Combining multiple structural inversions to constrain the solar modelling problem

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Combining multiple structural inversions to constrain the solar modelling problem	2 MB	Adobe Acrobat PDF	Read	Download
DOI Доступ к ресурсу на сайте издателя			10.1051/0004-6361/201833971

Title: Combining multiple structural inversions to constrain the solar modelling problem
Creator: Salmon, S. J. A. J.
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Noels, Arlette
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Scuflaire, R.
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Montalbán, Josefina
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Baturin, V. A.
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Eggenberger, Patrick
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Gryaznov, V. K.
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Iosilevskiy, I. L.
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Meynet, G.
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Chaplin, W. J.
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Miglio, A.
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Oreshina, A. V.
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Richard, O.
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Starostin, A. N.
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Buldgen, G.
Date: 2019
DOI: 10.1051/0004-6361/201833971
Description: Context. The Sun is the most studied of all stars, which serves as a reference for all other observed stars in the Universe. Furthermore, it also serves the role of a privileged laboratory of fundamental physics and can help us better understand processes occuring in conditions irreproducible on Earth. However, our understanding of our star is currently lessened by the so-called solar modelling problem, resulting from comparisons of theoretical solar models to helioseismic constraints. These discrepancies can stem from various causes, such as the radiative opacities, the equation of state as well as the mixing of the chemical elements.

Created: 08-07-2019

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Научное управление Combining multiple structural inversions to constrain the solar modelling problem