[en] Even though the solar photospheric abundances are now on the whole in very good agreement with the meteoritic values, some problems remain which will only be solved with a higher level of accuracy in the atomic data, especially the transition probabilities for faint lines. The authors justify this request for many more very accurate gf-values through a few particularly striking points.
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Grevesse, Nicolas ; Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO)