Can the solar angular momentum problem be solved without internal gravity waves?
Solar and Stellar Astrophysics
2024-12-04 v1
Abstract
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.
Cite
@article{arxiv.2412.02518,
title = {Can the solar angular momentum problem be solved without internal gravity waves?},
author = {Vittorio Canuto},
journal= {arXiv preprint arXiv:2412.02518},
year = {2024}
}
Comments
6 pages