Sidelobe reduction with array fed spherical lenses

J. Sanford, Z. Šipuš
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引用次数: 6

Abstract

The material contained in this paper is intended to help determine the feasibility of using a spherical lens as a low sidelobe multiple beam antenna. It includes what are deemed the most relevant points of a more thorough investigation. We consider the constant-k lens and the Luneberg lens. The constant-k lens, as the name implies, is a homogeneous dielectric sphere. R.K. Luneberg proposed the Luneberg lens in 1944. Morgan (1960) derived a general class of Luneberg lenses that focus from one arbitrary point source to another. In the 50s and 60s antenna designers applied Luneberg lenses to a wide variety of antenna and scattering applications. The array feed used to illuminate the lens has its surface on a sphere with a radius equal to, or larger than, the outer radius of the lens. Each element of the array forms an independent beam. These beams are combined to form a new beam with lower sidelobes.
用阵列馈电球面透镜减少旁瓣
本文所包含的材料旨在帮助确定使用球面透镜作为低旁瓣多波束天线的可行性。它包括被认为是更彻底的调查中最相关的要点。我们考虑常数k透镜和吕尼伯格透镜。常数k透镜,顾名思义,是一个均匀的介电球。1944年,鲁讷贝格提出了鲁讷贝格透镜。Morgan(1960)导出了一类吕尼伯格透镜,它从一个任意点源聚焦到另一个点源。在50年代和60年代,天线设计师将吕内伯格透镜应用于各种各样的天线和散射应用。用于照亮透镜的阵列馈电其表面在一个半径等于或大于透镜外半径的球体上。阵列的每个元素形成一个独立的波束。这些波束组合在一起形成一个具有较低旁瓣的新波束。
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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