Fig. 4.
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Base simulation results showing the CME evolution in equatorial (left) and meridional (right) planes. Panels (a–d) display the magnetic field component Bz (nT). Panels (e–h) display the radial velocity Vr (km/s), at 2022-03-12 09:59 UT (a–b, e–f) and 2022-03-13 19:59 UT (c–d, g–h). Left panels (a, c, e, g) show a top-down view of the CME propagation on the equatorial plane, while the right-hand panels (b, d, f, h) show the meridional plane, giving a side-on view of its vertical extent and latitudinal structure. The concentric circles indicate heliocentric distance contours and serve as radial reference markers.
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