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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Pith papers citing it
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astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
NUV continuum enhancements occur in 80 of 234 solar flares, concentrated on ribbon edges during the impulsive phase, with magnitude rising with flare class.
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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Statistical Study of Balmer Continuum Enhancement in Solar Flares
NUV continuum enhancements occur in 80 of 234 solar flares, concentrated on ribbon edges during the impulsive phase, with magnitude rising with flare class.