Investigating the capability to infer the magnetic field from non-local thermodynamic equilibrium inversions of the Mg I 12.32 μm line

Open Access

Fig. 3.

Mean differences between the inferred atmospheric parameters and those of the simulation (solid line) as a function of the optical depth log (τ₅₀₀). From top to bottom: Temperature, LOS velocity, and longitudinal and horizontal components of magnetic field. The dotted curves enclose the standard deviation of the differences.

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