Fig. A.1.
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Equatorial planes in the 3D dynamic heliosphere simulations with the cone (left) and spheromak (right) CMEs. The radial velocity and velocity divergence are plotted in the background. The contour of the CME tracing function, TRF, is overplotted. The snapshot corresponds to the observed arrival of the shock at BepiColombo. The BepiColombo location is indicated on the figure with ‘B’.
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