The SKA1_Low Telescope: The Station Design and Prototyping

J.G. Bij de Vaate,P. Hall,B. Juswardy, D. Kenney, F. Schlageuhaufer,M. Sokolowski,A. Sutinjo, D. Ung,R. Wayth, A. Williams,M. Alderighi, J. Bast, P. Bolli, G. Comoretto, A. Mattana,J. Monari, G. Naldi,F. Perini, G. Pupillo,S. Rusticelli, M. Schiaffino, F. Schilliro, P. Benthem, A. Aminei,R. Chiello, M. Jones, J. Baker, R. Bennett, R. Halsall, G. Kaligeridou, M. Roberts, H. Schnetler, J. Abraham, M. Gerbers,E. De Lera Acedo, A.J. Faulkner,N. Razavi-Ghods,D. Cutajar,A. DeMarco,A. Magro,K. Zarb Adami,S.J. Wijnholds, T. Booler, T. Colgate, B. Crosse, D. Emrich

2018 2nd URSI Atlantic Radio Science Meeting (AT-RASC)（2018）

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摘要

The Square Kilometre Array (SKA) [1] telescope consists in its first phase of two arrays, a dish array to be constructed in South Africa and a low frequency aperture array to be constructed in Western Australia. The aperture array, SKAI-Low, will consist of 512 stations, each with 256 wide bandwidth log periodic antennas. The frequency range of SKAI-Low is 50 to 350 MHz. The Low Frequency Aperture Array (LFAA) consortium is tasked to design the station, the infrastructure around them and the station signal processing.

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关键词

SKAI-Low telescope,low frequency aperture array consortium,square kilometre array telescope,station design,station signal processing,Western Australia,South Africa,dish array,frequency 50.0 MHz to 350.0 MHz

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