Dielectrically Loaded Quad-Ridge Flared Horn for Beamwidth Control Over Decade Bandwidth-Optimization, Manufacture, and Measurement
Journal article, 2020

We present the design, manufacture, and measured performance of a dielectrically loaded quad-ridge flared horn (QRFH) feed for decade bandwidth radio astronomy application. The introduction of the dielectric load improves the QRFH beamwidth control in H-plane at the mid and upper frequency range. Consequently on the reflector, illumination efficiency, phase efficiency, and the intrinsic cross-polarization ratio (IXR) have been improved. The dielectric load is made from homogeneous low-loss polytetrafluoroethylene and has a low profile with a cylinder shape for simple installation at the center of the QRFH. The dielectrically loaded QRFH presented here covers 1.5-15.5 GHz with a calculated average aperture efficiency above 50% on a f/D = 0.3 prime-focus reflector. We present a calculation of system noise temperature and sensitivity for the QRFH on a 100 m prime-focus reflector. Measured beam patterns of the QRFH are in good agreement with the simulations over the full frequency band. The input reflection coefficient was predicted to be below -10 dB across the bandwidth. We present a tolerance analysis that explains why the measured one deviates.

Bandwidth

reflector feed

Dielectrics

ultra wideband (UWB) antennas

Optimization

quad-ridge flared horn (QRFH)

radio astronomy

Feeds

Author

Jonas Flygare

Chalmers, Space, Earth and Environment, Onsala Space Observatory, Electronics Laboratory

Miroslav Pantaleev

Ruag Space Switzerland

IEEE Transactions on Antennas and Propagation

0018-926X (ISSN)

Vol. 68 1 207-216 8852836

RadioNet 4

European Commission (Horizon 2020), 2017-01-01 -- 2020-12-31.

Infrastructure

Onsala Space Observatory

Subject Categories

Communication Systems

Electrical Engineering, Electronic Engineering, Information Engineering

DOI

10.1109/TAP.2019.2940529

More information

Latest update

2/6/2020 1