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Velocity-field estimation techniques for on-disk solar coronal bright fronts (CBFs) and shock-wave propagation
Coronal mass ejections (CMEs) are large expulsions of plasma and magnetic fields from the solar corona into the heliosphere. Coronal shock waves are driven by CMEs, and accurate Solar Energetic Particles (SEP) forecasting requires knowing when and where shocks form, how fast they propagate, and how
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