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Fig. A.1.

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Temporal evolution of bisector velocities calculated from different intensity levels at the location of the dark core. The left plot shows the velocities of granule IBIS 6, and the right plot shows results from granule IBIS 3. The left dashed line marks the time at which the dark core is visible for the first time, and the right dashed line marks the time at which the exploding granule is split into a new generation of granules.

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