Characterization of SKA-AAlow antenna elements in the array environment

The electromagnetic modeling and testing is presented for antenna elements devoted to the low frequency band of the Square Kilometre Array (SKA) telescope [1]. Covering a band from 70 to 450 MHz, these elements consist on a log-periodic dipole array (LPDA) model and they have been designed for maximum sensitivity across the band in the region +/- 45 degrees from zenith. A 16-element array (AAVS0 - Aperture Array Verification System 0) has been built in Lords Bridge, Cambridge, UK, and it is being tested to validate the electromagnetic properties of the antenna elements and front-end. We focus on the modeling of these elements and compare simulated and measured data for simulation software validation.

[1]  Nima Razavi-Ghods,et al.  Non-periodic arrays for radio-astronomy applications , 2011, 2011 IEEE International Symposium on Antennas and Propagation (APSURSI).

[2]  H. C. Reader,et al.  SKA AA-low front-end developments (At Cambridge University) , 2012, 2012 6th European Conference on Antennas and Propagation (EUCAP).

[3]  Eloy de Lera Acedo,et al.  Broadband differentially fed tapered slot antenna array for radio astronomy applications , 2009, 2009 3rd European Conference on Antennas and Propagation.

[4]  Walton C. Gibson,et al.  The Method of Moments in Electromagnetics , 2007 .

[5]  Nima Razavi-Ghods,et al.  Fast MBF based method for large random array characterization , 2009, 2009 IEEE Antennas and Propagation Society International Symposium.

[6]  D. Gonzalez-Ovejero,et al.  Interpolatory Macro Basis Functions Analysis of Non-Periodic Arrays , 2011, IEEE Transactions on Antennas and Propagation.

[8]  R. Schilizzi The Square Kilometre Array , 2006, Proceedings of the International Astronomical Union.

[9]  S. Wijnholds,et al.  Calibratability and its impact on configuration design for the LOFAR and SKA phased array radio telescopes , 2011 .