The Dynamic Evolution of Twisted Omega-loops in a 3-D Convecting Flow

Details The Dynamic Evolution of Twisted Omega-loops in a 3-D Convecting Flow The Dynamic Evolution of Twisted Omega-loops in a 3-D Convecting Flow

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsh52a0474a&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SH52A-0474

Physics

7524 Magnetic Fields, 7544 Stellar Interiors And Dynamo Theory

Scientific paper

We present the latest results from 3D MHD simulations (in the anelastic approximation) of buoyant magnetic flux tubes interacting with turbulent convection in the solar interior. We focus our study on active region scale flux ropes and Omega-loops, and perform a large parameter space study of the effects of not only initial field strength, but twist and loop geometry on the morphology and dynamics of sub-surface magnetic structures. We also investigate the effects of different numerical treatments of viscosity, and quantify the amount of magnetic field in each simulation that succumbs to the effects of turbulent pumping.

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