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A Low-Cost Directional-Log Periodic Log Spiral Antenna

机译:低成本定向 - 日志定期日志螺旋天线

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The Square Kilometer Array (SKA) derives its name from its total aperture area, predominately achieved by thousands of parabolic dishes, each with an antenna feed situated at its focal point. The type of antenna feed selected for SKA operation in the 1 GHz to 10 GHz frequency range, referred to as a Wide Band Single Pixel Feed (WB+SPF) [1], has drawn increasing attention. This paper introduces a new WB+SPF to meet SKA scientific demands while also,providing a cost-effective solu-tion. The wide bandwidth of this new antenna is achieved by employing frequency independent (FI) design, principles for the development of a log periodic (LP) an-tenna [2]. A basic adherence to FI principles can be seen in several of the antennas currently proposed as WB+SPF solutions for the SKA, including the Allen Telescope.Array (ATA) feed [3], the Quasi-Self-Complementary (QSC) feed [4], and the Eleven feed [5]. These antennas efficiently illuminate the radio, dish with a single main lobe, ruling out entirely planar FI antennas, which generate two radiation lobes orthogonal to the plane of the, antenna. High sensitivity requirements prohibit the 3 dB power loss that would result from attenuating one of the lobes with an absorption cavity, as is often done for directional. FI antennas. Scaling the LP elements,into three-dimensional space, potentially over a ground plane [6], is the present method used for directional LP antennas. We instead propose confining these often complex LP elements into a single plane, while the ground "plane" takes on a:three dimensional form. Planar LP patterns permit low-cost implementations, including PCB and water jet cutting technology, without requiring the introduction of a complicated scaffolding to support the LP elements in 3-D. Additionally, various technologies such as metal spinning, can cost-effectively shape the ground "plane" into a 3-D structure. This low-cost WB+SPF. solution would scale well in the implementation of the thousands of antenna feeds that the SKA demands. We also' introduce a previously unreported LP design: the log periodic log spiral (LPLS) antenna.
机译:平方公里阵列(SKA)从其总孔径区域源自孔径区域,主要是通过数千个抛物面的抛物线,每个抛物线饲料都有一个位于其焦点的天线饲料。选择在1 GHz到10 GHz频率范围内的SKA操作所选择的天线饲料类型,称为宽带单像素馈送(WB + SPF)[1],越来越高。本文介绍了新的WB + SPF,以满足SKA科学需求,同时也提供了具有成本效益的解决方案。通过采用频率独立(FI)设计,用于开发日志周期(LP)AN-Tenna [2]来实现这一新天线的宽带宽。在目前建议为SKA的WB + SPF解决方案的几个天线中可以看到对FI原理的基本遵守,包括艾伦望远镜。array(ATA)饲料[3],准自互补(QSC)饲料[ 4]和11饲料[5]。这些天线有效地照亮了无线电,用单个主瓣的盘子,排列出完全平面的FI天线,其产生与天线的平面正交的两个辐射凸起。高灵敏度要求禁止3 DB功率损耗,该功率损失将导致其中一个具有吸收腔的裂隙,正如定向所做的那样。五个天线。将LP元素缩放到三维空间中,可能在接地平面[6]上,是用于定向LP天线的本方法。我们将这些经常复杂的LP元素提出将这些经常复杂的LP元素限制在一个平面中,而接地“平面”采用答:三维形式。平面LP图案允许低成本的实施,包括PCB和水射流切割技术,而无需引入复杂的脚手架以在3-D中支持LP元素。另外,诸如金属纺丝的各种技术可以成本有效地将接地“平面”形状为3-D结构。这种低成本的WB + SPF。解决方案在SKA所需的数千个天线饲料的实施中展示很好。我们还会引入以前未报告的LP设计:日志周期性日志螺旋(LPLS)天线。

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