A Chamfered Pyramidal Potter Horn Antenna With Low Sidelobe Level and Cross Polarization

IF 4.8 2区 计算机科学 Q2 ENGINEERING, ELECTRICAL & ELECTRONIC
Jun Xiao;Jing Wu;Tongyu Ding;Yan Wang;Chong-Zhi Han
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引用次数: 0

Abstract

In this letter, a chamfered pyramidal Potter horn antenna is designed with both low sidelobe level (SLL) and low cross-polarization level (XPL). First, a stepped discontinuity structure is introduced to excite the TM12 mode. By precisely controlling the amplitude and phase of the TM12 mode through structural adjustment, low SLL and low XPL performances are achieved. In addition, simple chamfered structures are also applied to change the electric field distribution across the horn aperture, which further reduces the XPL of the pyramidal horn antenna. Finally, the antenna is fabricated and measured. Measurements demonstrate excellent E-plane and H-plane symmetry with low SLL across 23.5 GHz to 29.5 GHz, achieving a bandwidth of 22.6% with XPL lower than −30 dB. The E-plane SLL remains below −25 dB throughout the operating band. Note that the proposed pyramidal Potter horn achieves an unprecedented minimum measured XPL of −37.8 dB.
具有低旁瓣电平和交叉极化的倒角锥形波特喇叭天线
本文设计了一种低旁瓣电平(SLL)和低交叉极化电平(XPL)的倒角锥形波特喇叭天线。首先,采用阶梯式不连续结构激发TM12模式。通过结构调整精确控制TM12模式的幅值和相位,实现了低SLL和低XPL性能。此外,还采用了简单的倒角结构来改变喇叭孔径上的电场分布,进一步降低了锥形喇叭天线的XPL。最后,对天线进行了制作和测量。测量结果表明,在23.5 GHz至29.5 GHz范围内,具有良好的e面和h面对称性,低SLL,在XPL低于- 30 dB时实现22.6%的带宽。E-plane的SLL在整个工作频带内保持在−25 dB以下。请注意,所提出的金字塔形波特喇叭达到了前所未有的最小测量XPL - 37.8 dB。
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
8.00
自引率
9.50%
发文量
529
审稿时长
1.0 months
期刊介绍: IEEE Antennas and Wireless Propagation Letters (AWP Letters) is devoted to the rapid electronic publication of short manuscripts in the technical areas of Antennas and Wireless Propagation. These are areas of competence for the IEEE Antennas and Propagation Society (AP-S). AWPL aims to be one of the "fastest" journals among IEEE publications. This means that for papers that are eventually accepted, it is intended that an author may expect his or her paper to appear in IEEE Xplore, on average, around two months after submission.
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