Fig. 1.
Temporal variation of the magnetic flux and AIA 193 intensity of the CBP along its full lifetime. Images at the top: HMI saturated at ±100 G (top row) and AIA 193 (bottom row). Bottom panel: AIA 193 intensity and LOS magnetic flux of the positive and negative polarities. Each curve is normalized to its maximum. The grey area highlights a period of magnetic flux and coronal emission increase, part of which is covered by the FISS data and is analysed here in detail.
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