Ultrawideband Conical Log-Spiral Circularly Polarized Feed for Radio Astronomy
Artikel i vetenskaplig tidskrift, 2020
In order to meet the requirements of the new generation of radio telescopes, we have developed a new topology called DYQSA, which stands for DYson Quad-Spiral Array. The design exhibits dual circular polarization contrary to dual linear polarization of state-of-the-art feeds. It covers the required ultrawideband (UWB) from 2 to 14 GHz with an almost constant and real input impedance which facilitates the design of the feeding structure and the low-noise amplifiers (LNAs). Different versions are investigated for enhancing feed performance, ensuring higher aperture efficiencies and mechanical stability. The simulation results of the reflector loaded by the proposed feed show an aperture efficiency of 65%±5% with a noise antenna temperature around 14 K and a system equivalent flux density (SEFD) of about 1300 Jy, both averaged over the required bandwidth at zenith. Measurements of the single-element and the four-element feeds are presented. Comparisons with other state-of-the-art feeds are shown in terms of total aperture efficiencies, design adaptability to different reflectors, calibration signal injection, and the required number of LNAs per feed, cost, and physical volume.
Very Long Baseline Interferometry (VLBI)
Antenna radiation patterns
Reflector antenna feeds
Log spiral antennas
Conical antennas
DYson Quad-Spiral Array (DYQSA)
Dual-polarized antennas
ultra wideband (UWB) antennas
Radio telescopes
Circular polarization
Signal to noise ratio
3-D printing
Apertures
Radio astronomy
VLBI2010 Global Observing System (VGOS)
Författare
Kerlos Atia Abdalmalak
Universidad Carlos III de Madrid
Aswan University
Gabriel Santamaría Botello
Universidad Carlos III de Madrid
Sergio Llorente-Romano
Universidad Carlos III de Madrid
Alejandro Rivera-Lavado
Universidad Carlos III de Madrid
Observatorio de Yebes (IGN)
Jonas Flygare
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium, Elektroniklaboratorium
José Antonio López Fernández
Observatorio de Yebes (IGN)
RUAG Space
José Manuel Serna Puente
RUAG Space
Observatorio de Yebes (IGN)
Luis Emilio García-Castillo
Universidad Carlos III de Madrid
Daniel Segovia-Vargas
Universidad Carlos III de Madrid
Miroslav Pantaleev
Chalmers, Rymd-, geo- och miljövetenskap, Onsala rymdobservatorium, Elektroniklaboratorium
Luis Enrique García-Muñoz
Universidad Carlos III de Madrid
IEEE Transactions on Antennas and Propagation
0018-926X (ISSN)
Vol. 68 3 1995-2007 8889508Infrastruktur
Onsala rymdobservatorium
Ämneskategorier
Elektroteknik och elektronik
DOI
10.1109/TAP.2019.2949700