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. (Contributor), Cappallo, Roger J. (Contributor), Corey, Brian E. (Contributor), Goeke, Robert F. (Contributor), Hewitt, Jacqueline N. (Contributor), Kincaid, Barton B. (Contributor), Kratzenberg, Eric W. (Contributor), Lonsdale, Colin John (Contributor), McWhirter, Stephen R. (Contributor), Morgan, Edward H. (Contributor), Remillard, Ronald Alan (Contributor), Rogers, Alan E. E. (Contributor), Salah, J. E. (Contributor), Whitney, Alan R. (Contributor), Williams, Christopher Leigh (Contributor)
Other Authors: Haystack Observatory (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2014-07-22T12:57:35Z.
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