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Analysis of reflector antenna systems for wide-angle scanning.

机译:反射镜天线系统的广角扫描分析。

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摘要

A near-field Cassegrain reflector (NFCR) is an effective way to magnify a small phased array into a much larger aperture antenna for limited scan applications. Traditionally, the pattern analysis of NFCR is based on a plane wave approach. This approach simplifies the computation tremendously, but fails to provide design information about the most critical component of the whole antenna system, namely, the feed array. Here, each element in the feed array is considered individually and its diffraction pattern from the subreflector is computed by GTD. The field contributions from all elements are superimposed at the curved main reflector surface, and a physical optics integration is performed to obtain the secondary pattern.; Beam-waveguide-fed Cassegrain reflector (BFCR) antennas are increasingly being used in space communication applications. Using a shooting and bouncing ray approach based on geometrical optics and aperture integration, the far-field pattern of the BFCR is calculated. This method is computationally efficient and is not restricted by the number of reflecting surfaces in the antenna configuration. The diffraction loss in the beam waveguide structure is calculated separately by the conventional near-field physical optics integration.; The segmented mirror antenna is designed for the radiometer application on the planned NASA Earth Science Geostationary Platforms in the 1990s. The antenna consists of two parts: a regular parabolic dish of 5 m in diameter which converts the radiation from feeds into a collimated beam, and a movable mirror that redirects the beam to a prescribed scan direction. The mirror is composed of 28 segmented planar conducting plates, mostly one square meter in size. Based on a physical optics analysis, we have analyzed the secondary pattern of the antenna. For frequencies between 50 and 230 GHz, and for a scan range of {dollar}pm{dollar} 8{dollar}spcirc{dollar} (270 beamwidths scan at 230 GHz), the worst calculated beam efficiency is 95%. To cover such a wide frequency and scan range, each of the 28 plates is individually controlled for a tilting less than 4{dollar}spcirc{dollar}, and for a sliding less than 0.5 cm.
机译:近场卡塞格伦反射器(NFCR)是一种有效的方法,可将小相控阵放大为孔径更大的天线,以进行有限的扫描应用。传统上,NFCR的模式分析基于平面波方法。这种方法极大地简化了计算,但是未能提供有关整个天线系统最关键的组件(即馈电阵列)的设计信息。在此,分别考虑馈源阵列中的每个元素,并通过GTD计算其从副反射镜的衍射图。所有元素的场贡献叠加在弯曲的主反射器表面上,并进行物理光学积分以获得次级图案。波束馈送的卡塞格伦反射器(BFCR)天线越来越多地用于空间通信应用中。使用基于几何光学和孔径积分的射击和弹跳射线方法,可以计算出BFCR的远场模式。该方法在计算上是有效的,并且不受天线配置中反射表面的数量的限制。光束波导结构中的衍射损耗是通过传统的近场物理光学积分法单独计算的。分段反射镜天线是专为1990年代计划中的NASA地球科学对地静止平台上的辐射计应用而设计的。天线由两部分组成:直径为5 m的规则抛物面形碟,可将来自馈电的辐射转换为准直光束;可移动镜,可将光束重定向至规定的扫描方向。镜子由28个分段的平面导电板组成,大部分尺寸为1平方米。基于物理光学分析,我们分析了天线的次级方向图。对于50到230 GHz之间的频率,以及对于{dollar} pm {dollar} 8 {dollar} spcirc {dollar}的扫描范围(在230 GHz下扫描270束宽度),最差的计算光束效率是95%。为了覆盖如此宽的频率和扫描范围,分别控制28个板中的每个板的倾斜度小于4 spspcirc {dollar},滑动小于0.5 cm。

著录项

  • 作者

    Houshmand, Bijan.;

  • 作者单位

    University of Illinois at Urbana-Champaign.;

  • 授予单位 University of Illinois at Urbana-Champaign.;
  • 学科 Engineering Electronics and Electrical.; Physics Astronomy and Astrophysics.
  • 学位 Ph.D.
  • 年度 1990
  • 页码 128 p.
  • 总页数 128
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 无线电电子学、电信技术;天文学;
  • 关键词

  • 入库时间 2022-08-17 11:50:35

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