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Fig. 9


Time sequence of the AIA images during the main reconnection episode of the flare. Each column corresponds to an AIA channel observing the flare (from left to right: 131, 171, and 1600Å) and each row displays a time during the main null-point reconnection episode (from top to bottom: 15:14:21 UT, 15:16:09 UT, 15:21:00 UT and 15:27:57 UT). The overplotted field lines are coloured as described in Fig. 8. The CEA projection is used for the co-alignment. The field of view for the magnetic field data is x = [550,750] ′′, y = [10,190] ′′.

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