Topical Issue - Space Weather Instrumentation
Open Access
Technical Article

Fig. 3

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Simulated CME kinematic profiles. Solid lines indicate the unperturbed torus instability. Dashed lines from right to left correspond to increasing durations (6 τA up to 10τA) of an upward, linearly rising velocity perturbation, resulting in fundamentally different acceleration profiles. The SunCET FOV (0–4 R; indicated in light blue) covers and extends beyond this simulation. Adapted from Schrijver et al. (2008), Figure 7.

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