Differential rotation in turbulent compressible convection

Details Differential rotation in turbulent compressible convection Differential rotation in turbulent compressible convection

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997assl..225..223b&link_type=abstract

SCORe'96 : Solar Convection and Oscillations and their Relationship, Proceedings of a workshop, held in Aarhus, Denmark, May 27

Astronomy and Astrophysics

Astrophysics

Solar Convection Zone, Differential Rotation, Turbulence

Scientific paper

Numerical simulations of 3D compressible convection in a local rectilinear geometry show that zonal and meridional mean flows, $\overline{u}(z)$ and $\overline{v}(z)$, can be produced when rotation is included. A wide variety of mean profiles can be achieved depending upon the parameters, including behaviour equivalent (within the limitations of the model) to that inferred from helioseismic solar observations.

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