Flare ribbon pixels in AIA 1600 Å and 304 Å images show consistent relative photometry, with the brightest pixels rising in under two minutes and decaying in two phases.
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Quantifying Chromosphere Response to Flare Energy Release Using AIA Observations in 1600~\AA\ and 304~\AA\ Passbands
Flare ribbon pixels in AIA 1600 Å and 304 Å images show consistent relative photometry, with the brightest pixels rising in under two minutes and decaying in two phases.