利用脊载u型辐射器的高效圆极化ka波段卫星通信天线的研制

IF 4.8 2区 计算机科学 Q2 ENGINEERING, ELECTRICAL & ELECTRONIC IEEE Antennas and Wireless Propagation Letters Pub Date : 2024-11-25 DOI:10.1109/LAWP.2024.3506452
Raha Roosefid;Sadegh Mansouri Moghaddam;Lukas Nyström;Jian Yang;Ashraf Uz Zaman
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引用次数: 0

摘要

本文介绍了一种基于脊隙波导(RGW)技术的低轮廓高增益腔背槽阵列天线,可在Ka频段内工作。天线阵由两层组成。上层包含一系列u形槽,位于装有金属脊段的空腔上,而下层是RGW公司配电网络,以相同的相位和振幅分别为每个空腔支撑的槽供电。所提出的阵列天线辐射圆极化波(轴比低于3$ \text{dB}$),带宽为8.6$ \%$,范围从27.5$ $ GHz到30$ $ \text{GHz}$。在中心频率为28.75 GHz时,宽带方向的峰值增益为27$ \text{dB}$,第一相对旁瓣电平低于- 13$ \text{dB}$。所提出的8 × 8元阵列天线的总尺寸为6.7$ \lambda _{0} \乘以6.5$ \lambda _{0} \乘以1.4$ \lambda _{0} $。
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Development of a High-Efficiency Circularly Polarized Ka-Band Satcom Antenna Utilizing Ridge-Loaded U-Shaped Radiator
This letter presents a low-profile, high-gain cavity-backed slot array antenna, based on ridge gap waveguide (RGW) technology, to operate within the Ka frequency band. The antenna array consists of two layers. The upper layer incorporates an array of U-shaped slots, positioned over a cavity loaded with a metal ridge section, while the lower layer is a RGW corporate distribution network, feeding each of the cavity-backed slots separately with equal phase and amplitude. The proposed array antenna radiates circularly polarized waves (axial ratio below 3$ \text{ dB}$) over a bandwidth of 8.6$ \%$ ranging from 27.5$ $ GHz to 30$ \, \text{ GHz}$. At the centre frequency of 28.75 GHz, the peak gain at the broadside direction is 27$ \text{ dBi}$ and the first relative sidelobe level is below −13$ \text{ dB}$. The total size of the proposed 8 × 8$ $-element array antenna is 6.7$ \lambda _{0} \times $ 6.5$ \lambda _{0} \times $ 1.4$ \lambda _{0} $.
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来源期刊
CiteScore
8.00
自引率
9.50%
发文量
529
审稿时长
1.0 months
期刊介绍: IEEE Antennas and Wireless Propagation Letters (AWP Letters) is devoted to the rapid electronic publication of short manuscripts in the technical areas of Antennas and Wireless Propagation. These are areas of competence for the IEEE Antennas and Propagation Society (AP-S). AWPL aims to be one of the "fastest" journals among IEEE publications. This means that for papers that are eventually accepted, it is intended that an author may expect his or her paper to appear in IEEE Xplore, on average, around two months after submission.
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