Fig. 3.
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Panel (a): equatorial (left) and meridional (right) snapshots of the radial solar wind speed from EUHFORIA. Panel (b): comparison of in situ plasma and magnetic field between observation and EUHFORIA simulation for the 2022 June 7 event. The panels from top to bottom present the solar wind proton number density, the solar wind speed, and the magnetic field magnitude. The blue and black lines show the EUHFORIA simulation results and measurements from Solar Orbiter, respectively.
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