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Author Correction: Helioseismic inference of the solar radiative opacity - Nature Communications
Correction to: Nature Communications https://doi.org/10.1038/s41467-024-54793-y, published online 27 January 2025 In the version of the article initially published, Sébastien Salmon (STAR Institute, Université de Liège, Liège, Belgium) was missing from the author list, while Arlette Noels (STAR Institute, Université de Liège, Liège, Belgium) was listed with an incorrect affiliation. The author names and affiliations are now amended in the HTML and PDF versions of the article.
Helioseismic inference of the solar radiative opacity - Nature Communications
Abstract The Sun is the most studied of all stars, and thus constitutes a benchmark for stellar models. However, our vision of the Sun is still incomplete, as illustrated by the current debate on its chemical composition. The problem reaches far beyond chemical abundances and is intimately linked to microscopic and macroscopic physical ingredients of solar models such as radiative opacity, for which experimental results have been recently measured that still await theoretical explanations.
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