Table 2.
Transport processes considered in this work.
| Process | Quantity | Adjusted parameter | Observational constraints |
|---|---|---|---|
| Atomic diffusion | C | – | – |
| Meridional circulation | C & AM | – | – |
| Shear-induced turbulence (R1 or R2) | C & AM | – | – |
| Magnetic torque | AM | K = 7.5 × 1030 erg | Surface rotation of solar-type stars |
| Penetrative convection | C | dov = 0.0325 | Surface Li abundance of young solar-type stars |
| Parametric turbulence | C | log T = 6.42 | Surface Li abundance of MS solar-type stars |
| Vertical viscosity | AM | νadd = 3.5 × 104 cm2 s−1 | Solar rotation profile |
Notes. Transport processes (Col. 1) and values of the free parameters (when relevant) (Col. 3) with the corresponding observational constraints adjusted (Col. 4) for the best model for solar-type stars (Paper I) and adopted in this study. The flags in Col. 2 indicate the transported quantity (C for chemicals and AM for angular momentum).
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