Understanding the global structure of the September 5, 2022, coronal mass ejection using sunRunner3D | Journal of Space Weather and Space Climate

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Figure 8

Radial velocity (km s⁻¹) as a function of heliocentric distance (AU) for the traces marked in Figure 7 but at the times of (a) 10 h, (b) 15 h, and (c) 20 h. The profiles are colour-coded according to the same colours as in Figure 7, with the legend providing the numerical integer values.

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