Analisys of cross-polarized radiation of optimized reflector antennas

N. Gorobets, V. Kiyko, V. Gorobets
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引用次数: 2

Abstract

Thus, the analysis and minimization of the main types cross-polarized radiation of highly directional antennas in the millimeter and submillimeter ranges are relevant and important for many practical applications. Let us consider the formation process of the spatial distribution of cross-polarized radiation reflector antennas in the whole space of observation (not just in the major E-and H-planes). In [1] was shown that in the case of single-reflector axially symmetric parabolic reflector antennas the radiation of the transverse polarization is equal to zero in the direction of the main beam on the basic polarization, as well as in the principal planes of observation. In this case, the maximum levels of cross-polarized radiation occur in the observation planes φ = ±45°. It is easy to show that this result can be generalize for all types of aperture antennas and field distribution is similar to elementary aperture radiator - Huygens radiator. Indeed, according to the rule of directional patterns multiplication, the directional pattern zeros of the elementary radiator in cross-polarized component automatically provides all zeros of the antenna radiation pattern in the same planes of observation.
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优化后反射面天线的交叉极化辐射分析
因此,分析和最小化高定向天线在毫米和亚毫米范围内的主要类型交叉极化辐射对许多实际应用具有重要意义。让我们考虑交叉极化辐射反射面天线在整个观测空间(不只是在主要的e面和h面)空间分布的形成过程。在[1]中表明,在单反射面轴对称抛物面反射面天线的情况下,在基本偏振方向上,以及在主观测平面上,横向偏振辐射在主波束方向上等于零。在这种情况下,交叉极化辐射的最大水平出现在φ =±45°的观测平面上。不难看出,这一结果可以推广到所有类型的孔径天线,其场分布与基本孔径辐射器-惠更斯辐射器相似。确实,根据方向图相乘的规律,交叉极化分量中基本辐射体的方向图零点自动提供了同一观测平面内天线辐射方向图的所有零点。
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