The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory
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Authors
Sokolowski, M.
Wayth, Randall
Lewis, M.
Date
2016Type
Conference Paper
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We characterize the low frequency radio-frequency interference (RFI) environment at the Murchison Radio-astronomy Observatory (MRO), the location selected for the low-frequency component of the Square Kilometre Array. Data were collected from the BIGHORNS instrument, located at the MRO, which records a contiguous bandwidth between 70 and 300 MHz, between November 2014 to March 2015 inclusive. The data were processed to identify RFI, and we describe a series of statistics in both the time and frequency domain, including modeling of the RFI occupancy and signal power as a series of distribution functions, with the goal of aiding future scientists and operation staff in observation planning.
Citation
Sokolowski, M. and Wayth, R. and Lewis, M. 2016. The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory, in Proceedings of the Global Electromagnetic Compatibility Conference (GEMCCON), Nov 10-12 2015, pp. 1-6. Adelaide, SA: IEEE.
Source Title
Conference Proceedings - GEMCCON 2015: IEEE Global Electromagnetic Compatibility Conference
Department
Department of Electrical and Computer Engineering
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