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| Paper: |
Self-organization of the Solar Turbulent Convection in Magnetic Field |
| Volume: |
462, Progress in Solar/Stellar Physics with Helio- and Asteroseismology |
| Page: |
382 |
| Authors: |
Kitiashvili, I. N.; Kosovichev, A. G.; Mansour, N. N.; Wray, A. A. |
| Abstract: |
Observations of the solar surface show a highly turbulent behavior
of convection, and reveal coherent structures in distributed magnetic fields.
We present results of realistic radiation magneto-hydrodynamics (MHD) simulations in three dimensions (3D)
of the solar subsurface layers, and investigate properties of magneto-convection for
various magnetic field topologies and strengths.
In particular, we discuss the filamentary structure and dynamics of sunspot penumbra, spontaneous formation of pore-like and small-scale magnetic structures, and compare the simulation results with observations. |
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