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On the bi-elliptical toroidal helical antenna problem

机译:关于双椭圆环形螺旋天线问题

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By eliminating the fundamental apriori assumption typical of previously reported formulations of bi-elliptical toroidal helical antenna (THA) problem, that the antenna will operate only at one or more of its three characteristic resonance frequencies, this paper describes a formulation of the problem in a vector potential approach, with basis in the derivation of a Green's function appropriate to the antenna geometry as starting point. Exact closed form expressions are derived for the radiation fields of the THA, and these expressions are shown to represent a general case of certain results reported in the open literature, as special cases. An important contribution of the derivation is that for the first time to the best of our knowledge, analysis is able to identify distinct contributions to the far-zone fields attributable to the main loop and the poloidal loops of the THA. Computational results for the THA operated in the dipole mode are presented in graphical formats displaying separate contributions of the main and poloidal loops, as well as their resultants, to the radiations fields. In the polar direction, radiation fields from these loops have similar shapes; though that due to the main loop is some 20 times larger in magnitude than that due to the poloidal loops. The resultant radiation field in the polar direction has the omnidirectional pattern characteristic of the dipole antenna. On the other hand, the phi-component of the radiation field is characterized by contributions from the main loop that are some 800 times greater in magnitude than those from the poloidal loops. And indeed, the computational results suggest that for the THA operated in the dipole mode, the phi-component in the far-zone dominates, with the net effect that that the THA's radiation field is directional, with the cardioid shape due to the dominant phi-component of the main loop.
机译:通过消除先前报道的双椭圆形环形螺旋天线(THA)问题的典型的基本先验假设,即天线将仅以其三个特征谐振频率中的一个或多个工作,本文描述了一个问题。向量势方法,以推导适合于天线几何形状的格林函数为基础。精确的闭式表达式是针对THA的辐射场得出的,这些表达式被表示为公开文献中报道的某些结果的一般情况,作为特殊情况。该推导的重要贡献是,就我们所知,这是第一次,分析能够确定对THA主回路和多倍体回路可归因于远区场的独特贡献。以偶极模式运行的THA的计算结果以图形格式显示,显示了主回路和极回路的单独贡献及其对辐射场的贡献。在极性方向上,来自这些回路的辐射场具有相似的形状。尽管由于主回路造成的振幅比因极回路造成的振幅大20倍。极化方向上的最终辐射场具有偶极天线的全向方向图特性。另一方面,辐射场的phi分量的特征是来自主回路的贡献在幅度上比来自极向回路的贡献大800倍。确实,计算结果表明,对于以偶极模式工作的THA,远区的phi分量占主导地位,其最终结果是THA的辐射场是定向的,心形因phi占主导而呈心形。 -主循环的组件。

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