Small-scale EUV features as the drivers of coronal upflows in the quiet Sun

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 4.

SJIs from IRIS showing a bright structure within the upper chromosphere (2796 Å and 1330 Å) and the upper transition region (1400 Å). The upflow region falls on the chromospheric network. No clear structure can be seen in the upper photosphere (2832 Å).

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