Fig. 5
Photospheric transverse velocity derived through LCT analysis of the SDO/HMI magnetograms. The background is the average line-of-sight magnetic field with positive (white) and negative (black) polarities. Arrows represent the transverse velocity, where black/white is located on the positive/negative polarity. The time interval for averaging the line-of-sight magnetic field is 02:25–02:50 UT.
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