Validation of the HARP method for simulation of mutual coupling between SKALA antennas

Q. Gueuning, C. Craeye, E. Colín-Beltrán, E. de Lera Acedo
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Abstract

The low-frequency instrument of the SKA radiotelescope will be made of large arrays of log-periodic antennas. Their mutual coupling may be strong and needs to be modeled in terms of embedded element patterns. The HARP method is based on Macro Basis Functions and computes their interactions versus relative positions, based on a limited number of explicit calculations in the near field. This paper shows results of this method in the low and medium range of the foreseen frequency spectrum, considering the SKALA (SKA Log-Periodic Antennas) designed for this new telescope.
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仿真SKALA天线间相互耦合的HARP方法的验证
SKA射电望远镜的低频仪器将由大型对数周期天线阵列组成。它们的相互耦合可能很强,需要根据嵌入的元素模式进行建模。HARP方法基于宏基函数,并基于有限数量的近场显式计算,计算它们与相对位置的相互作用。本文给出了该方法在预期频谱的中低频范围内的结果,并考虑了为该新型望远镜设计的SKA对数周期天线。
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