This paper discusses observational, calibration, and imaging requirements for solar and heliospheric science with the SKA radio telescope.
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Recent sub-second imaging spectroscopy of solar radio burst fine structures challenges existing theoretical models, with the SKA positioned to enable new frameworks for electron acceleration and coronal turbulence.
citing papers explorer
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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.
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Solar Radio Burst Fine Structures
Recent sub-second imaging spectroscopy of solar radio burst fine structures challenges existing theoretical models, with the SKA positioned to enable new frameworks for electron acceleration and coronal turbulence.