Connecting Solar Orbiter remote-sensing observations and Parker Solar Probe in situ measurements with a numerical MHD reconstruction of the Parker spiral

Solar Orbiter First Results (Nominal Mission Phase)

Open Access

Fig. 4.

Comparison between observed (squares) and RIMAP-modelled (red line) proton number density (top panel) and outflow velocity (bottom panel) along the same streamline, from 3 to 25 R_⊙. Black and red squares refer to Metis and PSP estimates, respectively.

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