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, Steven, Oberoi, D., Cairns, I., Donea, A., Duffin, R., Arcus, Wayne, Bernardi, G., Bowman, J., Briggs, F., Bunton, J., Cappallo, R., Corey, B., Deshpande, A., deSouza, L., Emrich, David, Gaensler, B., Goeke, R., Greenhill, L., Hazelton, B., Herne, David, Hewitt, J., Johnston-Hollitt, M., Kaplan, D., Kasper, J., Kennewell, J., Kincaid, B., Koenig, R., Kratzenberg, E., Lonsdale, C., Lynch, Mervyn, McWhirter, S., Mitchell, D., Morales, M., Morgan, E., Ord, S., Pathikulangara, J., Prabu, T., Remillard, R., Rogers, A., Roshi, A., Salah, J., Udaya-Shankar, N., Srivani, K., Stevens, J., Subrahmanyan, R., Waterson, Mark, Wayth, Randall, Webster, R., Whitney, A., Williams, A., Williams, C., Wyithe, J.
Format: Conference Paper
Published: Institute of Physics Publishing Ltd. 2013
Subjects:
Neutral hydrogen
Low frequency arrays
Initial operation
Aperture arrays
Brightness temperatures
Propagation effect
Western Australia
Radio sources
Online Access:http://hdl.handle.net/20.500.11937/35884

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