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Fig. 6


Density, temperature, plasma-β, and velocity distributions at t = 10   ks for the weak magnetic field model Rnd20. The colors blue/red are used for low/high values, and in particular ρ ∈  [10-13,   10-11]    g   cm-3, T ∈  [0,   4]    MK, β ∈  [10-2,   102], vx ∈  [−5,   5]    km   s-1, vz ∈  [−500,   0]    km   s-1, and Q ∈  [0,   1]. The 1% density perturbations that are applied to this model are too weak to be visible. Due to the saturation of the density color, the exponential profile of the chromosphere cannot be seen.

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