非对称馈电长形球面天线的辐射图

H. A. Myers
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引用次数: 5

摘要

本文描述了非对称馈电球面发射天线的辐射方向图。麦克斯韦方程组在受边界条件约束的长球面坐标系中求解。延长球函数以幂级数和洛朗级数的形式表示。得到了三种不同长度的天线的辐射图,最长约为一个波长,长度/厚度比约为5/ 1,10 /1,22/1和316/1,9个不对称间隙位置以及对称馈电情况。研究发现,影响相当薄天线的辐射方向图的两个最重要的因素是间隙的位置和电长度。对于小于半波长长的天线,图案是通常的对称数字8,并且基本上与间隙的位置无关(除了由于不同的间隙阻抗而引起的幅度变化)。对于三分之二到四分之三波长长的天线,数字8模式可以在较长元件的方向上“弯曲”,对于一个波长或更长波长的天线,小瓣开始出现。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Radiation patterns of unsymmetrically fed prolate spheroidal antennas
This paper describes the radiation pattern of the un-symmetrically-fed prolate spheroidal transmitting antenna. Maxwell's equations are solved in prolate spheroidal coordinates subject to the boundary conditions. The prolate spheroidal functions are expressed in the form of power series and Laurent series. Radiation patterns have been obtained for antennas of three different lengths up to about one wavelength long, for length/thickness ratios of about 5/1, 10/1,22/1, and 316/1, and for nine unsymmetrical gap locations as well as for the symmetrically-fed cases. It was found that the two most important factors affecting the radiation pattern of a fairly thin antenna were the location of the gap and the electrical length. For antennas less than a half wavelength long, the pattern was the usual symmetrical figure eight and was essentially independent of the location of the gap (except for magnitude changes due to the different gap impedances). For antennas two-thirds to three-quarters of a wavelength long the figure eight patterns could be "bent" in the direction of the longer element, and for antennas one wavelength long or longer minor lobes began to appear.
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