The Murchison Widefield Array: solar science with the low frequency SKA Precursor

The Murchison Widefield Array: solar science with the low frequency SKA Precursor

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 Observatory in the mid-west of Western Aust...

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Bibliographic Details
Main Authors: Tingay, S. J., Cappallo, Roger J., Corey, Brian E., Goeke, Robert F., Hewitt, Jacqueline N., Kincaid, Barton B., Kratzenberg, Eric W., Lonsdale, Colin John, McWhirter, Stephen R., Morgan, Edward H., Remillard, Ronald Alan, Rogers, Alan E. E., Salah, J. E., Whitney, Alan R., Williams, Christopher Leigh
Other Authors: Haystack Observatory
Format: Article
Language:en_US
Published: IOP Publishing 2014
Online Access:http://hdl.handle.net/1721.1/88453
https://orcid.org/0000-0002-4117-570X
https://orcid.org/0000-0001-7130-208X
https://orcid.org/0000-0003-1941-7458

Internet

http://hdl.handle.net/1721.1/88453
https://orcid.org/0000-0002-4117-570X
https://orcid.org/0000-0001-7130-208X
https://orcid.org/0000-0003-1941-7458

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