Fig. 15.
Model of multi-layers of the mini-flare atmosphere during the jet reconnection in a BP region. The model is based on the observations of emission or absorption of the IRIS lines and continua, and the images of AIA in the multi-temperature filters in the mini-flare (UV burst) around 02:04:28 UT ± 60 s (right column). The y-axis is along the LOS. The LOS successively crosses cool and hot layers (white for minimum of temperature, yellow for chromosphere until transition region temperatures, red for coronal temperatures).
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