Oxygen lines in solar granulation. I.

DOI

We seek to provide additional tests of the line formation of theoretical 3D solar photosphere models. In particular, we set out to test the spatially-resolved line formation at several viewing angles, from the solar disk-centre to the limb and focusing on atomic oxygen lines. The purpose of these tests is to provide additional information on whether the 3D model is suitable to derive the solar oxygen abundance. We also aim to empirically constrain the NLTE recipes for neutral hydrogen collisions, using the spatially-resolved observations of the OI 777nm lines.

Associated data

Identifier
DOI http://doi.org/10.26093/cds/vizier.35070417
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/507/417
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/507/417
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/507/417
Related Identifier https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/507/417
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/507/417
Provenance
Creator Pereira T.M.D.; Kiselman D.; Asplund; M.
Publisher CDS
Publication Year 2010
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics; Solar System Astronomy