Nonlinear magnetoconvection in a rapidly rotating sphere and Taylor's constraint
- 1 December 1994
- journal article
- Published by Taylor & Francis in Geophysical & Astrophysical Fluid Dynamics
- Vol. 77 (1) , 111-132
- https://doi.org/10.1080/03091929408203678
Abstract
No abstract availableKeywords
This publication has 30 references indexed in Scilit:
- Nonlinear Planetary DynamosPublished by Cambridge University Press (CUP) ,1994
- Nonlinear planetary dynamos in a rotating spherical shell. III. α2ω models and the geodynamoGeophysical & Astrophysical Fluid Dynamics, 1993
- Nonlinear planetary dynamos in a rotating spherical shell. II. The post-Taylor equilibration for α2-dynamosGeophysical & Astrophysical Fluid Dynamics, 1992
- The effect of a stable layer at the core-mantle boundary on thermal convectionGeophysical & Astrophysical Fluid Dynamics, 1992
- Nonlinear planetary dynamos in a rotating spherical shellGeophysical & Astrophysical Fluid Dynamics, 1991
- Differential rotation and thermal convection in a rapidly rotating hydromagnetic systemGeophysical & Astrophysical Fluid Dynamics, 1989
- αω-Dynamos and Taylor's constraintGeophysical & Astrophysical Fluid Dynamics, 1988
- The stabilizing role of differential rotation on hydromagnetic wavesJournal of Fluid Mechanics, 1983
- Hydromagnetic waves in a differentially rotating sphereJournal of Fluid Mechanics, 1983
- Magnetic waves in the core of the earth. IIGeophysical & Astrophysical Fluid Dynamics, 1979