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. 1.

pB (a) and UV (b) radial profiles at the north polar coronal hole, as measured by Metis (red dots) and UVCS (blue dots). The horizontal dashed line indicates the interplanetary H I Lyα intensity.

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