The uncertainty of magnetic fields in 3D non-local thermodynamic equilibrium inversions

We describe our approach to solving the problem of ensuring the solenoidality of the magnetic field vector in 3D inversions, as well as the estimation of the uncertainty in the inferred magnetic field. The solenoidality of the magnetic field vector is often disregarded in the inversion of spectropolarimetric data due to limitations in the traditional 1D inversion techniques. We propose a method for ensuring the solenoidal condition in 3D inversions based on our mesh-free approach. The increase in dimensionality with respect to the 1D inversion techniques is such that some of the traditional methods for determining the uncertainties become unfeasible. We propose a method based on a Monte Carlo approach for determining the uncertainty of the magnetic field inference. Due to the physics of the problem, we can compute the uncertainty while only increasing the total required computational time by a factor of about 2. We also propose a metric for quantifying the uncertainty that thus describes the degree of confidence of the magnetic field inference. Finally, we perform a numerical experiment to demonstrate the feasibility of both the method and the metric proposed to quantify the uncertainty.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2025-06-03
DOI
https://doi.org/10.1051/0004-6361/202554019
Citations
1
Primary Topic
Spectroscopy and Quantum Chemical Studies
Type
article
Field-Weighted Citation Impact
1.25
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article

The uncertainty of magnetic fields in 3D non-local thermodynamic equilibrium inversions

Jiří Štěpán, A. Vicente Arévalo, Tanausú del Pino Alemán
1 citations
Astronomy and Astrophysics
Spectroscopy and Quantum Chemical Studies
1.25
article

The uncertainty of magnetic fields in 3D non-local thermodynamic equilibrium inversions

Jiří Štěpán, A. Vicente Arévalo, Tanausú del Pino Alemán
article en
1 citations

Abstract

We describe our approach to solving the problem of ensuring the solenoidality of the magnetic field vector in 3D inversions, as well as the estimation of the uncertainty in the inferred magnetic field. The solenoidality of the magnetic field vector is often disregarded in the inversion of spectropolarimetric data due to limitations in the traditional 1D inversion techniques. We propose a method for ensuring the solenoidal condition in 3D inversions based on our mesh-free approach. The increase in dimensionality with respect to the 1D inversion techniques is such that some of the traditional methods for determining the uncertainties become unfeasible. We propose a method based on a Monte Carlo approach for determining the uncertainty of the magnetic field inference. Due to the physics of the problem, we can compute the uncertainty while only increasing the total required computational time by a factor of about 2. We also propose a metric for quantifying the uncertainty that thus describes the degree of confidence of the magnetic field inference. Finally, we perform a numerical experiment to demonstrate the feasibility of both the method and the metric proposed to quantify the uncertainty.

Astronomy and AstrophysicsVol. 699
Universidad de La Laguna (ES), Czech Academy of Sciences, Astronomical Institute (CZ), Institut für Sonnenphysik (DE), Instituto de Astrofísica de Canarias (ES)
Openalex Percentile: Top 21%
Spectroscopy and Quantum Chemical Studies
1.25
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The uncertainty of magnetic fields in 3D non-local thermodynamic equilibrium inversions — Jiří Štěpán, A. Vicente Arévalo, et al. · Astronomy and Astrophysics (2025) | TGRS Research Map | TGRS