Spectroscopic Imaging of the Sun with MeerKAT: Opening a New Frontier in Solar Physics
Devojyoti Kansabanik, Surajit Mondal, Divya Oberoi, James O. Chibueze,, N. E. Engelbrecht, R. D. Strauss, Eduard P. Kontar, Gert J. J. Botha, P. J., Steyn, Amore E. Nel

TL;DR
This paper presents the first spectroscopic images of the Sun using MeerKAT, demonstrating high-fidelity imaging capabilities across a broad frequency range and opening new avenues for solar physics research.
Contribution
It provides the first spectroscopic images of the Sun with MeerKAT, validating their quality and exploring flux recovery at various frequencies, thus paving the way for advanced solar studies.
Findings
MeerKAT can recover nearly all flux at frequencies below 900 MHz.
High morphological similarity between observed and simulated images.
Potential to correct for missing flux at higher frequencies.
Abstract
Solar radio emissions provide several unique diagnostics to estimate different physical parameters of the solar corona, which are otherwise simply inaccessible. However, imaging the highly dynamic solar coronal emissions spanning a large range of angular scales at radio wavelengths is extremely challenging. At GHz frequencies, MeerKAT radio telescope is possibly globally the best-suited instrument at present for providing high-fidelity spectroscopic snapshot solar images. Here, we present the first published spectroscopic images of the Sun made using the observations with MeerKAT in the 880-1670 MHz band. This work demonstrates the high fidelity of spectroscopic snapshot MeerKAT solar images through a comparison with simulated radio images at MeerKAT frequencies. The observed images show extremely good morphological similarities with the simulated images. Our analysis shows that below…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
