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

Published online by Cambridge University Press:  27 November 2018

Surajit Mondal
Affiliation:
National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune, India. email:[email protected]
Atul Mohan
Affiliation:
National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune, India. email:[email protected]
Divya Oberoi
Affiliation:
National Centre for Radio Astrophysics, Tata Institute of Fundamental Research, Pune, India. email:[email protected]
Leonid Benkevitch
Affiliation:
MIT Haystack Observatory, Westford, Massachusetts, USA.
Colin J. Lonsdale
Affiliation:
MIT Haystack Observatory, Westford, Massachusetts, USA.
John Morgan
Affiliation:
Curtin University, Perth, Australia.
Meagan Crowley
Affiliation:
University of Massachusetts, Massachusetts, USA.
Iver Cairns
Affiliation:
University of Sydney, Sydney, Australia.
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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.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

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