First results from Automated Imaging Routine for Compact Arrays for Radio Sun

At low radio frequencies the solar corona is very dynamic in both spectral and temporal domains. To capture the fine details of this complex dynamics, imaging studies at high temporal and spectral resolution are necessary. The advent of the new instruments like the Murchison Widefield Array (MWA; Ti...

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Published inProceedings of the International Astronomical Union Vol. 13; no. S340; pp. 159 - 160
Main Authors Mondal, Surajit, Mohan, Atul, Oberoi, Divya, Benkevitch, Leonid, Lonsdale, Colin J., Morgan, John, Crowley, Meagan, Cairns, Iver
Format Journal Article
LanguageEnglish
Published Cambridge, UK Cambridge University Press 01.02.2018
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Summary:At low radio frequencies the solar corona is very dynamic in both spectral and temporal domains. To capture the fine details of this complex dynamics, imaging studies at high temporal and spectral resolution are necessary. The advent of the new instruments like the Murchison Widefield Array (MWA; Tingay et al. 2013, Bowman et al. 2013), is now making this possible.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921318001679