Many dark H-alpha fibrils around magnetic network are statistically associated with preceding rapid blue and red excursions, suggesting they are cooling aftermaths of type II spicule heating events.
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Solar H-alpha features with hot onsets. IV. Network fibrils
Many dark H-alpha fibrils around magnetic network are statistically associated with preceding rapid blue and red excursions, suggesting they are cooling aftermaths of type II spicule heating events.