Open Access
Table A.1
Model properties of M3DIS solar models.
| Model | Teff | log(g) | [Fe/H] | composition | HD solver | EoS | Nbins |
|---|---|---|---|---|---|---|---|
| M3DIS (A) | 5923.5 ± 7.7 K | 4.44 | 0.0 | Magg et al. (2022) | HLLC | Gerber et al. (2023)* | 7 |
| M3DIS (B) | 5858.9 ± 14.8 K | 4.44 | 0.0 | Magg et al. (2022) | HLLC | Gerber et al. (2023)* | 7 |
| M3DIS (C) | 5786.0 ± 9.6 K | 4.44 | 0.0 | Magg et al. (2022) | HLLC | Gerber et al. (2023)* | 7 |
| M3DIS (D) | 5808.2 ± 14.8 K | 4.44 | 0.0 | Magg et al. (2022) | HLLC | Gerber et al. (2023)* | 7 |
| Stagger | 5768.51 K | 4.44 | 0.0 | Asplund et al. (2009) | Runge-Kutta | Mihalas et al. (1988) | 12 |
| CO5BOLD | 5781 K | 4.44 | 0.0 | Grevesse & Sauval (1998), except CNO | Roe Riemann | Wolf (1983) | 12 |
Notes.(*) The EoS is computed using Turbospectrum2020, which is consistent with MARCS in terms of chemical equilibrium. For all models presented in this table the opacities from Gustafsson et al. (2008) were used.
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