J/A+A/528/A113ivo://CDS.VizieR/J/A+A/528/A113doi:10.26093/cds/vizier.35280113CDSde la Cruz Rodriguez J.Kiselman D.Carlsson M.2011-07-06T23:04:57Z2011-03-11T09:26:29ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frthe-sunastronomical-modelsstellar-atmospheresspectroscopyWe 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=0.3.2011A&A...528A.113Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/528/A113CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJS/91/461 : EUV spectrum of solar active region (Thomas+, 1994)J/A+AS/113/71 : Lines in the infrared solar spectrum (Ramsauer+, 1995)J/A+AS/126/281 : Solar disk spectrum (660-1175A) (Curdt+ 1997)J/A+A/375/591 : SUMER Spectral Atlas of Solar Disk Features (Curdt+, 2001)J/ApJS/181/351 : Solar flux model in 30-1300nm wavelength range (Killen+, 2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/528/A113https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/528/A113http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/528/A113https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/528/A113https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/528/A113http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/528/A113GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/A+A/528/A113/linesLines studied: C5380.3, Ca8498.0, Ca8542.1, Ca8662.2, Fe5250.2, Fe5250.6, Fe5576.1, Fe6082.7, Fe6301.5, Fe6302.5, Fe7090.4recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintElElement (C, Ca or Fe)phys.atmol.elementcharVdopDoppler velocity (1)m/sspect.dopplerVelocdoublelambdaWavelength0.1nmem.wldoublelambdaCCentral Wavelength of the line0.1nmem.wl.central;spect.linedoubleNfactFTS atlas normalization factor (multiplicative) (2)arith.factordoublespPlot of spectrum for this linemeta.ref.urlcharI1.0Intensity at {mu}=1.0 (2)W.m**-2.Hz**-1.sr**-1spect.line.intensitydoubleI0.9Intensity at {mu}=0.9 (2)W.m**-2.Hz**-1.sr**-1spect.line.intensitydoubleI0.8Intensity at {mu}=0.8 (2)W.m**-2.Hz**-1.sr**-1spect.line.intensitydoubleI0.7Intensity at {mu}=0.7 (2)W.m**-2.Hz**-1.sr**-1spect.line.intensitydoubleI0.6Intensity at {mu}=0.6 (2)W.m**-2.Hz**-1.sr**-1spect.line.intensitydoubleI0.5Intensity at {mu}=0.5 (2)W.m**-2.Hz**-1.sr**-1spect.line.intensitydoubleI0.4Intensity at {mu}=0.4 (2)W.m**-2.Hz**-1.sr**-1spect.line.intensitydoubleI0.3Intensity at {mu}=0.3 (2)W.m**-2.Hz**-1.sr**-1spect.line.intensitydouble