Synthetic lines in the Sun

DOI

We have computed synthetic spectra from a realistic 3D numerical simulation of the solar photosphere. We provide the spatially averaged spectra for selected lines that are commonly used on solar applications. These data can be used to calibrate Doppler velocity measurements in the solar photosphere. The calculations are carried out along the solar disk from heliocentric angle mu=1.0 to mu=0.3.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35280113
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/528/A113
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/528/A113
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/528/A113
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/528/A113
Provenance
Creator de la Cruz Rodriguez J.; Kiselman D.; Carlsson M.
Publisher CDS
Publication Year 2011
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; Natural Sciences; Observational Astronomy; Physics; Solar System Astronomy; Stellar Astronomy