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The magnetic field of the quiet-Sun chromosphere remains a mystery for solarphysicists. The reduced number of chromospheric lines are intrinsically hard tomodel and only a few of them are magnetically sensitive. In this work, we use a3D numerical simulation of the outer layers of the solar atmosphere, to assesthe reliability of non-LTE inversions, in this case applied to the Ca II 8542\AA\ line. We show that NLTE inversions provide realistic estimates of physicalquantities from synthetic observations.

Chromospheric magnetic fields. Observations, simulations and their interpretation