Turbulence, Magnetism, and Shear in Stellar Interiors

DOI10.1146/annurev.fluid.010908.165215zbMath1159.76053OpenAlexW2157528951MaRDI QIDQ3608387

Juri Toomre, Mark S. Miesch

Publication date: 4 March 2009

Published in: Annual Review of Fluid Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1146/annurev.fluid.010908.165215

zbMATH Keywords

astrophysical fluid dynamicshelioseismologysolar oscillationsmeridional flows

Mathematics Subject Classification ID

Turbulence (76Fxx) Magnetohydrodynamics and electrohydrodynamics (76W05) Galactic and stellar structure (85A15) Research exposition (monographs, survey articles) pertaining to fluid mechanics (76-02) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Research exposition (monographs, survey articles) pertaining to astronomy and astrophysics (85-02)

Related Items (8)

Baroclinically-driven flows and dynamo action in rotating spherical fluid shells ⋮ Effects of a subadiabatic layer on convection and dynamos in spherical wedge simulations ⋮ A hybrid discrete exterior calculus and finite difference method for Boussinesq convection in spherical shells ⋮ Coarse-grained incompressible magnetohydrodynamics: analyzing the turbulent cascades ⋮ Tristable flow states and reversal of the large-scale circulation in two-dimensional circular convection cells ⋮ Emergence of substructures inside the large-scale circulation induces transition in flow reversals in turbulent thermal convection ⋮ Pattern formation in rapidly oscillating peculiar A stars ⋮ Oscillatory large-scale dynamos from Cartesian convection simulations

This page was built for publication: Turbulence, Magnetism, and Shear in Stellar Interiors