Diverging And Converging Flows Around Sunspot Structures In Axisymmetric Mhd Simulations

Details Diverging And Converging Flows Around Sunspot Structures In Axisymmetric Mhd Simulations Diverging And Converging Flows Around Sunspot Structures In Axisymmetric Mhd Simulations

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21640005h&link_type=abstract

American Astronomical Society, AAS Meeting #216, #400.05; Bulletin of the American Astronomical Society, Vol. 41, p.855

Astronomy and Astrophysics

Astronomy

Scientific paper

We present results on modeling solar pores and sunspots using 2D axisymmetric magneto-hydrodynamic (MHD) simulations. These models are helpful for understanding the mechanisms of magnetic field concentration in sunspots, and the large-scale flow patterns associated with them. The simulations provide consistent, self-maintained, even if not fully realistic, models of concentrated magnetic field near the solar surface. We explore under which conditions the associated flows are converging or diverging in nature near the surface.

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