Open uheiter opened 6 months ago
The set of solar abundances from Magg. et al. (2022) that is included in Turbospectrum uses the meteoritic abundances (A(El)met column on the right in Table 5 of Magg et al.): https://github.com/bertrandplez/Turbospectrum_NLTE/blob/8d8cad0856f09d9fa34e59199fd24dfeb28447b5/source/makeabund.f#L117-L130
What is the reason for this choice? It should also be explained in the documentation.
Note that the other two sets use photospheric abundances, and TSFitPy also uses the photospheric abundances from Magg (A(El)ph column on the left in Table 5): https://github.com/TSFitPy-developers/TSFitPy/blob/main/scripts/solar_abundances.py
The set of solar abundances from Magg. et al. (2022) that is included in Turbospectrum uses the meteoritic abundances (A(El)met column on the right in Table 5 of Magg et al.): https://github.com/bertrandplez/Turbospectrum_NLTE/blob/8d8cad0856f09d9fa34e59199fd24dfeb28447b5/source/makeabund.f#L117-L130
What is the reason for this choice? It should also be explained in the documentation.
Note that the other two sets use photospheric abundances, and TSFitPy also uses the photospheric abundances from Magg (A(El)ph column on the left in Table 5): https://github.com/TSFitPy-developers/TSFitPy/blob/main/scripts/solar_abundances.py