3D MHD Simulations of Magnetic Flux Emergence in Active Regions

Details 3D MHD Simulations of Magnetic Flux Emergence in Active Regions 3D MHD Simulations of Magnetic Flux Emergence in Active Regions

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp41a..11a&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SP41A-11

Physics

7509 Corona, 7524 Magnetic Fields, 7529 Photosphere

Scientific paper

We report on the progress of 3D simulations of active region magnetic flux emergence (and decay) through the stratified, sub-photospheric layers of the upper convection zone into the solar atmosphere and low corona. We use a recently-developed 3D semi-implicit MHD code (with a non-uniform, adaptive mesh) to address the inherent stiffness of the system of equations, and will compare our results with similar studies using second-order accurate, fully explicit numerical schemes.

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