Rate of angular momentum transport by mixed modes ( as defined by Eq. (59)) computed as described in Sect. 4.2 for the 1.3 M_⊙ model described in Sect. 5.1 versus the radius normalised by the radius of the radiative region. is normalised so that at the photosphere. The colour code is as follows: the solid red line corresponds to (thus to a spin down) and the solid blue line to (thus to a spin up). The top panel exhibits the result for the prograde mode ℓ = −m = 2 of frequency ν_R = 300,9 μHz, the middle panel corresponds to the retrograde mode ℓ = m = 2, and the bottom panel to summation of for the prograde and retrograde modes. We only show the inner radiative region, for which our formalism is valid.