Table 1.
Summary of the runs.
Run | Prot [days] | Ta [108] | urms [m s−1] | Brms [kG] | Co | Co(ω) | Rat | Re | Pe | ReM | τsim [years] | DR | Grid |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
HD1 | − | − | 18 | − | − | − | 6.5 × 105 | 189 | 37 | − | 302 | − | 2883 |
RHD1 | 433 | 0.16 | 17 | − | 0.6 | 0.1 | 2.3 × 106 | 181 | 36 | − | 58 | Anti-solar | 2883 |
RHD2 | 144 | 1.4 | 15 | − | 1.9 | 0.2 | 1.7 × 106 | 159 | 31 | − | 37 | Solar-like | 2883 |
RHD3 | 43 | 16 | 15 | − | 6.4 | 0.9 | 4.8 × 106 | 159 | 31 | − | 36 | Solar-like | 2883 |
RHD4 | 14 | 144 | 9.0 | − | 31 | 3.0 | 1.3 × 107 | 96 | 19 | − | 220 | Solar-like | 2883 |
RHD5 | 4.3 | 1600 | 5.7 | − | 166 | 11 | 7.9 × 107 | 61 | 12 | − | 209 | Solar-like | 2883 |
MHD0 | − | − | 18 | No dynamo | − | − | 6.5 × 105 | 189 | 37 | 95 | 87 | − | 2883 |
MHD1 | 433 | 0.16 | 14 | 11 | 0.7 | 0.1 | 1.2 × 106 | 145 | 29 | 72 | 143 | Anti-solar | 2883 |
MHD1h | 433 | 1.4 | 14 | 12 | 0.7 | 0.1 | 3.6 × 106 | 293 | 58 | 146 | 79 | Anti-solar | 5763 |
MHD2 | 144 | 1.4 | 14 | 4.5 | 2.0 | 0.3 | 1.7 × 106 | 152 | 30 | 76 | 107 | Solar-like | 2883 |
MHD3 | 43 | 16 | 10 | 10 | 9.1 | 1.2 | 3.2 × 106 | 111 | 22 | 55 | 134 | Solar-like | 2883 |
MHD3h | 43 | 64 | 10 | 12 | 9.4 | 1.4 | 8.0 × 106 | 215 | 43 | 107 | 83 | Solar-like | 5763 |
MHD4 | 14 | 144 | 5.8 | 13 | 49 | 3.6 | 7.8 × 106 | 62 | 12 | 31 | 201 | Solar-like | 2883 |
MHD5 | 4.3 | 2500 | 2.6 | 19 | 366 | 24 | 1.1 × 107 | 34 | 6 | 17 | 302 | Solar-like | 2883 |
MHD5h | 4.3 | 104 | 2.5 | 23 | 375 | 14 | 3.7 × 107 | 67 | 13 | 33 | 149 | Solar-like | 5763 |
Notes. All simulations have ℒ = 5.5 × 105. The diffusion coefficients in the lower resolutions (2883) runs are ν = 2.8 × 106 m2 s−1, m2 s−1, and η = 5.6 × 106 m2 s−1, in all cases except in run MHD5 where ν = 2.2 × 106 m2 s−1,
m2 s−1, and η = 4.4 × 106 m2 s−1. In runs MHD1h and MHD3h ν = 1.4 × 106 m2 s−1,
m2 s−1, and η = 2.8 × 106 m2 s−1, whereas in run MHD5h ν = 1.1 × 106 m2 s−1,
m2 s−1, and η = 2.2 × 106 m2 s−1. Run MHD0 is the same as run HD1 but with magnetic fields included. The initial value of χ = 2.0 × 103 m2 s−1 at the centre of the star. The quantity τsim is the length of the statistically steady part of the simulations and the last column indicates the sense of the differential rotation (DR).
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