The role of inertia in hydrodynamic models of the geodynamo

Author:

Fearn D.R,Morrison G

Publisher

Elsevier BV

Subject

Space and Planetary Science,Physics and Astronomy (miscellaneous),Geophysics,Astronomy and Astrophysics

Reference24 articles.

1. On convection driven dynamos in rotating spherical shells;Busse;Studia Geophys. Geod.,1998

2. Chandrasekhar, S., 1961. Hydrodynamic and Hydromagnetic Stability. Oxford University Press, Oxford.

3. Numerical modelling of the geodynamo: a systematic parameter survey;Christensen;Geophys. J. Int.,1999

4. A three-dimensional self-consistent computer simulation of a geomagnetic field reversal;Glatzmaier;Nature,1995

5. A three-dimensional convective dynamo solution with rotating and finitely conducting inner-core and mantle;Glatzmaier;Phys. Earth Planet. Inter.,1995

Cited by 6 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Inertia-less convectively-driven dynamo models in the limit of low Rossby number and large Prandtl number;Physics of the Earth and Planetary Interiors;2017-05

2. A spectral solution of nonlinear mean field dynamo equations: With inertia;Computers & Mathematics with Applications;2009-08

3. On the inviscid flow in the earth's liquid core;Geophysical & Astrophysical Fluid Dynamics;2007-10

4. The role of inertia in the evolution of spherical dynamos;Geophysical Journal International;2006-02

5. The role of inertia in models of the geodynamo;Geophysical Journal International;2004-08

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