Axially Corrugated Feed Horn for the Next Generation Very Large Array (ngVLA) Band-5 Receiver

This paper introduces a novel axially corrugated feed horn designed for the ngVLA Band-5 receiver, covering the 30–50 GHz range with potential adaptability to nearby bands. The horn features a circular waveguide with a flared throat and six precisely engineered quarter-wavelength corrugations. This structure achieves exceptional performance, including a return loss better than 25 dB and an average aperture efficiency of 95.5% across the full bandwidth. Measurements confirm the simulated results, validating the design. Compared to existing solutions, this feed horn offers a unique combination of wide bandwidth, high efficiency, and excellent signal fidelity in a compact, easily manufacturable form. These advancements address multiple challenges in radio astronomy receiver design, supporting the next generation of high-sensitivity telescopes like the ngVLA.

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Publication Details

Journal
IEEE Open Journal of Antennas and Propagation
Published
2025-05-23
DOI
https://doi.org/10.1109/ojap.2025.3572811
Primary Topic
Microwave Engineering and Waveguides
Type
article
Field-Weighted Citation Impact
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article

Axially Corrugated Feed Horn for the Next Generation Very Large Array (ngVLA) Band-5 Receiver

Doug Henke, Christos G. Christodoulou, W. Grammer, Brian B. Duverneay et al.
IEEE Open Journal of Antennas and Propagation
Microwave Engineering and Waveguides
article

Axially Corrugated Feed Horn for the Next Generation Very Large Array (ngVLA) Band-5 Receiver

Doug Henke, Christos G. Christodoulou, W. Grammer, Brian B. Duverneay, Jayakrishnan Vijayamohanan, A. Densmore, Sara Salem Hesari, B. Veidt
article en

Abstract

This paper introduces a novel axially corrugated feed horn designed for the ngVLA Band-5 receiver, covering the 30–50 GHz range with potential adaptability to nearby bands. The horn features a circular waveguide with a flared throat and six precisely engineered quarter-wavelength corrugations. This structure achieves exceptional performance, including a return loss better than 25 dB and an average aperture efficiency of 95.5% across the full bandwidth. Measurements confirm the simulated results, validating the design. Compared to existing solutions, this feed horn offers a unique combination of wide bandwidth, high efficiency, and excellent signal fidelity in a compact, easily manufacturable form. These advancements address multiple challenges in radio astronomy receiver design, supporting the next generation of high-sensitivity telescopes like the ngVLA.

IEEE Open Journal of Antennas and PropagationVol. 6(5)
Herzberg Institute of Astrophysics (CA), University of New Mexico (US), National Radio Astronomy Observatory (US), National Research Council Canada (CA)
Affordable and clean energy
Openalex Percentile: Top 91%
Microwave Engineering and Waveguides
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