Magneto-Convection: Structure and Dynamics

Robert F. Stein, Åke Nordlund
2004 Proceedings of the International Astronomical Union  
We present results from realistic, high resolution, simulations of solar magnetoconvection. Simulations were run with both a mean vertical and a mean horizontal field. The magnetic field is quickly swept out of the granules and meso-granules and concentrated in the intergranular lanes.
doi:10.1017/s1743921304005551 fatcat:ogpwfkz5lrdnngr7i5ea6psbsu