Regression Technique for Electromagnetic Field Sampling and Reconstruction

S. Rondineau, B. Fuchs, F. B. Ribeiro Costa, L. Le Coq, E. Gonçalves Sousa, M. Migliore
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Abstract

The presented work deals with an alternative technique for sampling and reconstructing the electromagnetic field radiated by any kind of antenna or equivalent currents, and measured in its far field region. Based on the electrical size of the radiating object, it truncates the vector spherical modal field expansion series. Then, each component of the field is projected on the classical Fourier space for the polar dependency. This is carried out by minimizing the variance of the residual noise, or, in other words, by applying the Tikhonov-Phillips regularization scheme. This results is not only a numerically well-posed problem, but also in the statistical independence of the resulting coefficients as their co-variance matrix is diagonal. Afterwards, the azimuth dependency is projected on the real valued Gegenbauer, also known as ultra-spherical, polynomial family, once again following the Tikhonov-Phillips regularization scheme. Once again, it does not only result in a numerically well-posed problem, leading to a statistical independence of the obtained spherical modal coefficients. Moreover this double regression technique leads to the smallest two-dimensional Cartesian grid of angular sampling positions, a very useful result for the far field antenna characterization industry where measurement time has to be reduced as much as possible. Additionally to this, both optimum estimators and stable regularizer are also extracted. Then, a statistical analysis of the residual error is performed by extracting and analyzing the noise properties and also creating a statistical filter that rejects any mode that is not statistically significant through the definition of a modal signal-to-noise ratio. This result turns out to be very useful when this technique is applied in a compressive-sensing-like radiated far field antenna analysis. At last, these estimators are modified to attend cases where the measured data do not form a full column ranked matrix. This corresponds to the case where measurements data are lacking in the previously defined smallest two-dimensional Cartesian grid of angular sampling positions. This technique is then applied to several different antenna measurements, as shown on fig. 1, where can be noticed a very good matching between in the far $E_{\theta}$ and $E_{\varphi}$ field 2D map in amplitude comparison of both the measured electric field and the reconstructed one for a flat metallic Luneburg lens antenna designed at the frequency 12 GHz in the frame of MERLIN, which is a joint laboratory of Thalès Alenia Space and IETR. More details about this radiating structure are available in the reference [1].
电磁场采样与重构的回归技术
本文提出了一种采样和重建任何天线或等效电流辐射的电磁场的替代技术,并在其远场区域进行了测量。根据辐射物体的电尺寸,截断矢量球模态场展开级数。然后,将场的每个分量投影到经典傅里叶空间中以表示极性依赖。这是通过最小化残余噪声的方差来实现的,或者换句话说,通过应用Tikhonov-Phillips正则化方案。这个结果不仅是一个数值上的适定问题,而且由于它们的协方差矩阵是对角的,所以所得到的系数在统计上是独立的。然后,将方位依赖投影到实值Gegenbauer多项式族(也称为超球面多项式族)上,再次遵循Tikhonov-Phillips正则化方案。再一次,它不仅导致一个数值上的适定问题,导致得到的球面模态系数的统计独立性。此外,这种双重回归技术导致最小的角度采样位置的二维笛卡尔网格,这对于远场天线表征行业非常有用,因为测量时间必须尽可能地减少。此外,还提取了最优估计量和稳定正则化器。然后,对残差进行统计分析,提取和分析噪声特性,并创建一个统计滤波器,通过定义模态信噪比来拒绝任何不具有统计意义的模态。结果表明,该方法可用于类压缩传感辐射远场天线的分析。最后,对这些估计量进行了修正,以适应实测数据不形成全列排序矩阵的情况。这对应于在先前定义的角采样位置的最小二维笛卡尔网格中缺乏测量数据的情况。然后将该技术应用于几种不同的天线测量,如图1所示,其中可以注意到在远$E_{\theta}$和$E_{\varphi}$场二维图中测量电场的振幅与重建电场的振幅比较非常匹配,这是在MERLIN框架下设计的12 GHz频率的平面金属Luneburg透镜天线,MERLIN是thal阿莱尼亚空间和IETR的联合实验室。关于这种辐射结构的更多细节可以在参考文献[1]中找到。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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