Artificial satellites Calibration Communication Cryogenic temperature Design Earth Extremely high frequencies geodesy Geodetics Laboratories Noise Observatories Radiation Radio telescopes radioastronomy radiometer radiotelescope receiver Receivers & amplifiers Superhigh frequencies Telescopes Temperature Very long base interferometry VLBI |
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Title | A Tri-Band Cooled Receiver for Geodetic VLBI |
URI | https://www.ncbi.nlm.nih.gov/pubmed/33920073 https://www.proquest.com/docview/2550454404 https://search.proquest.com/docview/2520874100 https://pubmed.ncbi.nlm.nih.gov/PMC8069004 https://doaj.org/article/6774ef68963845cf9cf0b22c1257c0b3 |
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