SKA's higher sensitivity and bandwidth will enable fuller exploitation of radio methods for measuring CME magnetic fields and improving space weather predictions.
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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.
citing papers explorer
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Role of SKA in Advancing Remote Measurements of Magnetic Fields of Solar Coronal Mass Ejections
SKA's higher sensitivity and bandwidth will enable fuller exploitation of radio methods for measuring CME magnetic fields and improving space weather predictions.
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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.