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Some issues related to the novel spectral acceleration method for the fast computation of radiation/scattering from one-dimensional extremely large scale quasi-planar structures

机译:与一维超大规模拟平面结构快速计算辐射/散射的新型光谱加速方法有关的一些问题

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摘要

The novel spectral acceleration (NSA) algorithm has been shown to produce an (Ntot) efficient iterative method of moments for the computation of radiation/scattering from both one-dimensional (1-D) and two-dimensional large-scale quasi-planar structures, where Ntot is the total number of unknowns to be solved. This method accelerates the matrix-vector multiplication in an iterative method of moments solution and divides contributions between points into “strong” (exact matrix elements) and “weak” (NSA algorithm) regions. The NSA method is based on a spectral representation of the electromagnetic Green's function and appropriate contour deformation, resulting in a fast multipole-like formulation in which contributions from large numbers of points to a single point are evaluated simultaneously. In the standard NSA algorithm the NSA parameters are derived on the basis of the assumption that the outermost possible saddle point, φs,max, along the real axis in the complex angular domain is small. For given height variations of quasi-planar structures, this assumption can be satisfied by adjusting the size of the strong region Ls. However, for quasi-planar structures with large height variations, the adjusted size of the strong region is typically large, resulting in significant increases in computational time for the computation of the strong-region contribution and degrading overall efficiency of the NSA algorithm. In addition, for the case of extremely large scale structures, studies based on the physical optics approximation and a flat surface assumption show that the given NSA parameters in the standard NSA algorithm may yield inaccurate results. In this paper, analytical formulas associated with the NSA parameters for an arbitrary value of φs,max are presented, resulting in more flexibility in selecting Ls to compromise between the computation of the contributions of the strong and weak regions. In addition, a “multilevel” algorithm, decomposing 1-D extremely large scale quasi-planar structures into more than one weak region and appropriately choosing the NSA parameters for each weak region, is incorporated into the original NSA method to improve its accuracy.
机译:新型频谱加速(NSA)算法已显示出可产生一矩(Ntot)的有效矩量迭代方法,用于从一维(1-D)和二维大规模拟平面结构计算辐射/散射,其中Ntot是要解决的未知总数。该方法以矩量解的迭代方法加快了矩阵矢量的乘积,并将点之间的贡献分为“强”(精确矩阵元素)和“弱”(NSA算法)区域。 NSA方法基于电磁格林函数的频谱表示和适当的轮廓变形,从而形成了一种快速的多极类公式化,其中可以同时评估从大量点到单个点的贡献。在标准NSA算法中,NSA参数是基于以下假设得出的:在复角域中沿实轴的最外面的鞍点φs,max小。对于准平面结构的给定高度变化,可以通过调整强区域Ls的大小来满足该假设。但是,对于高度变化较大的准平面结构,调整后的强区域大小通常较大,导致计算强区域贡献的计算时间显着增加,并降低了NSA算法的整体效率。另外,对于超大型结构,基于物理光学近似和平坦表面假设的研究表明,标准NSA算法中给定的NSA参数可能会产生不准确的结果。在本文中,提出了与NSA参数相关的φs,max任意值的解析公式,从而在选择Ls时有更大的灵活性,可以在强弱区域贡献的计算之间进行折衷。另外,一种“多级”算法将一维超大型准平面结构分解为一个以上的弱区域,并为每个弱区域适当选择了NSA参数,以提高其准确性。

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