Inertial effects on thermochemically driven convection and hydromagnetic dynamos in a spherical shell
Author:
Publisher
Oxford University Press (OUP)
Subject
Geochemistry and Petrology,Geophysics
Link
http://academic.oup.com/gji/article-pdf/212/3/2194/23569640/ggx529.pdf
Reference29 articles.
1. Thermochemical flows couple the Earth’s inner core growth to mantle heterogeneity;Nature,2008
2. The magnetic structure of convection-driven numerical dynamos;Geophys. J. Int.,2008
3. Modelling the palaeo-evolution of the geodynamo;Geophys. J. Int.,2009
4. Equations governing convection in the Earth’s core and the geodynamo;Geophys. Astrophys. Fluid Dyn.,1995
5. Thermochemically driven convection in a rotating spherical shell;Geophys. J. Int.,2010
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1. Thermochemical convection in a slowly rotating spherical shell: a transition between prograde and retrograde flows;Geophysical & Astrophysical Fluid Dynamics;2024-03-03
2. Influence of Centrifugal Buoyancy in Thermal Convection within a Rotating Spherical Shell;Symmetry;2022-09-26
3. Transition from laminar to turbulent dynamo: the effect of varying Prandtl number;Geophysical & Astrophysical Fluid Dynamics;2020-08-20
4. Magnetic and velocity fields in a dynamo operating at extremely small Ekman and magnetic Prandtl numbers;Contributions to Geophysics and Geodesy;2017-12-01
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