Figure 3
From: Small-Scale Upflows in a Coronal Hole – Tracked from the Photosphere to the Corona
SDO/AIA standard deviation maps, each column represents one time, which is the closest to the Hinode/EIS rasters in Figure 1.
Figure 3 | Solar Physics
From: Small-Scale Upflows in a Coronal Hole – Tracked from the Photosphere to the Corona
SDO/AIA standard deviation maps, each column represents one time, which is the closest to the Hinode/EIS rasters in Figure 1.