Fig. 18.
Heliospheric view in December 2022 with 3DView. The Parker field lines (at V = 500 km s−1) connected to Solar Orbiter and PSP are shown in yellow. The surface around the Sun (here at 30Rs) is the colour coded solar wind velocity output from the MULTI-VP code (Pinto & Rouillard 2017). The Solar OrbiterHI field of view is displayed in green.
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