Design of two Ku-band orthomode transducers for radio astronomy applications

IF 6.7 1区 计算机科学 Q1 Physics and Astronomy
R. Nesti, E. Orsi, G. Pelosi, S. Selleri
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引用次数: 0

Abstract

Two different designs of orthomode transducers for the coming Ku-band receiver of the Italian radio telescope in Medicina are presented and compared, showing design details, describing numerical simulations and discussing manufacturing and test results. Such orthomode transducers provide a tradeoff between low-loss and phase-matching, according to different initial requirements where the final receiver architecture has to be frozen. Both designs show high performance over the operative 13.5–18.1 GHz Ku-band. One of the OMT designs has been fabricated and tested, showing results in very good agreement with simulations.
射电天文学用两个ku波段正交换能器的设计
介绍和比较了两种不同设计的正交换能器,用于即将在美第奇纳的意大利射电望远镜ku波段接收机,展示了设计细节,描述了数值模拟,并讨论了制造和测试结果。这种正交换能器提供了低损耗和相位匹配之间的权衡,根据不同的初始要求,最终的接收器结构必须被冻结。两种设计都在工作的13.5-18.1 GHz ku波段表现出高性能。其中一种OMT设计已经制作完成并进行了测试,结果与仿真结果非常吻合。
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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来源期刊
CiteScore
7.20
自引率
3.00%
发文量
0
审稿时长
1.3 months
期刊介绍: Progress In Electromagnetics Research (PIER) publishes peer-reviewed original and comprehensive articles on all aspects of electromagnetic theory and applications. This is an open access, on-line journal PIER (E-ISSN 1559-8985). It has been first published as a monograph series on Electromagnetic Waves (ISSN 1070-4698) in 1989. It is freely available to all readers via the Internet.
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