Realizing orthogonal modes in compact cavity-backed dual-polarized antenna through simple feeding structures for millimeter-wave AiP applications

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS
Radio Science Pub Date : 2024-10-01 DOI:10.1029/2024RS008042
Tzu-Ming Huang;Yi-Cheng Lin
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引用次数: 0

Abstract

This paper presents a dual-polarized cavity-backed antenna designed for mm-wave applications, featuring simple feeding structures with a high-isolation for 60 GHz compact AiP applications. The dual-polarization design relies on two separate feed ports that excite two orthogonal modes within the same resonant cavity, achieving very high port isolation of up to 40 dB over the entire band. We conducted a detail analysis of the antenna, including its working principles and parametric studies. For verification, we fabricated an antenna test kit using standard printed process on substrates and measured the kit from the back-side of a GSG probing platform. The proposed antenna demonstrates a wide impedance bandwidth, stable radiation patterns, very low cross-polarization levels, and a high radiation efficiency. The co-located cavity-backed design ensures the compactness and facilitates easy integration with ICs in a very small AiP module. These features make the proposed antenna highly suitable for 60 GHz AiP applications, such as high-data-rate wireless communication and mmW polarimetric radar systems.
通过用于毫米波 AiP 应用的简单馈电结构,在紧凑型腔背双极化天线中实现正交模式
本文介绍了一种专为毫米波应用设计的双极化腔背天线,其特点是馈电结构简单,隔离度高,适用于 60 GHz 紧凑型 AiP 应用。双极化设计依靠两个独立的馈电端口,在同一谐振腔内激发两个正交模式,从而在整个频段内实现高达 40 dB 的极高端口隔离度。我们对天线进行了详细分析,包括其工作原理和参数研究。为了进行验证,我们使用标准印刷工艺在基板上制作了一个天线测试套件,并从 GSG 探测平台的背面对该套件进行了测量。所提出的天线具有较宽的阻抗带宽、稳定的辐射模式、极低的交叉极化水平和较高的辐射效率。同位腔背设计确保了结构紧凑,便于与集成电路集成在一个非常小的 AiP 模块中。这些特点使拟议的天线非常适合 60 GHz AiP 应用,如高数据速率无线通信和毫米波极坐标雷达系统。
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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