Journal
IEEE TRANSACTIONS ON ANTENNAS AND PROPAGATION
Volume 65, Issue 12, Pages 7322-7327Publisher
IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC
DOI: 10.1109/TAP.2017.2760365
Keywords
Radio telescope; reflector antenna; ridged antennas; ridged waveguide; wideband feed
Funding
- National Natural Science Foundation of China [61427801, 61771127, U1536123, U1536124, 11403080]
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This communication proposes a compact, high performance, quadruple-ridged flared horn operating from 8 to 50 GHz. A prototype fed by two coaxial connectors has been designed and fabricated based on the combination of a four-petal structure and a back plate. Measurements show that the input reflection coefficients are below -10 dB over more than 6: 1 frequency range. Radiation patterns were measured in an anechoic chamber, and good agreement was found with the simulation results. Physical optics calculations predict an average of 68% aperture efficiency with the feed installed on the square kilometer array shaped offset Gregorian reflector. The horn is a good demonstration at very high frequencies of a wideband feed for radio telescopes.
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