Fig. 9
Profiles of Fe i 6301.5 Å computed for four events (see Fig. 3) after the images at every wavelength were degraded to the resolution of the SP/SOT Hinode. Rows from top to bottom correspond to Events 1−4, respectively. Columns correspond to five locations of the snapshot on the solar disk. We also the wavelength axis in terms of corresponding Doppler shifts.
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