Prandtl-number dependence of convection-driven dynamos in rotating spherical fluid shells
From MaRDI portal
Publication:5694865
DOI10.1017/S0022112005004398zbMath1073.76080arXiv0910.4493OpenAlexW1973559471WikidataQ59793941 ScholiaQ59793941MaRDI QIDQ5694865
Radostin D. Simitev, Friedrich H. Busse
Publication date: 5 October 2005
Published in: Journal of Fluid Mechanics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0910.4493
General theory of rotating fluids (76U05) Magnetohydrodynamics and electrohydrodynamics (76W05) Geo-electricity and geomagnetism (86A25)
Related Items (14)
A study of global magnetic helicity in self-consistent spherical dynamos ⋮ Nonlinear thermal inertial waves in rotating fluid spheres ⋮ Advances in geodynamo modelling ⋮ Regimes of thermo-compositional convection and related dynamos in rotating spherical shells ⋮ Transition from laminar to turbulent dynamo: the effect of varying Prandtl number ⋮ Reynolds stresses and mean fields generated by pure waves: applications to shear flows and convection in a rotating shell ⋮ Rotating spherical Couette flow in a dipolar magnetic field: experimental study of magneto-inertial waves ⋮ Generation of a magnetic field by convective flows in a rotating horizontal layer ⋮ Rotating thermal convection in liquid gallium: multi-modal flow, absent steady columns ⋮ The effects of different parameter regimes in geodynamo simulations ⋮ Parameter dependences of convection-driven dynamos in rotating spherical fluid shells ⋮ Continuation of Double Hopf Points in Thermal Convection of Rotating Fluid Spheres ⋮ Scaling behaviour of small-scale dynamos driven by Rayleigh–Bénard convection ⋮ Magnetic field generation by convective flows in a plane layer: the dependence on the Prandtl numbers
This page was built for publication: Prandtl-number dependence of convection-driven dynamos in rotating spherical fluid shells