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Solar Surface Emerging Flux Regions: A Comparative Study of Radiative MHD Modeling and<i>Hinode</i>SOT Observations
We present results from numerical modeling of emerging flux regions on the solar surface. The modeling was carried out by means of 3D radiative MHD simulations of the rise of buoyant magnetic flux tubes through the convection zone and into the photosphere. Due to the strong stratification of the convection …