A Note on Anisotropic Convection and the Rotation of Stellar Convective Zones

Details A Note on Anisotropic Convection and the Rotation of Stellar Convective Zones A Note on Anisotropic Convection and the Rotation of Stellar Convective Zones

Apr 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974ap%26ss..27..419r&link_type=abstract

Astrophysics and Space Science, Volume 27, Issue 2, pp.419-424

Astronomy and Astrophysics

Astrophysics

4

Scientific paper

The interaction of rotation and convection produces a latitude dependent
anisotropic turbulent viscosity. When this friction is dominant,
equilibrium of a convective outer layer of a star is achieved by an
equatorial acceleration and a two-zone circulation, towards the equator
at low surface latitudes.

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