论文标题

SKA LFAA站设计报告

SKA LFAA Station Design Report

论文作者

Acedo, Eloy de Lera, Pienaar, Hardie, Ghods, Nima Razavi, Abraham, Jens, Beltran, Edgar Colin, Mort, Ben, Dulwich, Fred, Virone, Giuseppe, Fiorelli, Benedetta, Arts, Michiel, Craeye, Christophe, van Ha, Bui, Grainge, Keith, Dewdney, Peter, Wagg, Jeff, Labate, Maria Grazia, Faulkner, Andrew, de Vaate, Jan Geralt bij, Gerbers, Marchel

论文摘要

该报告是作为SKA低频孔径阵列的一部分提交的,描述了2013年至2018年之间进行的SKA1-LOW站的设计。 SKA1低场站刻在一个圆形区域,其有效的站直径(中心至中心)为38米,并具有256个SKALA4元素。本文档描述了现场站的电磁设计。特别是它描述了布局设计以及电磁建模和站点的特性。本文档描述了与布局和阵列相关的效果,例如相互耦合效应,侧瓣模式和梁的形状(例如光滑度,校准模型),并提出了我们测量阵列性能并验证模拟工作的能力的艺术状态。自LFAA PDR和系统基线设计以来的过去几年,源自SKA L1要求的当前LFAA场节点需求已经发展。 SKA1低场站旨在满足这些要求,因此跟踪其演变(例如灵敏度要求,阵列直径等)。上述要求代表了一个非常紧密的空间,渴望在较大的频率范围内(7至1)和广泛的视野(Zenith周围的90度锥体),同时将电台直径保持在最低限度,因此作为填充因子,但在同一时间之间可以使天线之间的空间易于维护。这导致了复杂的设计。

This report was submitted as part of the SKA Low Frequency Aperture Array Critical Design Review describing the design of the SKA1-LOW station that took place between 2013 and 2018. The SKA1 LOW field station is inscribed in a circular area having an effective station diameter (centre to centre) of 38 meters and has 256 SKALA4 elements. This document describes the electromagnetic design of the field station. In particular it describes the layout design and the electromagnetic modelling and characteristics of the station. This document describes the effects associated with the layout and array such as mutual coupling effects, side lobe pattern and beam shape (eg. smoothness, calibration models) and presents the state of the art of our ability to measure the array performance and validate the simulation work. The current LFAA field node requirements, derived from the SKA L1 requirements, have evolved over the last years since the LFAA PDR and the System Baseline Design. The SKA1 LOW field station has been designed to meet those requirements and has therefore tracked their evolution (eg. sensitivity requirements, array diameter, etc.). The aforementioned requirements represent a very tight space with a desire for very high sensitivity over a large frequency range (7 to 1) and wide field of view (90 degrees cone around zenith) while keeping the station diameter to a minimum, so as the filling factor but at the same time allowing for sufficient space between antennas to allow for easy maintenances, amongst many others. This results in a complex design.

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