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Table 1.

Summary of the numerical simulations reported in this paper.

Case Co* Co Re* Rm* ΔUx v ¯ rms $ \overline{v}_{\mathrm{rms}} $ ρ 0 s rms ¯ $ \overline{\rho_0 s_{\mathrm{rms}}} $ δ ¯ $ \overline{\delta} $ k ¯ x , mean $ \overline{k}_{x,\mathrm{mean}} $ k ¯ x , peak $ \overline{k}_{x,\mathrm{peak}} $ E kin $ E_{\mathrm{kin}}\prime $ E kin $ \widetilde{E}_{\mathrm{kin}} $ Emag R ¯ xz $ \overline{\mathcal{R}}_{xz} $ M ¯ xz $ \overline{\mathcal{M}}_{xz} $
HD-Co1 1 0.42 1087 –0.75 2.07 2.13 1.98 22.6 1.17 2.17 0.35 –0.03
HD-Co2 2 0.93 1097 –0.79 2.19 2.17 1.98 19.4 1.12 2.40 0.77 0.07
HD-Co5 5 2.64 1084 –2.99 2.45 2.18 2.09 15.3 1.92 2.88 1.25 –0.03
HD-Co10 10 4.05 1204 4.83 2.12 2.48 4.73 23.1 3.18 1.99 0.77 0.13
HD-Co20 20 6.58 1450 11.71 1.76 2.97 11.75 34.2 5.39 1.29 0.32 0.17

MHD-Co1 1 0.68 1196 866 –0.99 1.84 2.64 1.11 15.8 1.15 1.61 0.31 0.46 –0.69 0.87
MHD-Co2 2 1.43 1180 917 –2.15 1.85 2.66 1.07 15.0 1.26 1.60 0.49 0.51 –1.96 2.12
MHD-Co5 5 3.93 1163 978 –2.66 1.96 3.05 1.42 12.8 1.94 1.78 0.80 0.52 –2.08 2.12
MHD-Co10 10 6.31 1144 1072 1.55 1.57 3.90 3.10 20.0 6.46 1.09 0.37 0.55 0.82 –0.87
MHD-Co20 20 12.51 1050 1282 2.41 1.28 4.79 5.32 24.7 12.12 0.72 0.29 0.66 3.97 –3.85

Notes. The flux Coriolis number, Co*, is the only explicit free parameter in this study, whereas the dynamical Coriolis number, Co, was calculated as a simulation output. The Reynolds and magnetic Reynolds numbers, Re* and Rm*, depend on the grid resolution and are estimated in Appendix A. The amplitudes of the mean shear flow, ΔUx, are shown in units of v*. The volume-averaged values of the rms convective velocity, v ¯ rms $ \overline{v}_{\mathrm{rms}} $, rms entropy fluctuation, ρ 0 s rms ¯ $ \overline{\rho_0 s_{\mathrm{rms}}} $, and superadiabaticity, δ ¯ $ \overline{\delta} $, are quoted in units of v*, ρrcvM*2, and M 2 $ \mathrm{M}_{*}^{2} $, respectively. The mean and peak longitudinal wavenumbers, k ¯ x , mean $ \overline{k}_{x,\mathrm{mean}} $ and k ¯ x , peak $ \overline{k}_{x,\mathrm{peak}} $, are in units of 2πLx−1. The volume-integrated kinetic energies of fluctuating velocity, E kin = ( ρ 0 / 2 ) v 2 d V $ E\prime_{\mathrm{kin}}=\int (\rho_0/2)\boldsymbol{v}^{\prime^{2}} dV $, and y-averaged velocity, E kin $ \widetilde{E}_{\mathrm{kin}} $, and total magnetic energy, Emag, are all quoted in units of 102ρrv*2Hr3. The mean values of the turbulent Reynolds and Maxwell stresses, R ¯ xz $ \overline{\mathcal{R}}_{xz} $ and M ¯ xz $ \overline{\mathcal{M}}_{xz} $, are reported in units of ρrv*2.

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