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Paper: Comparison of Parameters from Three-Dimensional Magnetoconvection Simulations of the Solar Photosphere
Volume: 526, Solar Polarization Workshop 8
Page: 195
Authors: Cubas Armas, M.; Fabbian, D.; Vitas, N.
Abstract: We present preliminary results from a comparison of parameters derived from three-dimensional magnetohydrodynamic simulations of a plage obtained with the MURaM and STAGGER codes. We first compared the computed atmospheric physical parameters stored in the output temporal snapshots. Subsequently, we used the same snapshots as input to perform spectral synthesis calculations using the NICOLE code. We compared the synthetic Fe I 630.1 nm and 630.2 nm spectral lines in terms of central intensity, equivalent width, full width at half maximum, as well as area and amplitude asymmetry of the Stokes V profile.
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