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Combining multiple structural inversions to constrain the solar modelling problem

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Academic year: 2021

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Figure

Table 1: Parameters of the standard solar models used in this study
Fig. 2: Relative differences in entropy proxy, S 5/3 , between the Sun and calibrated solar models
Fig. 4: Relative differences in adiabatic gradient between the CEFF, OPAL and FreeEOS equation of state with respect to the
Fig. 5: Inversion results for models with modified opacities including a gaussian peak of fixed height and width at various temperatures (see text for details)
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