Table 1.
Global properties for the considered cases.
| Case | F1a | F1b | F3 | F5 |
|---|---|---|---|---|
| (Nr, Nθ, Nϕ) | (1205, 512, 1024) | (1205, 1024, 2048) | (1205, 1024, 2048) | (1205, 1024, 2048) |
| Ω0 (Ω⊙) | 1 | 1 | 3 | 5 |
| νtop (cm2 s−1) | 3.5 × 1013 | 1.05 × 1013 | 1.75 × 1013 | 1.05 × 1013 |
| κtop (cm2 s−1) | 1.4 × 1014 | 4.2 × 1013 | 7 × 1013 | 4.2 × 1013 |
| rt (cm) | 8.9 × 1010 | 8.9 × 1010 | 8.9 × 1010 | 8.9 × 1010 |
| Longest time series (day) | 117 | 52 | 48 | 130 (280) |
Notes. The last row of the table specifies the longest vr time series we have for each case (with a time sampling dt below 1250s to keep the Nyquist frequency of the series above Nmax = 400 μHz, see Sect. 4.2.), with outputs saved for one depth every 1% of the stellar radius. The value between parenthesis in the F5 case correspond to the length of the time series for which we save outputs only at r = 0.13 R⋆. This time series is used in Sects. 4.4 and 4.5.
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