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. 3.

Comparison between PSP-measured (black) and RIMAP-modelled (red) solar wind parameters from January 15 to 21, 2021. From top to bottom, the panels display the proton number density, the solar wind speed, the radial, and the tangential components of the interplanetary magnetic field (RTN).

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