EUV kernels in an M2.5 flare are unresolved at scales ≲1 Mm² and exhibit heating times of less than a few seconds.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
High-resolution coronagraph images resolve CME substructures and fast circular wave-trains interpreted as quasi-periodic propagating fast magnetosonic modes.
citing papers explorer
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Small-Scale and Transient EUV Kernels in Solar Flare Ribbons
EUV kernels in an M2.5 flare are unresolved at scales ≲1 Mm² and exhibit heating times of less than a few seconds.
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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.