Finite element method modeling of the wire thickness of a monopole on a circular ground plane

IF 1.6 4区 地球科学 Q3 ASTRONOMY & ASTROPHYSICS Radio Science Pub Date : 2024-12-31 DOI:10.1029/2024RS008068
C. G. Hynes;R. G. Vaughan
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Abstract

Simulations and measurements of the input impedance and matching of a cylindrical monopole at the center of a circular ground plane are presented. The design parameters are the monopole length (0.231 to 0.261), the monopole radius (10 −5 λ to 5 × 10 −3 λ), and the ground plane radius (0.2λ to 2.0λ), where λ is the wavelength. Using new numerical results from the Finite Element Method (FEM), previous theoretical impedance results for an infinitesimally thin element are shown to be inaccurate for monopoles of practical thicknesses since there can be a strong dependence on the wire thickness—even for electrically very thin wires. The FEM offers convenient modeling for the wire thickness and the results match well with physical experiments. To obtain good antenna impedance matching to a 50 Ω impedance, that is, 5 11 < — 10 dB, for any ground plane radius greater than 1/2 (an arbitrary lower bound) and any practical wire monopole radius, the simulations show that a monopole length of 0.241 can be used.
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圆形地平面上单极子导线厚度的有限元建模
对圆形地平面中心的圆柱单极子的输入阻抗和匹配进行了仿真和测量。设计参数为单极子长度(0.231 ~ 0.261)、单极子半径(10 × 5λ ~ 5 × 10−3λ)和接地面半径(0.2λ ~ 2.0λ),其中λ为波长。利用有限元法(FEM)的新数值结果,先前的无限小薄单元的理论阻抗结果对于实际厚度的单极子是不准确的,因为即使对于电非常薄的导线,也可能对导线厚度有很强的依赖性。该方法为线材厚度的模拟提供了方便,模拟结果与物理实验结果吻合较好。为了获得与50 Ω阻抗匹配良好的天线阻抗,即511 < - 10 dB,对于任何大于1/2的地平面半径(任意下界)和任何实际线单极子半径,仿真表明单极子长度为0.241可以使用。
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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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