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In the past years, a systematic downward revision of the metallicity of the Sun has led to the "solar modeling problem", namely the disagreement between predictions of standard solar models and inferences from helioseismology.
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Vagnozzi, S.; Freese, K.; Zurbuchen, T.H. Solar models in light of new high metallicity measurements from solar wind data. Astrophys. J. 2017
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Yang, W. Rotating Solar Models with Low Metal Abundances as Good as Those with High Metal Abundances. Astrophys. J. 2019
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