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An array of lens-coupled antennas for cosmic microwave background measurements in the 30 Ghz band

机译:一组透镜耦合天线,用于在30 GHz频段内进行宇宙微波背景测量

摘要

An array of bow-tie slot antennas coupled through an extended hemispherical lens is proposed to operate in the 30 GHz frequency band. The design includes a combination of three microstrip Wilkinson power dividers (WPD) and transitions to coplanar wave guides (CPW) to form the feeding antenna network. This configuration is suitable for the integration with heterodyne imaging detectors commonly used in radioastronomy. Measurements and simulation results exhibit a frequency range of operation from 20 to 40 GHz with a bandwidth of 24% achieved for -10 dB return loss at the central frequency. The measured radiation patterns show a maximum peak gain of around 13 dB with HPBW of 10° for the E-plane, and whose first side lobes are lower than 13 dB below the main lobe in both angular shift sides. The presented results will be considered as preliminary feasibility studies in the 30 GHz QUIJOTE-CMB Instrument, which is designed to study the anisotropies of the Cosmic Microwave Background (CMB). © 2011 Springer Science+Business Media B.V.
机译:提议通过扩展的半球形透镜耦合的领结缝隙天线阵列在30 GHz频带内工作。该设计包括三个微带威尔金森功率分配器(WPD)和过渡到共面波导(CPW)以形成馈电天线网络的组合。这种配置适合与射电天文学中常用的外差成像探测器集成。测量和仿真结果显示,工作频率范围为20至40 GHz,在中心频率处的-10 dB回波损耗实现了24%的带宽。测得的辐射方向图显示,E平面的HPBW为10°时,最大峰值增益约为13 dB,并且在两个角度偏移侧,其第一旁瓣低于主瓣以下13 dB。提出的结果将被视为30 GHz QUIJOTE-CMB仪器的初步可行性研究,该仪器旨在研究宇宙微波背景(CMB)的各向异性。 ©2011 Springer Science + Business Media B.V.

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