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Fig. 2.

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Hard X-ray emission of the November 11, 2022 event in the time window between 01:30:00 and 01:32:00 UT. Left panel: STIX light-curves corresponding to three energy channels. Right panel: level curves of the count emission provided by MEM_GE and superimposed to the 1600 Å emission recorded by SDO/AIA (the AIA data have been appropriately reprojected in order to account for the Solar Orbiter and SDO different vantage points). The red level curves correspond to the thermal emission in the energy range of 4 − 6 keV, while the green ones correspond to the non-thermal emission in the energy range of 22 − 25 keV.

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