Table 1.
Summary of runs.
| Run |
 |
Ta[106] | Ra[107] | PrSGS | Re | Co | DR |
 |
 |
 |
 |
 |
 |
 |
 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| H0 | 0.0 | 0.0 | 4.0 | 2.0 | 52 | 0.0 | ? | 4.863 | 0.127 | 0.706 | 4.031 | ||||
| H0.005 | 0.005 | 1.3(−4) | 4.0 | 2.0 | 52 | 0.006 | ? | 4.884 | 0.124 | 0.677 | 4.083 | ||||
| H0.01 | 0.01 | 5.4(−4) | 4.0 | 2.0 | 52 | 0.011 | AS | 4.873 | 0.134 | 0.652 | 4.087 | ||||
| H0.1 | 0.1 | 5.4(−2) | 4.0 | 2.0 | 47 | 0.12 | AS | 10.307 | 6.727 | 0.293 | 3.298 | ||||
| H0.5 | 0.5 | 1.3 | 4.0 | 2.0 | 47 | 0.62 | AS | 11.203 | 7.608 | 0.292 | 3.303 | ||||
| H1 | 1.0 | 5.4 | 4.0 | 2.0 | 49 | 1.2 | AS | 54.087 | 50.976 | 0.554 | 2.557 | ||||
| H1.5 | 1.5 | 9.7 | 4.0 | 2.0 | 41 | 1.9 | AS | 62.036 | 60.103 | 0.337 | 2.364 | ||||
| H2 | 2.0 | 21.6 | 4.0 | 2.0 | 44 | 2.7 | AS | 14.515 | 11.699 | 0.051 | 2.765 | ||||
| H2.5 | 2.5 | 33.7 | 4.0 | 2.0 | 43 | 3.4 | S | 9.541 | 6.811 | 0.041 | 2.689 | ||||
| H3.0 | 3.0 | 48.6 | 4.0 | 2.0 | 41 | 4.3 | S | 10.669 | 8.109 | 0.035 | 2.526 | ||||
| H5 | 5.0 | 125 | 4.0 | 2.0 | 34 | 8.4 | S | 5.402 | 3.569 | 0.018 | 1.815 | ||||
| H7 | 7.0 | 190 | 3.4 | 2.4 | 26 | 13.6 | S | 4.381 | 3.078 | 0.011 | 1.129 | ||||
| H10 | 10.0 | 260 | 2.8 | 2.9 | 18 | 22.9 | S | 3.107 | 2.176 | 0.005 | 0.926 | ||||
| M0.5 | 0.5 | 1.3 | 4.0 | 2.0 | 44 | 0.7 | AS | 7.141 | 3.910 | 0.199 | 3.032 | 0.362 | 0.032 | 0.019 | 0.311 |
| M1 | 1.0 | 5.4 | 4.0 | 2.0 | 40 | 1.5 | AS | 4.084 | 1.259 | 0.074 | 2.751 | 0.775 | 0.074 | 0.063 | 0.638 |
| M1.5 | 1.5 | 12 | 4.0 | 2.0 | 39 | 2.2 | AS | 3.163 | 0.691 | 0.045 | 2.427 | 0.789 | 0.107 | 0.077 | 0.605 |
| M2 | 2.0 | 22 | 4.0 | 2.0 | 40 | 2.9 | AS | 3.065 | 0.483 | 0.036 | 2.547 | 0.479 | 0.055 | 0.048 | 0.376 |
| M2.5 | 2.5 | 34 | 4.0 | 2.0 | 40 | 3.7 | S | 2.992 | 0.524 | 0.029 | 2.438 | 0.506 | 0.087 | 0.044 | 0.375 |
| M3 | 3.0 | 49 | 4.0 | 2.0 | 39 | 4.5 | S | 3.584 | 1.268 | 0.026 | 2.290 | 0.593 | 0.120 | 0.050 | 0.423 |
| M4 | 4.0 | 86 | 4.0 | 2.0 | 36 | 6.6 | S | 3.741 | 1.741 | 0.019 | 1.981 | 0.801 | 0.144 | 0.100 | 0.557 |
| M5 | 5.0 | 35 | 4.0 | 2.0 | 34 | 8.6 | S | 3.600 | 1.804 | 0.015 | 1.780 | 0.987 | 0.190 | 0.136 | 0.660 |
| M7 | 7.0 | 264 | 4.0 | 2.0 | 31 | 13.4 | S | 2.481 | 1.040 | 0.009 | 1.432 | 1.109 | 0.206 | 0.198 | 0.704 |
| M10 | 10.0 | 540 | 4.0 | 2.0 | 27 | 21.5 | S | 1.550 | 0.465 | 0.005 | 1.079 | 1.159 | 0.212 | 0.242 | 0.705 |
| M15 | 15.0 | 1897 | 7.4 | 2.0 | 27 | 40.3 | S | 0.746 | 0.066 | 0.002 | 0.677 | 1.216 | 0.126 | 0.290 | 0.799 |
| M30 | 30.0 | 13488 | 16.1 | 2.0 | 26 | 110.9 | S | 0.392 | 0.021 | 0.001 | 0.370 | 2.007 | 0.305 | 0.462 | 1.241 |
Notes. Second to fourth columns: input parameters. Columns 6 to 15 show the output parameters, which are calculated from the saturated stage of the simulations. DR indicates the type of differential rotation, either it is anti-solar (AR), or solar (S)-like or inconclusive (?) differential rotation. The energies E are given in 105 J m−2 and their definitions are given in Eqs. (5)–(9). All runs have a density contrast of Γρ ≡ ρ(r = 0.7R)/ρ(R) = 31 and the MHD runs (Set M) PrM = 1. The resolution is 180 × 256 × 128 grid points for all runs, except it is 360 × 512 × 256 for Run H10.
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