Five hundred-meter aperture spherical radio telescope (FAST) is a multi-disciplinary basic research platform that is used for a wide range of astronomy research. Currently, narrow-band multi-beam feed are primarily employed for observation. The development of ultra-wide broadband feed system is beneficial for covering more scientific objectives, while also giving full play to the advantages of the FAST huge reception area in wider frequency band. This paper focuses on the 0.5-3.3GHz feed design, which has better than 10 dB simulated return loss across the bandwidth with the method of using fitting curves and dielectric loading and adding corrugated structures to improve the performance of quad ridge flared horn (QRFH). A centrally positioned PTFE dielectric rod regulates electromagnetic wave phase velocity, enhancing radiation directivity and main lobe symmetry. The dielectric rod is formed by two concentric layers with the same dielectric constant but different structures. The outer layer is evenly slotted to reduce its dielectric constant. The addition of the above technical means ensures the symmetry of the E-plane and H-plane far-field patterns, making the aperture efficiency of the feed relatively balanced over 6.6:1 bandwidth. This kind of feed is designed with an emphasis on performance, ease of tuning and manufacturability compared to the case of multi-layer dielectric rods.
Published in | Science Discovery (Volume 13, Issue 3) |
DOI | 10.11648/j.sd.20251303.12 |
Page(s) | 46-50 |
Creative Commons |
This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited. |
Copyright |
Copyright © The Author(s), 2025. Published by Science Publishing Group |
Quad Ridge Flared Horn, Radio Telescope, Ultra-wide Band, Feed, Reflector Antenna
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APA Style
Yu, J., Liu, H., Li, J. (2025). Design and Simulation of Dielectric Load Ultra-Wide Band Corrugated Feed for FAST. Science Discovery, 13(3), 46-50. https://doi.org/10.11648/j.sd.20251303.12
ACS Style
Yu, J.; Liu, H.; Li, J. Design and Simulation of Dielectric Load Ultra-Wide Band Corrugated Feed for FAST. Sci. Discov. 2025, 13(3), 46-50. doi: 10.11648/j.sd.20251303.12
@article{10.11648/j.sd.20251303.12, author = {Jinglong Yu and Hongfei Liu and Jianbin Li}, title = {Design and Simulation of Dielectric Load Ultra-Wide Band Corrugated Feed for FAST }, journal = {Science Discovery}, volume = {13}, number = {3}, pages = {46-50}, doi = {10.11648/j.sd.20251303.12}, url = {https://doi.org/10.11648/j.sd.20251303.12}, eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.sd.20251303.12}, abstract = {Five hundred-meter aperture spherical radio telescope (FAST) is a multi-disciplinary basic research platform that is used for a wide range of astronomy research. Currently, narrow-band multi-beam feed are primarily employed for observation. The development of ultra-wide broadband feed system is beneficial for covering more scientific objectives, while also giving full play to the advantages of the FAST huge reception area in wider frequency band. This paper focuses on the 0.5-3.3GHz feed design, which has better than 10 dB simulated return loss across the bandwidth with the method of using fitting curves and dielectric loading and adding corrugated structures to improve the performance of quad ridge flared horn (QRFH). A centrally positioned PTFE dielectric rod regulates electromagnetic wave phase velocity, enhancing radiation directivity and main lobe symmetry. The dielectric rod is formed by two concentric layers with the same dielectric constant but different structures. The outer layer is evenly slotted to reduce its dielectric constant. The addition of the above technical means ensures the symmetry of the E-plane and H-plane far-field patterns, making the aperture efficiency of the feed relatively balanced over 6.6:1 bandwidth. This kind of feed is designed with an emphasis on performance, ease of tuning and manufacturability compared to the case of multi-layer dielectric rods. }, year = {2025} }
TY - JOUR T1 - Design and Simulation of Dielectric Load Ultra-Wide Band Corrugated Feed for FAST AU - Jinglong Yu AU - Hongfei Liu AU - Jianbin Li Y1 - 2025/06/11 PY - 2025 N1 - https://doi.org/10.11648/j.sd.20251303.12 DO - 10.11648/j.sd.20251303.12 T2 - Science Discovery JF - Science Discovery JO - Science Discovery SP - 46 EP - 50 PB - Science Publishing Group SN - 2331-0650 UR - https://doi.org/10.11648/j.sd.20251303.12 AB - Five hundred-meter aperture spherical radio telescope (FAST) is a multi-disciplinary basic research platform that is used for a wide range of astronomy research. Currently, narrow-band multi-beam feed are primarily employed for observation. The development of ultra-wide broadband feed system is beneficial for covering more scientific objectives, while also giving full play to the advantages of the FAST huge reception area in wider frequency band. This paper focuses on the 0.5-3.3GHz feed design, which has better than 10 dB simulated return loss across the bandwidth with the method of using fitting curves and dielectric loading and adding corrugated structures to improve the performance of quad ridge flared horn (QRFH). A centrally positioned PTFE dielectric rod regulates electromagnetic wave phase velocity, enhancing radiation directivity and main lobe symmetry. The dielectric rod is formed by two concentric layers with the same dielectric constant but different structures. The outer layer is evenly slotted to reduce its dielectric constant. The addition of the above technical means ensures the symmetry of the E-plane and H-plane far-field patterns, making the aperture efficiency of the feed relatively balanced over 6.6:1 bandwidth. This kind of feed is designed with an emphasis on performance, ease of tuning and manufacturability compared to the case of multi-layer dielectric rods. VL - 13 IS - 3 ER -