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Using mean-field hydrodynamic models of the solar angular momentum balance weshow that the non-monotonic latitudinal dependence of the radial angularmomentum fluxes caused by Lambda-effect can affect the number of the meridionalcirculation cells stacking in radial direction in the solar convection zone. Inparticular, our results show the possibility of a complicated triple-cellmeridional circulation structure. This pattern consists of two largecounterclockwise circulation cells (the N-hemisphere) and a smaller clockwisecell located at low latitudes at the bottom of the convection zone.

Angular momentum fluxes caused by Lambda-effect and meridional circulation structure of the Sun