The influence of NLTE effects in Fe I lines on an inverted atmosphere I. 6301 A and 6302 A lines formed in 1D NLTE (1912.07007v2)

Abstract: Ultraviolet over-ionisation of iron atoms in the solar atmosphere leads to deviations in their level populations from the Saha-Boltzmann statistics. This causes their line profiles to form in Non-Local Thermodynamic Equilibrium (NLTE) conditions. While inverting such profiles to determine atmospheric parameters, the NLTE effects are often neglected and deviations from LTE are compensated for by tweaking other quantities. We investigate how the routinely employed LTE inversion of iron lines formed in NLTE under- or over-estimates atmospheric quantities such as temperature (T), line-of-sight velocity (v_LOS), magnetic field strength (B) and inclination (gamma) while the previous papers have focused mainly on T. We synthesize the Stokes profiles of Fe I 6301.5 A and 6302.5 A lines in both LTE and NLTE using a snapshot of a 3D MHD simulation. The profiles are then inverted in LTE. By considering the atmosphere inferred from inversion of LTE profiles to be the fiducial model, we compare atmosphere from the inversion of NLTE profiles with it. Any differences observed are attributed to NLTE effects. Neglecting the NLTE effects introduces errors in the inverted atmosphere. While the errors in T can go up to 13%, in v_LOS and B the errors can be as high as 50% or more. We find these errors to be present at all three inversion nodes. Importantly, they survive degradation from spatial averaging of the profiles. We give an overview of how the neglect of NLTE effects influences the values of T, v_LOS, B and gamma determined by inverting Fe I 6300 A line pair, as observed, e.g., by Hinode. Errors are found at the sites of granules, intergranular lanes, magnetic elements, basically in every region susceptible to NLTE effects. For an accurate determination of atmospheric quantities and their stratification, it is therefore important to take account of NLTE effects.