2024/12/03 by Canuto, Vittorio
#14F05 #F.2.2 #FOS: Physical sciences #Solar and Stellar Astrophysics (astro-ph.SR)
paper · doi:10.48550/arxiv.2412.02518
The solar radiative zone spin down problem is treated without internal gravity waves, IGW. The shear-only model of the Reynolds stresses adopted thus far in all calculations, is substituted by a shear vorticity model. The latter component is shown to play a role analogous to the IGW and with a similar time scale of about 107years.