Value of the standard parameters for the temperature forced (TF) and radiative transfer (RT) simulations.
|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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