A low insertion loss L-band feed front-end for the FAST Core Array

We designed a low insertion loss L-band feed front-end system to operate over a 1.15-1.75 GHz frequency range for the Five-hundred-meter Aperture Spherical radio Telescope (FAST) Core Array. The L-band feed front-end system comprises quadruple-ridge ortho-mode transducers and a choke horn. The coaxial output of the transducers extracts two mutually orthogonal polarization signals by coupling the input of a circular waveguide. Two non-cryogenic low temperature low-noise amplifiers with average noise of only 10 K at room temperature connected to coaxial outputs respectively. Because it operates at room temperature, the new developed ortho-mode transducer requires lower insertion loss than in designs intended to operate in extremely cold environments. This paper focuses on the 1.15–1.75 GHz L-Band ortho-mode transducer and choke horn design, with a measured L-band return loss of more than −20 dB, and an insertion loss of more than 0.09 dB. Considering the large quantity of front-end systems required for array applications, our design of ortho-mode transducers balances performance, adjustability, and ease of manufacture, and our choke horn design has high aperture efficiency across the L-band.

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Publication Details

Journal
Astronomical Techniques and Instrument
Published
2025-12-01
DOI
https://doi.org/10.3724/ati2025070
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
0.00

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article

A low insertion loss L-band feed front-end for the FAST Core Array

Rurong Chen, Xiaoming Chai, Jinglong Yu, Hengqian Gan et al.
Astronomical Techniques and Instrument
Radio Astronomy Observations and Technology
article

A low insertion loss L-band feed front-end for the FAST Core Array

Rurong Chen, Xiaoming Chai, Jinglong Yu, Hengqian Gan, Bin Liu, Yang Cao
article en

Abstract

We designed a low insertion loss L-band feed front-end system to operate over a 1.15-1.75 GHz frequency range for the Five-hundred-meter Aperture Spherical radio Telescope (FAST) Core Array. The L-band feed front-end system comprises quadruple-ridge ortho-mode transducers and a choke horn. The coaxial output of the transducers extracts two mutually orthogonal polarization signals by coupling the input of a circular waveguide. Two non-cryogenic low temperature low-noise amplifiers with average noise of only 10 K at room temperature connected to coaxial outputs respectively. Because it operates at room temperature, the new developed ortho-mode transducer requires lower insertion loss than in designs intended to operate in extremely cold environments. This paper focuses on the 1.15–1.75 GHz L-Band ortho-mode transducer and choke horn design, with a measured L-band return loss of more than −20 dB, and an insertion loss of more than 0.09 dB. Considering the large quantity of front-end systems required for array applications, our design of ortho-mode transducers balances performance, adjustability, and ease of manufacture, and our choke horn design has high aperture efficiency across the L-band.

Astronomical Techniques and Instrument
National Natural Science Foundation of China
Affordable and clean energy
Openalex Percentile: Top 25%
Radio Astronomy Observations and Technology
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