Derive
abundance
Reported abundances are on the "12+log-epsilon" scale, i.e. log10 of the fraction of nuclei of
the element in any form relative to the number of hydrogen in any form plus an offset of 12. For the Sun, the abundance
values of H, He, and Li are approximately 12, 10.9, and 1.05.
If stellar parameters (Teff, logg and monh) are fixed, abundances may be derived using
only the lines selected below.
Stellar structure
prediction (optional)
When activated, surface abundances are reported during post-processing.
