Wideband sun-star shape coplanar waveguide antenna for terahertz sensing applications

IF 3 Q3 Physics and Astronomy
Sina Kiani, Pejman Rezaei, Maryam Khajenoori
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引用次数: 0

Abstract

In this article, a miniaturized surface sun-star antenna has been presented to meet the requirements of a wide frequency band. During the antenna design phase, the concept of the propagation part is inspired by the combination of the sun and star. The coplanar waveguide has been selected as a 50-ohm feed. The configuration of the patch and the feedline of the proposed antenna has been constructed with gold. They have been placed on a polyimide substrate. This structure has a compact physical dimension of 4050000 µm3. The results of the simulated antenna, including the S11 parameter, radiation pattern, surface current distribution, and gain have been investigated. This investigated antenna covers a frequency range from 372 GHz to 683 GHz for S11 ≤ −10 dB with a bandwidth ratio of 1.84:1 and a fractional bandwidth of 59 %. Moreover, the far-field results in the frequency band depict an omnidirectional pattern with a radiation gain of 5 dBi and 93 % efficiency.
用于太赫兹传感应用的宽带太阳星形共面波导天线
本文提出了一种满足宽频带要求的小型化表面日星天线。在天线设计阶段,传播部分的概念灵感来自太阳和恒星的结合。共面波导被选为50欧姆馈电。该天线的贴片和馈线的结构都是用金构造的。它们被放置在聚酰亚胺基板上。该结构的物理尺寸紧凑,为4050000µm3。仿真结果包括S11参数、辐射方向图、表面电流分布和增益。该天线覆盖372 GHz ~ 683 GHz的频率范围,S11≤- 10 dB,带宽比为1.84:1,分数带宽为59%。此外,远场结果在波段描绘了全向模式,辐射增益为5 dBi,效率为93%。
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
Results in Optics
Results in Optics Physics and Astronomy-Atomic and Molecular Physics, and Optics
CiteScore
2.50
自引率
0.00%
发文量
115
审稿时长
71 days
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