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Fig. 2.

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Magnetic flux emergence episode. Panels (a) and (b): LOS magnetograms, respectively, from SST/CRISP and SDO/HMI aligned to SST. Panels (c) and (d): LOS magnetograms from the original SDO/HMI data without and with deconvolution, respectively. Panels (e), (f), (g), and (h): Magnetic flux evolution within the red rectangle for the corresponding magnetograms, showing the unsigned flux (black), the positive flux (blue), and the absolute value of the negative flux (red). In panels (e) and (g), the gray band represents the standard deviation of the unsigned flux measured in the original SST/CRISP and SDO/HMI data, respectively. An animation of this figure is available online showing the time evolution from 08:07 to 08:59 UT.

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