The Sun’s differential rotation is controlled by high-latitude baroclinically unstable inertial modes
Sign Up to like & getrecommendations! Published in 2024 at "Science Advances"
DOI: 10.1126/sciadv.adk5643
Abstract: Rapidly rotating fluids have a rotation profile that depends only on the distance from the rotation axis, in accordance with the Taylor-Proudman theorem. Although the Sun was expected to be such a body, helioseismology showed… read more here.
Keywords: inertial modes; baroclinically unstable; rotation; latitude baroclinically ... See more keywords