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

doi:10.1088/1742-6596/440/1/012033

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

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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

Description

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

Collections	ANU Research Publications
Date published:	2013
Type:	Conference paper
URI:	http://hdl.handle.net/1885/81406
Source:	Journal of Physics: Conference Series
DOI:	10.1088/1742-6596/440/1/012033

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

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