Extended Data Figure 2: Example of a mini-filament jet.
A large coronal jet produced in conjunction with the eruption of a mini-filament23, as seen by the Solar Dynamics Observatory’s Atmospheric Imaging Assembly in Fe xii at wavelength λ = 193 Å. a–c, Images prior to the jet (a), during the jet (b) and after the jet (c). The inferred coronal loop structure is depicted in white in a. We are grateful to R. L. Moore for providing the unpublished video from which these images were extracted.
