Magnetoconvection in a rotating spherical shell: structure of flow in the outer core
Open Access
- 30 November 1995
- journal article
- Published by Elsevier in Physics of the Earth and Planetary Interiors
- Vol. 92 (1-2) , 109-118
- https://doi.org/10.1016/0031-9201(95)03065-5
Abstract
No abstract availableThis publication has 19 references indexed in Scilit:
- Chaotic thermal convection in a rapidly rotating spherical shell: consequences for flow in the outer corePhysics of the Earth and Planetary Interiors, 1994
- Towards a realistic theory of the geodynamoGeophysical & Astrophysical Fluid Dynamics, 1991
- Geomagnetic secular variationPhilosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1989
- Three-dimensional thermal convection in a spherical shellJournal of Fluid Mechanics, 1989
- On the computation of steady, self - consistent spherical dynamosGeophysical & Astrophysical Fluid Dynamics, 1987
- Numerical simulations of stellar convective dynamos. II - Field propagation in the convection zoneThe Astrophysical Journal, 1985
- Numerical simulations of stellar convective dynamos III. At the base of the convection zoneGeophysical & Astrophysical Fluid Dynamics, 1985
- Numerical simulations of stellar convective dynamos. I. the model and methodJournal of Computational Physics, 1984
- Nonlinear dynamics of boussinesq convection in a deep rotating spherical shell-iGeophysical & Astrophysical Fluid Dynamics, 1977
- A Model of the GeodynamoGeophysical Journal of the Royal Astronomical Society, 1975