Non-LTE inversions of the Mg II h&k and UV triplet lines
Jaime de la Cruz Rodr\'iguez, Jorrit Leenaarts, Andr\'es Asensio, Ramos

TL;DR
This paper develops non-LTE inversion techniques for Mg II h&k and UV triplet lines to analyze the solar chromosphere, demonstrating the ability to reconstruct atmospheric models from photosphere to transition region using observations.
Contribution
It introduces a novel non-LTE inversion method including partial redistribution effects and assesses its effectiveness with both simulations and real IRIS spectra.
Findings
Mg II h&k lines enable reconstructing atmospheric models from middle photosphere to transition region.
Multi-line setups can recover full stratification of physical parameters, including magnetic fields.
First successful inversions of IRIS spectra from various solar regions show promising results.
Abstract
The Mg II h&k lines are powerful diagnostics for studying the solar chromosphere. They have become particularly popular with the launch of the IRIS satellite, and a number of studies that include these lines have lead to great progress in understanding chromospheric heating, in many cases thanks to the support from 3D MHD simulations. In this study we utilize another approach to analyze observations: non-LTE inversions of the Mg II h&k and UV triplet lines including the effects of partial redistribution. Our inversion code attempts to construct a model atmosphere that is compatible with the observed spectra. We have assessed the capabilities and limitations of the inversions using the FALC atmosphere and a snapshot from a 3D radiation-MHD simulation. We find that Mg II h&k allow reconstructing a model atmosphere from the middle photosphere to the transition region. We have also explored…
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