Higher-Order Quasi-OAM Generation Utilizing a Quasi-Circular Array Antenna

Reham M. Fouda, T. Baum, K. Ghorbani
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Abstract

Orbital Angular Momentum (OAM) is a physical property of EM fields, which allows for the superposition of an infinite number of modes to exist on the same frequency carrier. However, as the number of OAM mode transmitted increases, so does the aperture size. Previous studies have shown that a QuasiCircular Array Antenna (QCA), where the annular aperture is truncated, is capable of producing a first-order Quasi-OAM noninteger mode. This paper investigates the capability of QCA apertures, in producing higher-order Quasi-OAM modes. The experimental results in free-space demonstrated herein, show that a QCA of six elements, is able to produce a non-integer Quasi-OAM mode of I = +1. 5, falling to the nearest integer mode I = +2 in the far-field.
利用准圆形阵列天线产生高阶准oam
轨道角动量(OAM)是电磁场的一种物理性质,它允许在同一频率载波上存在无限多模的叠加。然而,随着传输OAM模式的数量增加,孔径大小也会增加。先前的研究表明,截断环形孔径的准圆阵列天线(QCA)能够产生一阶准oam非整数模式。本文研究了QCA孔径产生高阶准oam模式的能力。在自由空间中的实验结果表明,六元QCA能够产生I = +1的非整数准oam模式。5,落到最接近的整数模式I = +2在远场。
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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