探地雷达用维瓦尔第天线

S. Memon, A. A. Jamali, M. Anjum, M. Memon, S. Qadri
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引用次数: 1

摘要

探地雷达(GPR)是一种用于识别和探测地表以下物体的先进技术。超宽带(UWB)天线作为探地雷达系统的一部分,用于发射和接收短电磁脉冲。探地雷达探测地下目标的根本难点在于天线本身的反射。这些反射引起晚时间振铃;这给地下物体的识别带来了问题。天线本身的反射可以通过研究天线的瞬态行为来检测。本文重点对探地雷达应用的超宽带维瓦尔第天线(1GHz - 2.6GHz)的设计进行了理论研究。在CST微波工作室对维瓦尔第天线进行了设计、优化和仿真。优化后的Vivaldi天线在中心频率(1.8 GHz)为-35dB时回波损耗较低,驻波比在1.0左右。维瓦尔第天线也采用探地雷达环境(即地球和地球内部的散射体)进行建模。因此,提出了优化后的维瓦尔第天线用于探地雷达应用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Vivaldi Antenna for Ground Penetrating Radar Applications
The Ground Penetrating Radar (GPR) is an advanced technique used for identifying and detecting objects beneath the surface. Ultra Wideband (UWB) antennas are utilized as a part of GPR system for transmission and reception of short electromagnetic pulses. The fundamental source of difficulty lies in the performance of GPR for detecting the subsurface objects is the reflection from the antenna itself. These reflections cause late time ringing; which makes problem in the recognition of the underground object. Reflections in the antenna itself can be examined by studying transient behavior of the antenna. This paper focuses on the theoretical investigation of the design of UWB Vivaldi antenna (1GHz - 2.6GHz) for GPR applications. Vivaldi antenna has been designed, optimized and simulated in the CST Microwave Studios. The optimized Vivaldi antenna has a lower return loss and VSWR at a center frequency (1.8 GHz) of -35dB and around 1.0, respectively. Vivaldi antenna is also modeled with the GPR environment (i.e. with earth and scatterer inside the earth). Hence, the optimized Vivaldi antenna is presented to use for GPR applications.
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