Fig. 2.

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Change of the maximum height of field lines rooted in the photosphere at time t = 600 s compared to their initial height, Δh = h(t = 600)−h(t = 0). Panels from left to right show the result for the simulations initialized at t−24, t−12 and the reference time, respectively, using Ωopt. The orange solid (black dashed) contour indicates field lines of lengths 100 (200) Mm. The gray scale shows the vertical component of photospheric magnetic field saturated at ±0.1 T.
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