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Reflector feeds for large adaptive reflector antennas.

机译:大型自适应反射器天线的反射器馈电。

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摘要

A novel Feed-Reflector system for large Cassegrain antennas for Radio Astronomy and Deep-Space Communication applications is investigated. This Feed-Reflector is used to illuminate a hyperboloid sub-reflector with 5–10 m diameter located 500 m above the ground. Because the sub-reflector is located in the near field of the Feed-Reflector antenna, a theory based on the near field focusing properties of paraboloid reflectors is established. The focusing at near distance is formed by moving the feed horn away from the focal point of the Feed-Reflector. In this theory the properties of axial defocused paraboloid reflectors at near distance are investigated in some detail.; By using equivalence path law, sub-reflector shape is obtained. It is found that the hyperbola can approximate the sub-reflector well. A detailed ray tracing analysis is performed on the entire system which reveals that some part of the sub-reflector receive three rays per point from the feed. The performance of the system over the operating band (1–22 GHz) is also studied and shown that the lower frequency limit is dependent on sub-reflector and Feed-Reflector sizes.; To obtain higher efficiencies, three sets of shaping techniques, based on the genetic algorithm and Jacobi Fourier surface expansion, are performed. An efficiency of 78.5% for a 5 m sub-reflector is obtained.; In another method of analysis, the Feed-Reflector aperture field distribution is expanded into a set of Gaussian-Laguerre modes. These modes propagate from the Feed-Reflector aperture in a simple and well defined way. The Feed-Reflector near field radiation pattern is calculated at the sub-reflector location. The sub-reflector parameters in this system are found by maximizing the Large Adaptive Reflector (LAR) aperture efficiency which includes phase and taper efficiencies, and minimizing the LAR spillover loss.; An exact equation for the offset LAR surface is obtained in this thesis. To scan the beam up to 60°, which is one of the LAR requirements, the concept of the dual offset LAR with the Feed-Reflector is introduced. In this design the cross-polarization is eliminated by proper orientation of the sub-reflector. The parameters of the configuration are obtained by utilizing generalized Gauss-Laguerre beam modes and matrix representation of beam mode transformation factor. In this design the blockage effect due to the Feed-Reflector is totally removed.
机译:研究了一种用于射电天文学和深空通信应用的大型卡塞格伦天线的新型馈电反射器系统。该馈电反射器用于照明离地面500 m处直径为5–10 m的双曲面次反射器。由于副反射器位于馈电反射器天线的近场中,因此建立了基于抛物面反射器近场聚焦特性的理论。通过将馈电喇叭从馈电反射镜的焦点移开,可以形成近距离的聚焦。在该理论中,对轴向散焦抛物面反射器在近距离处的特性进行了详细研究。通过使用等效路径定律,可以获得副反射镜的形状。发现双曲线可以很好地近似副反射器。在整个系统上进行了详细的光线追踪分析,该分析表明,副反射镜的某些部分每点从进料接收三束光线。还研究了系统在工作频带(1-22 GHz)上的性能,并表明较低的频率限制取决于副反射镜和馈电反射镜的尺寸。为了获得更高的效率,执行了三套基于遗传算法和Jacobi Fourier表面扩展的成形技术。对于5 m的副反射镜,其效率为78.5%。在另一种分析方法中,前馈反射器的孔径场分布扩展为一组高斯-拉格勒模式。这些模式以简单且定义明确的方式从反光板孔传播。在副反射器位置计算进给反射器近场辐射方向图。通过使包括相位和锥度效率的大型自适应反射器(LAR)孔径效率最大化,并使LAR溢出损耗最小化,可以找到该系统中的副反射器参数。本文获得了一个偏移的LAR表面的精确方程。为了扫描高达60°的光束(这是LAR的要求之一),引入了带有馈电反射器的双偏移LAR的概念。在该设计中,通过副反射器的正确定向消除了交叉极化。通过使用广义高斯-拉格瑞光束模式和光束模式转换因子的矩阵表示来获得配置的参数。在这种设计中,完全消除了由于馈电反射器引起的阻塞效应。

著录项

  • 作者

    Mousari Bafrooei, Pedram.;

  • 作者单位

    The University of Manitoba (Canada).;

  • 授予单位 The University of Manitoba (Canada).;
  • 学科 Engineering Electronics and Electrical.
  • 学位 Ph.D.
  • 年度 2001
  • 页码 162 p.
  • 总页数 162
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 无线电电子学、电信技术;
  • 关键词

  • 入库时间 2022-08-17 11:46:56

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