A three-dimensional convective dynamo solution with rotating and finitely conducting inner core and mantle
- 1 September 1995
- journal article
- Published by Elsevier in Physics of the Earth and Planetary Interiors
- Vol. 91 (1-3) , 63-75
- https://doi.org/10.1016/0031-9201(95)03049-3
Abstract
No abstract availableThis publication has 40 references indexed in Scilit:
- On the effect of boundary topography on flow in the Earth's coreGeophysical & Astrophysical Fluid Dynamics, 1993
- Highly supercritical thermal convection in a rotating spherical shell: Centrifugal vs. radial gravityGeophysical & Astrophysical Fluid Dynamics, 1993
- A geodynamo powered by luni-solar precessionGeophysical & Astrophysical Fluid Dynamics, 1991
- Generation of magnetic fields by convection in a rotating spherical fluid shell of infinite Prandtl numberPhysics of the Earth and Planetary Interiors, 1990
- On the computation of steady, self - consistent spherical dynamosGeophysical & Astrophysical Fluid Dynamics, 1987
- Thermal core– mantle interactionsNature, 1987
- Mantle plumes and the periodicity of magnetic field reversalsGeophysical Research Letters, 1986
- Space-laboratory and numerical simulations of thermal convection in a rotating hemispherical shell with radial gravityJournal of Fluid Mechanics, 1986
- Torque balance and energy budget for the precessionally driven dynamoPhysics of the Earth and Planetary Interiors, 1975
- Motions of the Earth's Core and Mantle, and Variations of the Main Geomagnetic FieldScience, 1967