Digital Beamforming Demonstration of a Microstrip Antenna Phased Array Feeds (PAF) at 1.25 GHz

Abstract We introduce the structure of a radio astronomy phased array feeds (PAF) beamforming demonstrator. In a laboratory environment, we have demonstrated beamforming on a received 1.25 GHz sinusoidal signal and used digital weighting techniques to plot the 2D pattern of the PAF. The radio frequency part of the demonstrator includes a 4 × 4 linearly polarized microstrip antenna array, all of which is connected in series with a low-noise amplifier. The signals from the central 4 × 2 array elements are injected into a radio frequency system-on-chip digital board, which can receive eight inputs with a bandwidth of 512 MHz. Combining the principle of undersampling, the beamforming is completed at a frequency of 1.25 GHz for the offline data, and a 2D image of the beam is plotted using beam scanning technology.

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Publication Details

Journal
Research in Astronomy and Astrophysics
Published
2024-09-05
DOI
https://doi.org/10.1088/1674-4527/ad7792
Primary Topic
Radio Astronomy Observations and Technology
Type
article
Field-Weighted Citation Impact
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article

Digital Beamforming Demonstration of a Microstrip Antenna Phased Array Feeds (PAF) at 1.25 GHz

Peng 鹏 Wu 仵, Mao-Zheng 卯蒸 Chen 陈, Jian 健 Li 李, Kai 凯 Wang 王 et al.
Research in Astronomy and Astrophysics
Radio Astronomy Observations and Technology
article

Digital Beamforming Demonstration of a Microstrip Antenna Phased Array Feeds (PAF) at 1.25 GHz

Peng 鹏 Wu 仵, Mao-Zheng 卯蒸 Chen 陈, Jian 健 Li 李, Kai 凯 Wang 王, Liang 亮 Cao 曹, Han 涵 Yu 于
article en

Abstract

Abstract We introduce the structure of a radio astronomy phased array feeds (PAF) beamforming demonstrator. In a laboratory environment, we have demonstrated beamforming on a received 1.25 GHz sinusoidal signal and used digital weighting techniques to plot the 2D pattern of the PAF. The radio frequency part of the demonstrator includes a 4 × 4 linearly polarized microstrip antenna array, all of which is connected in series with a low-noise amplifier. The signals from the central 4 × 2 array elements are injected into a radio frequency system-on-chip digital board, which can receive eight inputs with a bandwidth of 512 MHz. Combining the principle of undersampling, the beamforming is completed at a frequency of 1.25 GHz for the offline data, and a 2D image of the beam is plotted using beam scanning technology.

Research in Astronomy and AstrophysicsVol. 24(10)
Xinjiang Astronomical Observatory (CN), University of Chinese Academy of Sciences (CN)
Openalex Percentile: Top 89%
Radio Astronomy Observations and Technology
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