Figure 4
From: Small-Scale Upflows in a Coronal Hole – Tracked from the Photosphere to the Corona
IRIS slit-jaw images, each column represents the time, which is the closest to the Hinode/EIS rasters in Figure 1.
Figure 4 | Solar Physics
From: Small-Scale Upflows in a Coronal Hole – Tracked from the Photosphere to the Corona
IRIS slit-jaw images, each column represents the time, which is the closest to the Hinode/EIS rasters in Figure 1.