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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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.