Fig. 5
HMI magnetograms showing the magnetic flux emergence at the site of the blob eruption. The magnetogram at 23:00 UT is overlaid with the AIA 1600 Å EUV flare ribbons near the flux emergence site. Bottom: the temporal evolution of positive, unsigned negative, and total unsigned flux derived from the HMI magnetograms on 25 March 2011. Two vertical dotted lines indicate the duration of blob eruption and the associated flare.
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