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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

Figure 1: Relative differences in squared adiabatic sound speed between the Sun and standard solar models built using various opacity tables.
Figure 2: Relative differences in squared adiabatic sound speed between the Sun and standard solar models built using various abundance tables of the heavy elements.
Figure 5: Relative differences in squared adiabatic sound speed between the Sun and solar models built using an ad-hoc modi- modi-fication of the mean Rosseland opacity and additional mixing of the chemical elements at the base of the convective zone.
Figure 7: Differences in Ledoux discriminant, A, between the Sun and solar models built using an ad-hoc modification of the mean Rosseland opacity and additional mixing of the chemical elements at the base of the convective zone.

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This indicates that an approach using simultaneously all the information of these inversions could per- haps be used to derive a more precise estimation of the required opacity