First polar observations of the fast solar wind with the Metis – Solar Orbiter coronagraph: Role of 2D turbulence energy dissipation in the wind acceleration

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 2.

n_e (a) and V_out (b) radial profiles at the north polar coronal hole, as measured with Metis (red dots) and UVCS (blue dots) data, compared with some results from previous literature (marked with different colored lines, as listed in the legend). The thick solid black curve in panel (b) denotes the NI MHD turbulence + SW model applied to the joint UVCS – Metis V_out estimates.

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