Synthetic lines in the Sun Virtual Observatory Resource

Authors
  1. de la Cruz Rodriguez J.
  2. Kiselman D.
  3. Carlsson M.
  4. Published by
    CDS
Abstract

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.

Keywords
  1. the-sun
  2. astronomical-models
  3. stellar-atmospheres
  4. spectroscopy
Bibliographic source Bibcode
2011A&A...528A.113D
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/528/A113
IVOA Identifier IVOID
ivo://CDS.VizieR/J/A+A/528/A113
Document Object Identifer DOI
doi:10.26093/cds/vizier.35280113

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/528/A113
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/528/A113
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/528/A113
IVOA Table Access TAP
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History

2011-03-11T09:26:29Z
Resource record created
2011-03-11T09:26:29Z
Created
2011-07-06T23:04:57Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr