Coronal dimmings from CMEs appear as drops in Sun-as-a-star differential emission measure at 10^5.7 to 10^6.3 K after gradual-phase correction.
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High-resolution coronagraph images resolve CME substructures and fast circular wave-trains interpreted as quasi-periodic propagating fast magnetosonic modes.
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Signatures of coronal mass ejections in differential emission measure analysis of the Sun as a star
Coronal dimmings from CMEs appear as drops in Sun-as-a-star differential emission measure at 10^5.7 to 10^6.3 K after gradual-phase correction.
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A view of the evolution of a CME and the associated wave-trains at high spatial and temporal resolution
High-resolution coronagraph images resolve CME substructures and fast circular wave-trains interpreted as quasi-periodic propagating fast magnetosonic modes.