Fig. 2.

Evolution of the maximum velocity (black) and velocity at the spot boundary vh(1.1 Mm) (red) of the flow field for all analysed active regions. If the maximum velocity is localised at the sunspot boundary, these values are equal to vh(1.1 Mm) and are not visible in the diagram. The abscissa values are given in days with the loss of the penumbra being set as a common point in time.
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