Solar Surface Emerging Flux Regions: A Comparative Study of Radiative MHD Modeling and Hinode SOT Observations
We present results from numerical modeling of emerging flux regions on the solar surface. The modeling was carried out by means of three-dimensional (3D) radiative MHD simulations of the rise of buoyant magnetic flux tubes through the convection zone and into the photosphere. Due to the strong strat...
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Veröffentlicht in: | The Astrophysical journal 2008-11, Vol.687 (2), p.1373-1387 |
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Sprache: | eng |
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