Accelerating 3D Non-LTE Synthesis with Graph Neural Networks
A. Vicente Ar\'evalo, A. Asensio Ramos, C. J. D\'iaz Baso

TL;DR
This paper introduces a Graph Neural Network-based method to efficiently compute 3D non-LTE atomic populations in the solar atmosphere, significantly speeding up spectral synthesis while maintaining accuracy.
Contribution
It extends previous 1.5D GNN approaches to full 3D, enabling fast and accurate non-LTE calculations in complex solar atmospheric models.
Findings
GNN predictions exceed 0.99 correlation in the photosphere and mid-chromosphere.
Inference speed is approximately one million times faster than traditional methods.
Spectral line profiles are reproduced with less than 2% residuals.
Abstract
Spectropolarimetric interpretation of chromospheric lines requires solving the radiative transfer problem under non-local thermodynamic equilibrium (non-LTE) conditions. This means computing atomic-level populations self-consistently with the radiation field. While traditional inversion codes employ 1.5D approximations, they neglect horizontal radiative transfer, which can be significant near magnetic structures and in the chromosphere. We present a method to solve 3D atomic-level populations using Graph Neural Networks (GNNs), extending prior 1.5D work to the full 3D domain. By discretizing the solar atmosphere as a directed graph, in which nodes encode physical properties and edges encode spatial distances, an Encode-Process-Decode GNN propagates information to efficiently capture radiative coupling. The network is trained on a Bifrost simulation using Ca II populations from Multi3D…
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