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Fig. 4


Vertical cuts through typical magnetic flux concentrations in the six simulations with B0 = 100 G. The grey scale indicates the density ϱ/ ⟨ ϱz relative to the horizontal mean density; the solid (dotted) yellow curve represents the τR = 1 (τR = 0.01) surface; the dashed blue contours indicate iso-B contours of 500, 1000, and 1500 G; the red dash-dotted curves indicate the T/Teff = 0.9, 1.0, and 1.1 surfaces. x and z coordinates are to scale for each panel but differ by more than one order of magnitude for the different stellar models.

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