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Table 1

Summary of the runs.

Run Ra Pr δn Roc Re Co Emer/Ekin Erot/Ekin Remarks

A 3.93 × 105 40.4 2.50 0.73 35 1.24 -2.47 -0.51 4.20 0.003 0.954 0.09 1.01 AS
B 3.54 × 105 20.3 2.25 0.69 34 1.27 -2.36 -0.50 3.87 0.003 0.954 0.18 0.84 AS
C 3.16 × 105 13.6 2.00 0.65 33 1.33 -2.28 -0.49 3.60 0.003 0.955 0.30 0.66 AS
D 2.92 × 105 11.3 1.85 0.63 29 1.50 0.03 0.04 0.33 0.001 0.466 0.34 0.62 SL
E 2.77 × 105 10.1 1.75 0.61 27 1.60 -0.01 0.09 0.38 0.001 0.593 0.37 0.53 SL, polar jet

D0 2.92 × 105 11.3 1.85 0.63 29 1.50 0.03 0.04 0.33 0.001 0.466 0.34 0.62 SL
D1 3.16 × 105 13.5 2.00 0.65 29 1.50 0.16 0.07 0.37 0.001 0.517 0.28 0.65 SL
D2 3.31 × 105 15.6 2.10 0.67 30 1.44 0.13 0.05 0.37 0.001 0.465 0.24 0.72 SL
D3 3.47 × 105 18.4 2.20 0.68 32 1.37 0.03 0.01 0.28 0.002 0.243 0.21 0.81 SL
D4 3.62 × 105 22.7 2.30 0.70 35 1.27 -2.33 -0.50 3.93 0.003 0.955 0.19 0.87 AS

B0 3.54 × 105 20.3 2.25 0.69 34 1.27 -2.36 -0.50 3.87 0.003 0.954 0.18 0.84 AS
B1 3.47 × 105 18.5 2.20 0.68 34 1.27 -2.26 -0.50 3.92 0.002 0.956 0.24 0.85 AS
B2 3.31 × 105 15.7 2.10 0.67 33 1.31 -2.27 -0.50 3.87 0.003 0.958 0.27 0.77 AS
B3 3.16 × 105 13.6 2.00 0.65 33 1.34 -2.18 -0.49 3.67 0.003 0.958 0.31 0.71 AS
B4 3.00 × 105 12.0 1.90 0.64 32 1.37 -2.15 -0.49 3.54 0.003 0.958 0.34 0.64 AS
B5 2.85 × 105 10.8 1.80 0.62 31 1.41 -2.06 -0.49 3.38 0.003 0.958 0.38 0.59 AS
B6 2.69 × 105 9.7 1.70 0.60 30 1.45 -1.98 -0.48 3.16 0.003 0.957 0.41 0.54 AS
B7 2.38 × 105 8.2 1.50 0.57 28 1.54 -1.86 -0.47 2.83 0.003 0.958 0.48 0.44 AS
B8 2.22 × 105 7.6 1.40 0.55 27 1.60 -1.76 -0.45 2.63 0.003 0.958 0.51 0.39 AS
B9 2.07 × 105 7.0 1.30 0.53 22 2.01 0.04 0.12 0.25 0.001 0.632 0.54 0.28 SL, polar jets
B10 1.59 × 105 5.8 1.00 0.46 18 2.43 0.06 0.12 0.19 0.001 0.668 0.65 0.17 SL, polar jets
B10b 1.59 × 105 5.8 1.00 0.46 17 2.61 0.33 0.11 0.34 0.000 0.831 0.65 0.17 SL

Notes. All models have PrSGS = 0.25, ℒ = 3.85 × 10-5, Ta = 2.98·106, ξ = 0.0325 corresponding to Γ ≈ 12, Ω0/ Ω = 1, and use a grid resolution 128 × 256 × 128. With χSGS(r1) = 5 × 108 m2 s-1, we have , and ν = 9.3 × 107 m2 s-1. is the volume averaged total kinetic energy, in units of GMρ0/R. and are the kinetic energies of the meridional circulation and differential rotation. and are the fractions of total flux transported by radiative conduction and resolved convection at r = rm. Runs D and D0, and Runs B and B0 are the same. Run D1 was continued from a snapshot of Run D, whereas the other models in Set D were continued from a relaxed state of D1. In Set B, a snapshot of Run B0 was used as an initial condition. In the last column, AS and SL stand for anti-solar and solar-like differential rotation, respectively.

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