SKA's sensitivity, bandwidth and frequency coverage will enable routine radio diagnostics of CME magnetic fields that current precursors can only demonstrate sporadically, improving space-weather models.
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This paper discusses observational, calibration, and imaging requirements for solar and heliospheric science with the SKA radio telescope.
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Role of SKA in Advancing Remote Measurements of Magnetic Fields of Solar Coronal Mass Ejections
SKA's sensitivity, bandwidth and frequency coverage will enable routine radio diagnostics of CME magnetic fields that current precursors can only demonstrate sporadically, improving space-weather models.
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State-of-the-art Observation, Calibration, and Imaging Framework for Solar and Heliospheric Sciences with SKA
This paper discusses observational, calibration, and imaging requirements for solar and heliospheric science with the SKA radio telescope.