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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 ,
Atul Mohan Open the ORCID record for Atul Mohan [Opens in a new window] ,
Divya Oberoi Open the ORCID record for Divya Oberoi [Opens in a new window] ,
Leonid Benkevitch ,
Colin J. Lonsdale ,
John Morgan ,
Meagan Crowley  and
Iver Cairns
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
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 159 - 160
Copyright
Copyright © International Astronomical Union 2018 

References

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