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Magneto-Convection: Structure and Dynamics
2004
Proceedings of the International Astronomical Union
Preserved Fulltext
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