A three-dimensional convective dynamo solution with rotating and finitely conducting inner core and mantle

Physics of the Earth and Planetary Interiors

Volumn 91, Issue 1-3, 1995, Pages 63-75

  Glatzmaier, Gary A ^a   Roberts, Paul H ^b  

^a LOS ALAMOS NATIONAL LABORATORY   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

CONVECTION; CORE; FLUID MOTION; GEODYNAMO; GEOMAGNETIC FIELD; MANTLE;

EID: 0029480581     PISSN: 00319201     EISSN: None     Source Type: Journal    
DOI: 10.1016/0031-9201(95)03049-3     Document Type: Article

References (49)

1. Three-dimensional thermal convection in a spherical shell
2. Simple models of fluid flow at the core surface derived from geomagnetic field models
3. The secular variation of the Earth's magnetic field
4. Thermal core-mantle interactions
5. Time-dependent mapping of the magnetic field at the core-mantle boundary
6. Structure of the F layer and reasons for convection in the Earth's core
7. Local turbulence in the Earth's core
8. Simulation of turbulent cyclonic magneto-convection
9. An experimental approach to thermochemical convection in the Earth's core
10. What is a stellar dynamo?
11. On the computation of steady self-consistent spherical dynamos
12. Viscosity of the Earth's core
13. Dynamically consistent nonlinear dynamos driven by convection in a rotating spherical shell II Dynamos with cycles and strong feedbacks
14. Dynamically consistent nonlinear dynamos driven by convection in a rotating spherical shell
15. Numerical simulations of stellar convective dynamos. I. The model and method
16. Numerical simulations of stellar convective dynamos II Field propagation in the convection zone
17. Numerical simulations of stellar convective dynamos III At the base of the convection zone
18. Highly supercritical thermal convection in a rotating spherical shell: centrifugal vs. radial gravity
19. Intermediate dynamo models
20. Rotation of the inner core
21. Space-laboratory and numerical simulations of thermal convection in a rotating hemispherical shell with radial gravity
22. Motions of the Earth's core and mantle, and variations of the main geomagnetic field
23. Dynamo theorems
24. Earth's variable rotation
25. Magnetohydrodynamic Ekman and Stewartson layers in a rotating spherical shell
26. 2-dynamo in the limit of asymptotically small viscosity
27. A geodynamo model incorporating a finitely conducting inner core
28. Influence of the Earth's inner core on geomagnetic fluctuations and reversals
29. On the magnetically stabilizing role of the Earth's inner core
30. Time-dependent flow at the core surface and conservation of angular momentum in the coupled core-mantle system
31. Computer simulation of a magnetohydrodynamic dynamo II
32. On the effect of boundary topography on flow in the Earth's core
33. The main field
34. Torque balance and energy budget for the precessionally driven dynamo
35. Mantle plumes and the periodicity of magnetic field reversals
36. Precession of the Earth as the cause of geomagnetism
37. Turbulent dynamos driven by convection
38. Dynamo action in stratified convection with overshoot
39. Hydromagnetic dynamo models
40. The stability of the magnetostrophic approximation I Taylor state solutions
41. The strong field branch of the Childress-Soward dynamo
42. The magneto-hydrodynamics of a rotating fluid and the Earth's dynamo problem
43. A geodynamo powered by luni-solar precession
44. Steady flows at the top of Earth's core derived from geomagnetic field models
45. A steady velocity field at the top of the Earth's core in the frozen-flux approximation—errata and further comments
46. Convection driven magnetohydrodynamic dynamos in rotating spherical shells
47. Generation of magnetic fields by convection in a rotating spherical fluid shell of infinite Prandtl number