The Research on Excitation Method of All-metal Vivaldi Antenna Array Feeder for FAST

Hu Zhang*, Hong Da Lu, Yong Liu

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

Abstract

In order to improve the sensitivity and efficiency of the radio telescope receiver system and to solve the problem of discontinuous field of view of the feed cluster, a phase array feed is proposed as the feed of the radio telescope, and the amplitude and phase control of the array beam is an important part of the phase array feed design. In this paper, a 61-element phased array feeder for Five-hundred-meter Aperture Spherical radio Telescope (FAST) based on all-metal Vivaldi antenna is proposed. The direct conjugate field matching (DCFM) excitation method and the indirect conjugate field matching (ICFM) excitation method are compared and analyzed. The performances of the beamforming based on the proposed feeder array is verified by co-simulation which consists of full-wave method and quasi-optical method. In the frequency range of 2-6 GHz, the aperture efficiencies above 60% are obtained.

Original languageEnglish
Title of host publication2022 IEEE Conference on Antenna Measurements and Applications, CAMA 2022
PublisherInstitute of Electrical and Electronics Engineers
ISBN (Electronic)9781665490375
DOIs
Publication statusPublished - 2022
Event2022 IEEE Conference on Antenna Measurements and Applications, CAMA 2022 - Guangzhou, China
Duration: 14 Dec 202217 Dec 2022

Publication series

NameIEEE Conference on Antenna Measurements and Applications, CAMA
Volume2022-December
ISSN (Print)2474-1760
ISSN (Electronic)2643-6795

Conference

Conference2022 IEEE Conference on Antenna Measurements and Applications, CAMA 2022
Country/TerritoryChina
CityGuangzhou
Period14/12/2217/12/22

Keywords

  • Conjugate Field Matching Excitation
  • Focal Plane Field Analysis
  • Phased Array Feed

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