Modeling of the Turbulent Dynamo

Details Modeling of the Turbulent Dynamo Modeling of the Turbulent Dynamo

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003spd....34.1904b&link_type=abstract

American Astronomical Society, SPD meeting #34, #19.04; Bulletin of the American Astronomical Society, Vol. 35, p.842

Astronomy and Astrophysics

Astronomy

Scientific paper

We report on the development progress of a 3-D spherical anelastic MHD code (SANMHD) that will be used to study the turbulent dynamo in solar and stellar interiors. SANMHD is a complement to the existing Cartesian anelastic MHD code, ANMHD; to model the interaction between penetrative turbulent convection and magnetic field deep in the interior of stars, it becomes necessary to consider a gravitationally stratified atmosphere in a spherical geometry. We discuss issues regarding the creation of a highly modular code that is portable across multiple platforms, code structuring to allow the flexibility to investigate a variety of physical scenarios and testing strategies.

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