维瓦尔第阵列天线带内散射截面估计方法

Shi-xue Fang, S. Qu
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引用次数: 0

摘要

天线的带内散射是天线模式散射和结构模式散射的叠加。本文证明了阵列边缘散射源引起的散射是结构模式散射的主要原因。此外,可以通过天线单元的辐射估计阵列的天线模式散射。因此,可以通过估计天线模式和结构模式散射的叠加来估计带内散射截面(SCS)。制作并测量了x波段维瓦尔第阵列天线。实测的单稳态SCS结果与仿真结果一致,表明了分析的正确性和估计方法的有效性。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Method to Estimate in-band Scattering Cross Section of Vivaldi Array Antenna
The in-band scattering of the antenna is the superposition of the antenna mode scattering and structural mode scattering. In this paper, the scattering, resulted from the scattering sources on the edges of the array, is proved to be the main contribution to the structural mode scattering. Moreover, the antenna mode scattering of the array can be estimated through the radiation of the antenna element. Therefore, the in-band scattering cross section (SCS) can be estimated by the superposition of the estimated antenna mode and structural mode scattering. The X-band Vivaldi array antenna is fabricated and measured. The measured monostatic SCS results are in an agreement with the simulations, showing the correctness of the analysis and the effectiveness of the estimation method.
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