and bottom panels in Fig. \[fig:spectraB\] might support this interpretation.

Condensation: Time Evolution {#sec:chrom_time}
----------------------------

We now focus on the dynamics displayed by multiple flaring pixels, in particular those comprising the ribbon between the y=\[114$''$,127$''$\] positions in Fig. \[fig:ltspec\]. These are the same pixels analyzed in Paper I.

Using the fits described in Section \[sec:chrom\_spectra\], we derive the centroid of the second, shifted Gaussian component for each line, pixel and time step. The velocity scale for each line is obtained with respect to the rest wavelength shown in Figs. \[fig:spectraA\] and \[fig:spectraB\]. To remove fits where the velocity determination could be biased by nearby lines or low signal, we discarded the fits when the total intensity of the shifted component was below 30% of the maximum reached in any given pixel. This also removes some of the influence of the instrumental point spread function (PSF) described in Appendix \[sec:appendixB\].

To find commonalities in the flow evolution of the different pixels and lines, in analogy to Paper I we perform a superposed-epoch analysis, aligning the velocity-time curve for each pixel and spectral line to a common zero time. The latter is defined as the time at which maximum shift of the 