Fig. 5.
Temporally and azimuthally averaged rotation profiles 
for the simulations in set MHD. The values for runs MHD4 and MHD5 are clipped to highlight features near to the equator. The full ranges are indicated in the parenthesis above and below the colour bar. The arrows indicate the mass flux due to meridional circulation 
. The arrow widths are proportional to 
. The maximum meridional flow speeds are indicated in the bottom right corners of each panel.
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