Global models of the magnetic Sun

Details Global models of the magnetic Sun Global models of the magnetic Sun

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008iaus..247...33b&link_type=abstract

Waves & Oscillations in the Solar Atmosphere: Heating and Magneto-Seismology, Proceedings of the International Astronomical Unio

Astronomy and Astrophysics

Astronomy

2

Sun: Cycle, Dynamo, Rotation, Convection, Flux Emergence, Radiative Interior, Mhd

Scientific paper

We briefly present recent simulations of the internal magnetism of the Sun with the 3-D ASH code and with the 2-D STELEM code. The intense magnetism of the Sun is linked to local and global dynamo action within our star. We focus our study on how magnetohydrodynamical processes in stable (radiative) or unstable (convective) zones, nonlinearly interact to establish the solar differential rotation, meridional circulation, confine the tachocline, amplify and organise magnetic fields and how magnetic flux emerge to the surface. We also test the robustness of flux transport dynamo models to various profiles of circulation.

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