Fig. 10.
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Overview of the coronal and solar wind configuration obtained from EUHFORIA. (a) BR at the source surface height (2.5 R⊙) derived from the PFSS model in EUHFORIA. (b) BR at the heliospheric inner boundary (0.1 au) derived from the coronal model in EUHFORIA. (c) and (d) BR (scaled by r2, where r is the distance from the Sun) and VR in the heliocentric equatorial plane and in the Solar Orbiter meridional plane from EUHFORIA around the time the ICME is observed to arrive at Solar Orbiter. An animated version of panels c and d is available online. The animations run from June 4, 2020, 00:03 UT to June 14, 2020, 00:03 UT.
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