Laboratory Models of Planetary Core Fluid Dynamics (Invited)

Details Laboratory Models of Planetary Core Fluid Dynamics (Invited) Laboratory Models of Planetary Core Fluid Dynamics (Invited)

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufm.p43e..06a&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #P43E-06

Physics

[1507] Geomagnetism And Paleomagnetism / Core Processes, [1510] Geomagnetism And Paleomagnetism / Dynamo: Theories And Simulations, [5440] Planetary Sciences: Solid Surface Planets / Magnetic Fields And Magnetism, [5734] Planetary Sciences: Fluid Planets / Magnetic Fields And Magnetism

Scientific paper

I will discuss recent laboratory simulations of physical processes within planetary cores. This survey will consider buoyancy-driven models of core convection and mechanically-driven models of core flow and dynamo action. Comparisons will be made between the results of laboratory experiments, numerical dynamo simulations and planetary magnetic field observations.

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