Observing the Sun with the Murchison Widefield Array

Observing the Sun with the Murchison Widefield Array

The Sun has remained a difficult source to image for radio telescopes, especially at the low radio frequencies. Its morphologically complex emission features span a large range of angular scales and the emission mechanisms involved, span a wide range in brightness temperatures. In addition, time and...

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Bibliographic Details
Main Authors: Oberoi, D., Sharma, R., Bhatnagar, S., Lonsdale, C., Matthews, L., Cairns, I., Tingay, Steven, Benkevitch, L., Donea, A., White, S., Bernardi, G., Bowman, J., Briggs, F., Cappallo, R., Corey, B., Deshpande, A., Emrich, D., Gaensler, B., Goeke, R., Greenhill, L., Hazelton, B., Johnston-Hollitt, M., Kaplan, D., Kasper, J., Kratzenberg, E., Lynch, Mervyn, McWhirter, S., Mitchell, D., Morales, M., Morgan, E., Offringa, A., Ord, Stephen, Prabu, T., Rogers, A., Roshi, A., Salah, J., Shankar, N., Srivani, K., Subrahmanyan, R., Waterson, M., Wayth, Randall, Webster, R., Whitney, A., William, A., Williams, C.
Format: Conference Paper
Published: Institute of Electrical and Electronics Engineers Inc. 2014
Online Access:http://hdl.handle.net/20.500.11937/26195

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