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Fig. A.1.

image

Identification of the CME boundaries in EUHFORIA time series at various heliocentric distances. At each heliocentric distance, the proton, βp, magnetic field intensity, B, speed, v, and proton number density, np, are provided. In all panels, the arrival time of the CME-driven shock is marked by the dashed blue line. Top panel: the boundaries of the magnetic ejecta identified by imposing different βp thresholds are marked by coloured vertical lines, while the ultimate boundaries of the magnetic ejecta obtained by applying the threshold condition βp ≤ 0.5 are marked as continuous blue lines in the second, third, and fourth panels.

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