Fig. 5.

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Overview of STX2023-04-22T22:21 showing STIX light curves (panel a) and two EUI/FSI short-exposure frames (panels b and c). The first short-exposure frame shows four non-thermal sources both in HXR (blue contours, 18–50 keV) and EUV 174 Å emission. The red contours show the 6–10 keV thermal HXR emission. We interpret that emission in the later EUI frame as the previously heated flare loop that has cooled sufficiently such that it was observable in the 174 Å passband. The thermal emission from STIX at this time originates from an elongated source that only appears in the EUI/FSI short-exposure frame at 23:00:50 (not shown). As before, the maps shown here have been rotated such that north is up.

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