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The influence of magnetic fields in planetary dynamo models

  • Published:2012-06 Issue: Volume:333-334 Page:9-20
  • ISSN:0012-821X
  • Container-title:Earth and Planetary Science Letters
  • language:en
  • Short-container-title:Earth and Planetary Science Letters

Author:

Soderlund Krista M.,King Eric M.,Aurnou Jonathan M.

Funder

NASA Planetary Atmospheres Program

National Science Foundation

Miller Institute for Basic Research in Science, and K.M.S

University of Texas Institute for Geophysics (UTIG)

NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center

Publisher

Elsevier BV

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference60 articles.

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

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

3. Remarks on some typical assumptions in dynamo theory;Busse;Geophys. Astrophys. Fluid Dyn.,2011

4. Towards a rapidly rotating liquid sodium dynamo experiment;Cardin;Magnetohydrodynamics,2002

5. The influence of toroidal magnetic field on thermal convection in the core;Cardin;Earth Planet. Sci. Lett.,1995

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