The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory

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 record...

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Main Authors: Sokolowski, M., Wayth, Randall, Lewis, M.
Format: Conference Paper
Published: 2016
Online Access:http://hdl.handle.net/20.500.11937/43307
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author Sokolowski, M.
Wayth, Randall
Lewis, M.
author_facet Sokolowski, M.
Wayth, Randall
Lewis, M.
author_sort Sokolowski, M.
building Curtin Institutional Repository
collection Online Access
description 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.
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spelling curtin-20.500.11937-433072018-03-29T09:07:47Z The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory Sokolowski, M. Wayth, Randall Lewis, M. 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. 2016 Conference Paper http://hdl.handle.net/20.500.11937/43307 10.1109/GEMCCON.2015.7386856 restricted
spellingShingle Sokolowski, M.
Wayth, Randall
Lewis, M.
The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory
title The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory
title_full The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory
title_fullStr The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory
title_full_unstemmed The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory
title_short The statistics of low frequency radio interference at the Murchison Radio-astronomy Observatory
title_sort statistics of low frequency radio interference at the murchison radio-astronomy observatory
url http://hdl.handle.net/20.500.11937/43307