Coronal mass ejection precursors in Sun-like stars: Flux rope modelling and coronal signatures

Open Access

Fig. 5.

Left vertical axis: Evolution of the average vertical velocity inside the MFR, weighted by normalised area ${\hat{v}}_{y}$ $Mathematical equation: $ \hat{v}_y $$ (black lines). Squares, circles, and diamonds represent cases C1, C2, and ${C 2}_{T}^{-}$ $Mathematical equation: $ \mathrm{C2}_{T}^{-} $$ , respectively. Symbol colours indicate the height of the MFR centre. Right vertical axis: MFR centre velocity values v_y, MFR (grey lines).

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