An investigation of reversing numerical dynamos driven by either differential or volumetric heating

Author:

Rotvig Jon

Publisher

Elsevier BV

Subject

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

Reference22 articles.

1. Varying the spherical shell geometry in rotating thermal convection;Al-Shamali;Geophys. Astrophys. Fluid Dyn.,2004

2. Steady zonal flows in spherical shell dynamos;Aubert;J. Fluid Mech.,2005

3. The magnetic structure of convection-driven numerical dynamos;Aubert;Geophys. J. Int.,2008

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

5. A numerical dynamo benchmark;Christensen;Phys. Earth Planet. Int.,2001

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1. Magnetic reversals from planetary dynamo waves;Nature;2016-11

2. The role of buoyancy in polarity reversals of the geodynamo;Geophysical Journal International;2014-10-17

3. A buoyancy profile for the Earth's core;Geophysical Journal International;2011-09-28

4. Complex polarity reversals in a geodynamo model;Earth and Planetary Science Letters;2011-04

5. Thermochemically driven convection in a rotating spherical shell;Geophysical Journal International;2010-08-02

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