Side lobe suppression analysis of spiral array optical antenna

N. Kondratiev, Marcus Engsig, Evgeny Lonshakov, C. Kasmi, S. Cordette
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Abstract

Optical array antennas have diverse applications in optical communication, remote sensing, imaging, and astronomy, supporting a broad range of optical and photonics-based technologies. Traditional square phased array antennas require a half-wavelength emitter spacing to prevent secondary orders of emission (aliasing). However, achieving such small distances in optics is impractical. To break this limitation irregularly-placed arrays has been proposed. This study focuses on the alias-free spiral array, which allows for high level of sidelobe suppression. Using standard Huygens–Fresnel principle approach to calculate the emission pattern, we identify key parameters of the spiral and consider their influence on the result. We perform multi-parametric optimisation of the spiral array for maximum suppression of sidelobes, enhancing its performance by dB compared to previously suggested bio-inspired design. This research provides insights into overcoming aliasing challenges and improving the efficiency of optical array antennas.
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螺旋阵列光学天线的边叶抑制分析
光阵列天线在光通信、遥感、成像和天文学等领域有着广泛的应用,支持各种基于光学和光子学的技术。传统的方形相控阵天线需要半波长的发射器间距,以防止二次发射(混叠)。然而,在光学技术中实现如此小的距离是不切实际的。为了打破这一限制,有人提出了不规则排列阵列。本研究的重点是无混叠螺旋阵列,这种阵列可实现高水平的侧射抑制。我们使用标准的惠更斯-菲涅尔原理方法计算发射模式,确定螺旋阵列的关键参数,并考虑它们对结果的影响。我们对螺旋阵列进行了多参数优化,以最大限度地抑制侧叶,使其性能比以前提出的生物启发设计提高了分贝。这项研究为克服混叠难题和提高光学阵列天线的效率提供了真知灼见。
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