极地超视距雷达接收阵列

R. Riddolls, S. Henault
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引用次数: 4

摘要

极地超视距雷达的接收阵列设计主要是为了减轻出现在各个方位角的极光雷达杂波。阵列必须足以在这种杂波存在的情况下检测和定位目标。虽然在半波长单元间距上部署最大性能的大型二维天线网格是可行的,但阵列的细化可以降低成本。基于解析杂波模型,表明元件密度可以在不显著降低性能的情况下减半。将密度细化到1 / 4会开始产生明显的性能影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Receive Arrays for Polar Over-the-Horizon Radar
Receive array design for Polar Over-the-Horizon Radar is driven primarily by the need to mitigate auroral radar clutter that appears at all azimuth angles. Arrays must be adequate to enable the detection and location of targets in the presence of this clutter. While it is feasible to deploy a maximum-performance large two-dimensional antenna grid at half-wavelength element spacing, thinning of the array can reduce cost. Based on an analytic clutter model, it is shown that the element density could potentially be halved without significant decrease in performance. Thinning to one-quarter density starts to incur noticeable perfomance impacts.
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