Modeling of RFI and RFI Mitigation Techniques in SKA1 Mid Telescope

T. Gunaratne, A. Peens-Hough
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引用次数: 1

Abstract

Radio Frequency Interference (RFI) has become a great challenge for the highly sensitive next-generation radio telescopes such as the Square Kilometre Array (SKA). The SKA phase-1 Mid frequency (SKA1-Mid) telescope is exposed to RFI from aeronautical navigation and satellite broadcasting and navigation, although, it is generally protected from terrestrial RFI being located in a radio-quite zone in South Africa. An earlier study was conducted to model the RFI that is expected by the receivers of SKA1-Mid at the Karoo site. This is further extended to study, through modelling, the responses of the receiver’s analog signal chain and the correlator and beamformer’s digital signal processing chain along with the RFI mitigation techniques proposed for the SKA1-Mid telescope. Simulations have been conducted to confirm that the stringent requirements, which needed to meet the science goals of the telescope, can be met under several RFI scenarios.
SKA1中望远镜RFI建模与RFI抑制技术
射频干扰(RFI)已成为平方公里阵列(SKA)等高灵敏度下一代射电望远镜面临的巨大挑战。SKA第一阶段中频(SKA1-Mid)望远镜暴露在来自航空导航和卫星广播和导航的射频信号中,尽管它位于南非的无线电安静区,通常不受地面射频信号的影响。早期的一项研究对Karoo位点SKA1-Mid受体所期望的RFI进行了建模。通过建模,进一步扩展到研究接收机模拟信号链、相关器和波束形成器数字信号处理链的响应,以及为SKA1-Mid望远镜提出的RFI缓解技术。已经进行了模拟,以确认在几个RFI场景下可以满足满足望远镜科学目标所需的严格要求。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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