Slow solar wind sources - High-resolution observations with a quadrature view

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 5.

Highly dynamical small-scale structures are observed in the transition region with IRIS SJI 2796 (panel a) and IRIS SJI 1400 (panel b). The rectangle shows the Hinode/EIS field of view. The contour inside it presents ROI-A that spatially corresponds to the coronal upflow region with a projected velocity v < −5 km s⁻¹.

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