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momentum to help explain the measured rotation rates of red giant cores  \citep{Mosser_2012,Cantiello_2014}.   {\bf The presence of strong internal magnetic fields might help explaining the extra internal mixing observed in   red giant and asymptotic giant stars \citep{Busso_2007}. Interestingly the amplitude of magnetic fields required for magnetic buoyancy mixing  to operate is similar to the amplitude of the fields required for dipole modes suppression \citep{Nucci_2014,Fuller15}.}