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The Murchison widefield array: Solar science with the low frequency SKA precursor

Tingay, Steven; Oberoi, D; Cairns, Iver Hugh; Donea, A; Duffin, R; Arcus, W; Bernardi, G; Bowman, Judd D; Briggs, Franklin; Deshpande, Avinash; Emrich, David; Greenhill, Lincoln; Hazelton, B; Kaplan, D L; Kincaid, Barton B; Mitchell, Daniel A; Ord, S M; Prabu, T; Rogers, Alan; Roshi, Anish; Srivani, K. S.; Whitney, Alan; Williams, Christopher L


The Murchison Widefield Array is a low frequency (80-300 MHz) SKA Precursor, comprising 128 aperture array elements (known as tiles) distributed over an area of 3 km diameter. The MWA is located at the extraordinarily radio quiet Murchison Radioastronomy

CollectionsANU Research Publications
Date published: 2013
Type: Conference paper
Source: Journal of Physics: Conference Series
DOI: 10.1088/1742-6596/440/1/012033


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