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dc.contributor.authorSokolowski, M.
dc.contributor.authorWayth, Randall
dc.contributor.authorLewis, M.
dc.date.accessioned2017-01-30T15:06:30Z
dc.date.available2017-01-30T15:06:30Z
dc.date.created2016-05-08T19:30:24Z
dc.date.issued2016
dc.identifier.citationSokolowski, 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.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/43307
dc.identifier.doi10.1109/GEMCCON.2015.7386856
dc.description.abstract

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.

dc.titleThe statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory
dc.typeConference Paper
dcterms.source.titleConference Proceedings - GEMCCON 2015: IEEE Global Electromagnetic Compatibility Conference
dcterms.source.seriesConference Proceedings - GEMCCON 2015: IEEE Global Electromagnetic Compatibility Conference
dcterms.source.isbn9781467385480
curtin.departmentDepartment of Electrical and Computer Engineering
curtin.accessStatusFulltext not available


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