Table 1
3D model properties.
| Model ID (d3gt57g44) | Box size (Mm3) | Resolution (km3) | Grid points Nx × Ny × Nz | Teff (K) | 〈Bz〉 (G) | Rad. trans. Module |
|---|---|---|---|---|---|---|
| msc600 | 8.0 × 8.0 × 2.3 | 32× 32× 10 … 15 | 250 × 250 × 207 | 5773 ± 9.4 | – | MSCrad |
| n59 | 5.6 × 5.6 × 2.3 | 40 × 40 × 15 | 140 × 140 × 150 | 5774 ± 16 | – | LCFrad |
| m595 | 5.6 × 5.6 × 2.3 | 40 × 40 × 15 | 140 × 140 × 150 | 5775 ± 15 | – | MSCrad |
| b000 | 5.6 × 5.6 × 2.3 | 40 × 40 × 15 | 140 × 140 × 150 | 5750 ± 19 | 0 | MSCrad |
| b200 | 5.6 × 5.6 × 2.3 | 40 × 40 × 15 | 140 × 140 × 150 | 5793 ± 17 | 200 | MSCrad |
Notes. “Model ID” lists the name of a 3D model used in this paper (note all models share the prefix “d3gt57g44”), “Box Size” the geometrical size of its computational domain, “Resolution” the applied grid spacing, “Grid Points” the number of mesh points per dimension, “Teff” the effective temperature of the model, “〈Bz〉” the mean magnetic field component in vertical direction, and “Rad. Trans. Module” the name of the radiation transport module used (see Sect. 2.1 for an explanation). Different from the other models, the msc600 model uses a variable grid spacing in the vertical direction; for that reason the covered range is provided. We note that ‘±’ in “Teff” should not be interpreted as an uncertainty: it is the natural dispersion of effective temperature in the time series illustrating fluctuations between snapshots. Each model has log(g) = 4.44 and solar metallicity.
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