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Interferometer angle-of-arrival determination using precalculated phases

机译:使用预先计算的相位确定干涉仪的到达角

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摘要

A method has been developed to determine the angle of arrival (AoA) of incident radiation using precomputed lookup tables. The phase difference between two receiving antennas can be used to infer AoA as measured from the pair baseline, but there will be more than one possible solution for antenna spacings greater than or equal to half a wavelength. Larger spacings are preferable to minimize mutual coupling of elements in the receive array and to decrease the relative uncertainty in measured phase difference. We present a solution that uses all unique antenna pairs to determine probabilities for all possible azimuth and zenith values. Prior to analysis, the expected phase differences for all AoAs are calculated for each antenna pair. For a received signal, histograms of possible AoAs for each antenna pair phase difference are extracted and added to produce a two-dimensional probability density array that will maximize at the true value of the AoA. A benefit of this method is that all possible antenna pairs are utilized rather than the restriction to specific pairs along baselines used by some interferometer algorithms. Numerical simulations indicate that performance of the suggested algorithm exceeds that of existing methods, with the benefit of additional flexibility in antenna placement. Meteor radar data have been used to test this method against existing methods, with excellent agreement between the two approaches. This method of AoA determination will allow the construction of low-cost interferometric direction finding arrays with different layouts, including construction of difficult terrain and three-dimensional antenna arrangements. Plain Language Summary A method has been developed to determine the direction that radio waves are coming from when detected by an arrangement of antennas. The method looks at each of the unique pairs of antennas and compares the received signal with what would be expected for all possible directions. The results from all of the pairs of antennas are added to find the true direction that the radio waves are coming from. This improves the accuracy of simple radars and allows different types of antenna patterns to be used. Computer simulations show that the suggested method is very effective. Tests of data from a real radar also show excellent agreement between the new method and existing techniques.
机译:已经开发出一种使用预先计算的查找表确定入射辐射的到达角(AoA)的方法。两个接收天线之间的相位差可用于推断从一对基线测量的AoA,但是对于大于或等于一半波长的天线间距,将有不止一种可能的解决方案。较大的间距是可取的,以最大程度地减少接收阵列中元素的相互耦合,并减小所测相位差的相对不确定性。我们提出了一种使用所有唯一天线对来确定所有可能方位角和天顶值概率的解决方案。在分析之前,为每个天线对计算所有AoA的预期相位差。对于接收到的信号,提取并添加每个天线对相位差的可能AoA的直方图,并将其相加以生成二维概率密度阵列,该阵列将在AoA的真实值处最大化。这种方法的好处是,利用了所有可能的天线对,而不是沿某些干涉仪算法所使用的基线对特定天线对的限制。数值模拟表明,所建议算法的性能超过了现有方法,并具有天线放置额外灵活性的优势。流星雷达数据已用于对照现有方法测试此方法,两种方法之间具有极好的一致性。这种确定AoA的方法将允许构建具有不同布局的低成本干涉式测向阵列,包括构建困难的地形和三维天线布置。朴素的语言摘要已开发出一种方法,用于确定通过天线装置检测到的无线电波的方向。该方法查看每对唯一的天线,并将接收到的信号与所有可能方向的预期信号进行比较。来自所有天线对的结果相加,以找到无线电波来自的真实方向。这提高了简单雷达的精度,并允许使用不同类型的天线方向图。计算机仿真表明,该方法非常有效。来自真实雷达的数据测试还表明,新方法与现有技术之间有着极好的一致性。

著录项

  • 来源
    《Radio Science》 |2017年第10期|1058-1066|共9页
  • 作者

    Younger J. P.; Reid I. M.;

  • 作者单位

    ATRAD Pty Ltd, Thebarton, SA, Australia|Univ Adelaide, Sch Phys Sci, Adelaide, SA, Australia;

    ATRAD Pty Ltd, Thebarton, SA, Australia|Univ Adelaide, Sch Phys Sci, Adelaide, SA, Australia;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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