SKA's sensitivity, snapshot spectroscopic imaging, and angular resolution will enable detection, polarization studies, and thermal association of nonthermal emissions from the quiet solar corona to test acceleration theories and probe coronal heating.
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Unravelling the nonthermal emissions from the quiet solar corona with the SKA
SKA's sensitivity, snapshot spectroscopic imaging, and angular resolution will enable detection, polarization studies, and thermal association of nonthermal emissions from the quiet solar corona to test acceleration theories and probe coronal heating.