Fig. 1.
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Context view of AR13470 (top row) and AR13468 (bottom row) observed on 19 and 20 October 2023, respectively. Left column: WoW-enhanced EUI/HRI-174Å images with the slits (white lines) used for the coronal oscillation analysis. Middle column: Stokes-I continuum from PHI/HRT. Right column: PHI/HRT inverted line of sight (LOS) component of the magnetic field, linearly scaled between −500 G (black colours) to 500 G (white colours). The white ellipse shows the re-projected SST/CRISP FOV. The thin white dashed lines represent the helioprojective coordinate frame as seen from Solar Orbiter.
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