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A Novel Collimation Correction Of Active Array Antenna implemented In Risat

机译:在Risat中实现的新型有源阵列天线准直校正

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摘要

Traditionally, collimation error estimation of an active array antenna is carried out from the Near-Field (NF) hologram where all the elements of the active array antenna are illuminated simultaneously. However, typical NF processing resolution is ~λ and typical element spacing in scan direction is less than ~0.7 λ. Consequently it becomes very difficult to resolve amplitude and phase errors, especially in the presence of sharp amplitude and phase discontinuities. Further, this method requires area scanning of antenna in near field to obtain . hologram. This paper presents a novel method, where amplitude and gain response of individual rows are measured using a single scan. For this purpose, TR modules are switched one at a time. The correction coefficients, estimated with this method, are very accurate and free from aforementioned distortions because of wide impulse response of NF processor. Further, only a linear scan is sufficient to assess the correction factors with significant impact on the time required for such estimation.
机译:传统上,有源阵列天线的准直误差估计是从近场(NF)全息图进行的,其中有源阵列天线的所有元素都同时被照亮。但是,典型的NF处理分辨率为〜λ,并且在扫描方向上的典型元素间距小于〜0.7λ。因此,解决振幅和相位误差变得非常困难,尤其是在振幅和相位不连续性很尖锐的情况下。此外,该方法需要在近场中对天线进行区域扫描以获得。全息图。本文提出了一种新颖的方法,其中使用单次扫描测量单个行的幅度和增益响应。为此,TR模块一次切换一次。用这种方法估算的校正系数非常精确,并且由于NF处理器的宽脉冲响应而没有上述失真。此外,仅线性扫描就足以评估对这种估计所需时间有重大影响的校正因子。

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