Wideband LP to CP converter using a reflectarray based on modulated admittance surfaces capable of wide-range beam-scanning for Ku/K band applications

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Radio Science Pub Date : 2024-08-01 DOI:10.1029/2023RS007881
Hamid Tahermanesh;Mohammad Sadegh Abrishamian;Zahra Ghattan Kashani;Mahdi Salehi
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Abstract

This study provides the design and demonstration of a Ku/K band horn-fed linear polarization (LP) to circular polarization (CP) converter using a reflectarray antenna based on the holographic technique and the generalized law of total reflection without any iterative algorithms. The proposed hologram performs wide-range frequency beam scanning with minimum gain losses and cross-polarization levels. It comprises 2,500 diagonal slotted octagonal subwavelength metasurfaces with a periodicity of 0.266λ 0 = 4 mm at 20 GHz as the center frequency. Two equations are defined to compute Y 11 of the proposed unit cell regarding its dimensions for TE(0,0) and TM(0,0) Floquet modes. They significantly simplify the coding procedure and reduce the computational time for synthesizing the hologram. The antenna is simulated using the CST software from 14 to 25 GHz. As a confirmation, a prototype is manufactured and measured at 16, 18, 20, 22, and 24 GHz to verify its performance. The simulated and measured results are well-matched. The presented hologram achieves 40% 1.8-dB axial ratio (AR) bandwidth (16–25 GHz), 40% 3.3-dB gain bandwidth (16–24 GHz), and above 30% 2-dB gain bandwidth (16–22 GHz). Moreover, the antenna can perform beam scanning from 42° to 24° by changing the frequency from 16 to 24 GHz with peak gain values greater than 20.33 dBi. The LHCP pencil beams are at least 24° off-broadside, so the proposed hologram avoids the feed blockage. These achievements make the hologram one of the best candidates for satellite communications, radar applications, short-range communication, and point-to-point communication.
使用基于调制导纳面的反射阵列的宽带 LP 到 CP 转换器,能够为 Ku/K 波段应用提供宽范围波束扫描
本研究基于全息技术和广义全反射定律,在不使用任何迭代算法的情况下,利用反射阵列天线设计并演示了一种 Ku/K 波段喇叭馈电线性极化(LP)到圆极化(CP)转换器。所提出的全息图能以最小的增益损耗和交叉极化水平实现宽频波束扫描。它由 2,500 个对角开槽八边形亚波长元面组成,周期为 0.266λ0 = 4 毫米,中心频率为 20 千兆赫。我们定义了两个方程,用于计算拟议单元尺寸中 TE(0,0) 和 TM(0,0) Floquet 模式的 Y11。这两个方程大大简化了编码过程,减少了合成全息图的计算时间。该天线使用 CST 软件在 14 至 25 GHz 范围内进行了仿真。作为确认,制造了一个原型,并在 16、18、20、22 和 24 GHz 下进行了测量,以验证其性能。模拟和测量结果匹配良好。所展示的全息图实现了 40% 的 1.8 分贝轴向比 (AR) 带宽(16-25 千兆赫)、40% 的 3.3 分贝增益带宽(16-24 千兆赫)和高于 30% 的 2 分贝增益带宽(16-22 千兆赫)。此外,通过改变 16 至 24 千兆赫的频率,该天线还能进行 42° 至 24° 的波束扫描,峰值增益大于 20.33 dBi。LHCP 铅笔形波束至少偏离路边 24°,因此所提议的全息图可避免馈电阻塞。这些成就使全息图成为卫星通信、雷达应用、短程通信和点对点通信的最佳选择之一。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Radio Science
Radio Science 工程技术-地球化学与地球物理
CiteScore
3.30
自引率
12.50%
发文量
112
审稿时长
1 months
期刊介绍: Radio Science (RDS) publishes original scientific contributions on radio-frequency electromagnetic-propagation and its applications. Contributions covering measurement, modelling, prediction and forecasting techniques pertinent to fields and waves - including antennas, signals and systems, the terrestrial and space environment and radio propagation problems in radio astronomy - are welcome. Contributions may address propagation through, interaction with, and remote sensing of structures, geophysical media, plasmas, and materials, as well as the application of radio frequency electromagnetic techniques to remote sensing of the Earth and other bodies in the solar system.
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