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Fig. 1.

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(a): Full-disk image of EUI in 174 Å (inverted grayscale) superposed with HRIEUV, with the relative positions of Solar Orbiter. (b): Image of HRIEUV (rotated to facilitate the analysis), with the centrally positioned white box (also the FOV of panel d and its enlargement labeled with the target filament position). (c): Multiple jets throughout the filament eruption. (d1)–(d6): Filament evolution in HRIEUV images. Different features are annotated. The dashed blue line in panel d5 indicates the slice position. (e): Intensity profiles (blue) along the slice; the red and yellow curves fitted with a Gaussian indicate the UF and LF position, respectively, and the double-decker filament centers are indicated with dashed lines. (f): Time-space plot of the filament eruption; the UF and LF eruption speeds are labeled, and the time corresponds to panel d5.

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