Stokes diagnostics of simulations of magnetoconvection of mixed-polarity quiet-Sun regions
Realistic solar magneto-convection simulations including the photospheric layers are used to study the polarization of the Fe i Zeeman-sensitive spectral lines at 6301.5, 6302.5, 15 648 and 15 652 Å. The Stokes spectra are synthesized in a series of snapshots with a mixed-polarity magnetic field whose average unsigned strength varies from B > = 10
Khomenko, E. V. et al.
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2005