Role of SKA in Advancing Remote Measurements of Magnetic Fields of Solar Coronal Mass Ejections

Coronal Mass Ejections (CMEs) are large expulsions of magnetized plasma from the Sun into interplanetary space and are the primary drivers of extreme space weather variations.

The strength and topology of CME magnetic fields largely determine their impact on Earth.

Although visible-light coronagraphs routinely observe CMEs and provide their geometric and kinematic properties, they cannot directly measure CME vector magnetic fields.

These fields evolve from initiation through the inner heliosphere due to interactions with other CMEs, coronal structures, and the ambient solar wind, leading to significant structural deformation.

Such evolution complicates predictions of the CME magnetic field at Earth.

Accurate measurements of CME magnetic fields in the corona and heliosphere are therefore essential for advancing space weather forecasting.

Radio observations spanning MHz to GHz frequencies provide a powerful remote-sensing approach for measuring CME magnetic fields from the ground.

Recent observations with Square Kilometre Array (SKA) precursors and pathfinder instruments, as well as other new-generation facilities, have demonstrated the potential of these radio techniques for CME magnetic-field diagnostics.

At the same time, these studies have highlighted several limitations of current instruments.

The higher sensitivity, wider instantaneous bandwidth, and broader frequency coverage of the SKA will open a new observational window, enabling these techniques to be fully exploited for constraining SpWx models and improving predictive accuracy.

However, such observations are non-standard and require special consideration in scheduling, calibration, and imaging.

Developments achieved with SKA precursors and pathfinders are paving the way for robust CME magnetic-field measurements with the SKA.