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Long‐term variations of turbulent transport coefficients in a solarlike convective dynamo simulation

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Characterizing the feedback of magnetic field on the differential rotation of solar-like stars

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Effect of shear and magnetic field on the heat-transfer efficiency of convection in rotating spherical shells

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The impact of rotation on turbulent tidal friction in stellar and planetary convective regions

S. Mathis, P. Auclair-Desrotour, M. Guenel, F. Gallet and C. Le Poncin-Lafitte
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Dependence of magnetic cycle parameters on period of rotation in non-linear solar-type dynamos

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Monthly Notices of the Royal Astronomical Society 451 (2) 1528 (2015)
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DYNAMO EFFECTS NEAR THE TRANSITION FROM SOLAR TO ANTI-SOLAR DIFFERENTIAL ROTATION

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ON THE CAUSE OF SOLAR-LIKE EQUATORWARD MIGRATION IN GLOBAL CONVECTIVE DYNAMO SIMULATIONS

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HIGH-RESOLUTION CALCULATION OF THE SOLAR GLOBAL CONVECTION WITH THE REDUCED SPEED OF SOUND TECHNIQUE. II. NEAR SURFACE SHEAR LAYER WITH THE ROTATION

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