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Table 1

Parameters for two-dimensional hydrodynamic simulations of the young sun.

Inner radius (R) Outer radius (R) ro,top (R) wo (% R) τconv(106 s) Time span (τconv) Grid type

Low1 0.41 (small) 0.91 0.50 9.4 3.21 ± 2.10 358 uniform
Low2 0.31 (small) 0.91 0.44 3.7 1.52 ± 0.47 465 uniform
Low3 0.21 (medium) 0.94 0.45 4.0 1.40 ± 0.34 686 uniform
Low4 0.10 (large) 0.97 0.45 2.9 2.66 ± 0.75 338 uniform
Low5 0.21 (medium) 0.97 0.45 3.4 2.07 ± 0.32 330 uniform
Low6 0.10 (large) 0.94 0.45 4.2 1.61 ± 0.66 473 uniform
Low7 0.47 (none) 1.00 1.29 ± 0.40 432 uniform
Low8 0.21 (medium) 1.00 0.44 2.6 1.88 ± 0.16 68 uniform
Low9 0.21 (medium) 1.00 0.47 7.7 0.88 ± 0.20 69 spliced
Hi1 0.24 (medium) 0.94 0.52 13.5 1.17 ± 0.12 157 uniform
Hi2 0.10 (large) 0.97 0.53 16.6 1.20 ± 0.15 85 uniform
Hi3 0.21 (medium) 0.97 0.51 11.3 1.08 ± 0.22 163 uniform
Hi4 0.21 (medium) 1.00 0.58 14.7 0.91 ± 0.23 49 uniform
Hi5 0.21 (medium) 1.00 0.54 13.1 0.72 ± 0.07 59 spliced
ExH2 0.10 (large) 0.97 0.56 15.1 0.91 ± 0.07 18 uniform

Notes. The inner and outer radius of the spherical shell are given in units of the total radius of the young sun R. The amount of the radiative zone included is categorized in terms of a small, medium, or large amount, or none. Diagnostic results are summarized, including the outer radius ro,top of the overshooting layer, the width of the overshooting layer wo, and the convective turnover time τconv. The total time span and the type of grid used for each simulation is also indicated. The type of grid is linked to the type of boundary condition at the surface.

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