Can the solar angular momentum problem be solved without internal gravity waves?
Vittorio Canuto

TL;DR
This paper investigates the solar radiative zone spin-down problem by replacing internal gravity waves with a shear vorticity model, showing it can produce similar effects on a comparable timescale.
Contribution
The study introduces a shear vorticity model as an alternative to internal gravity waves for explaining solar radiative zone spin-down.
Findings
Shear vorticity model mimics IGW effects
Spin-down timescale around 10^7 years
Potential alternative to IGW in solar models
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsSolar and Space Plasma Dynamics · Geophysics and Gravity Measurements · Spacecraft Dynamics and Control
