arXiv · 1501.05017
Antenna array characterization via radio interferometry observation of astronomical sources
Abstract
We present an in-situ antenna characterization method and results for a "low-frequency" radio astronomy engineering prototype array, characterized over the 75-300 MHz frequency range. The presence of multiple cosmic radio sources, particularly the dominant Galactic noise, makes in-situ characterization at these frequencies challenging; however, it will be shown that high quality measurement is possible via radio interferometry techniques. This method is well-known in the radio astronomy community but seems less so in antenna measurement and wireless communications communities, although the measurement challenges involving multiple undesired sources in the antenna field-of-view bear some similarities. We discuss this approach and our results with the expectation that this principle may find greater application in related fields.
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T. M. Colegate, A. T. Sutinjo, P. J. Hall, S. K. Padhi, R. B. Wayth, J. G. Bij de Vaate, B. Crosse, D. Emrich, A. J. Faulkner, N. Hurley-Walker, E. de Lera Acedo, B. Juswardy, N. Razavi-Ghods, S. J. Tingay, A. Williams. 2015-01-20. Antenna array characterization via radio interferometry observation of astronomical sources. https://doi.org/10.1109/cama.2014.7003436
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