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Table 1
Value of the standard parameters for the temperature forced (TF) and radiative transfer (RT) simulations.
| Quantity | TF | RT |
|
|
||
| Horizontal resolution | 144λ, 90φ | |
| Vertical resolution, Nz | 66 | |
| Dynamical timestep (s) | 1200 | 30 |
| Radiative timestep (s) | – | 150 |
| Initial inner boundary pressure, pmax (Pa) | 220 × 105 | 200 × 105 |
| Rotation rate, Ω (s-1) | 2.06 × 10-5 | |
| Radius, Rp (m) | 9.44 × 107 | 9.0 × 107 |
| Radius to outer boundary, Rtop (m) | 1.1 × 107 | 9.0 × 106 |
| Surface gravity, gp (m s-2) | 9.42 | 10.79 |
| Specific heat capacity (constant pressure), cp (J kg-1 K-1) | 14 308.4 | 13 000.0 |
| Ideal gas constant, R (J kg-1 K-1)(1) | 4593 | 3556.8 |
Diffusion setting, Kλ (see Sect. 2.1 for applied coefficient,  ) |
0.158 | |
| Horizontal vector Laplacian damping coefficient, νλ,φ | 0.1 | 0.0 |
| Vertical vector Laplacian damping coefficient, νr | 0.0 | |
| Vertical, “sponge”, damping coefficient Rw | 0.15 | |
| Temperature characterising intrinsic luminosity of the planet (K), Tint | – | 100 |
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