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A Deterministic Propagation Model for Multipath Analysis at SKA Precursor Telescopes—A Case Study on MeerKAT

机译:SKA前驱望远镜多路径分析的确定性传播模型—以MeerKAT为例

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Interferometers comprising large numbers of small diameter antennas are increasingly on the rise. This is in part driven by the technology and science around the Square Kilometre Array (SKA) and leads to progressively higher receiver sensitivities. Consequently, these new generation radio telescopes are more susceptible to radio frequency interference. The situation may be further aggravated when dishes are deployed in a compact fashion since this can result in a complex multipath environment. Focusing on the 64-dish SKA precursor, MeerKAT, multipath effects in the core area comprising 44 dishes of 13.5 m diameter in a 1 km radius are investigated. Due to complexity of the environment, empirical models offer limited benefit, and hence, numerical modeling becomes a compelling solution. We thus present a deterministic propagation model exploiting the method of moments for antenna and real ground modeling and physical optics for representing scattering from metallic surfaces. In this way, the MeerKAT core was reproduced computationally and attenuation maps were produced revealing high- and low-risk regions.
机译:包括大量小直径天线的干涉仪正在日益增长。这部分是由平方公里阵列(SKA)周围的技术和科学驱动的,并导致接收器灵敏度逐渐提高。因此,这些新一代射电望远镜更容易受到射频干扰。当以紧凑的方式部署碗碟时,情况可能会进一步恶化,因为这会导致复杂的多路径环境。着眼于64碟SKA前驱物MeerKAT,研究了核心区域的多径效应,该核心区域包括44个直径13.5 m的碟形天线,半径1 km。由于环境的复杂性,经验模型提供的收益有限,因此,数值建模成为一种引人注目的解决方案。因此,我们提出了一种确定性传播模型,该模型利用了天线和真实地面建模的矩量方法以及代表从金属表面散射的物理光学技术。通过这种方式,通过计算重现了MeerKAT核心,并生成了衰减图,揭示了高风险和低风险区域。

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