J/A+AS/113/237ivo://CDS.VizieR/J/A+AS/113/237CDSSamain D.1997-12-09T17:51:18Z1997-12-09T18:51:15ZCDS support team

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

cds-question@unistra.frthe-sunspectroscopyultraviolet-astronomyAn ultraviolet atlas of the solar spectrum with a spectral resolution of 15mA in the region 1948-2000A is presented. It is the first part of the spectra recorded on the quiet Sun between 1900 and 2130A. Measurements were performed from a balloon-borne instrumentation flown at an altitude of 39km. The wavelength atlas with a list of about 550 lines has been synthesized from data at center of the Sun ({mu}=1) and at {mu}=0.89, smoothed out over an area of 30 arcsec. The wavelength scale is given with respect to the average solar spectrum. Tracings are presented at {mu}=0.89, with an intensity scale adjusted in absolute values on the level of the continuum near 2000A.1995A&AS..113..237Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/113/237CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/113/237https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/113/237http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/113/237https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/113/237https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/113/237http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/113/237GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapUVdefaultJ/A+AS/113/237/table3Observed wavelengths, laboratory values and identificationsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSpOrdSpectrum orderinstr.orderintSolLamWavelength determination of all solar and telluric lines measurable on the spectrum (1)0.1nmem.wldoublen_SolLamSee Note (2)meta.notecharIntens[]? Intensity of the line in an arbitrary scale from 0 to 9 (3)meta.code;spect.line.intensityintn_IntensWhen '?' uncertain valuemeta.notecharTypeAcronyms for the type of line (4)meta.notecharIdentifPossible element responsible for the observed line (5)phys.atmol.elementcharLabLamLaboratory wavelength0.1nmem.wl;phys.atmol.transitioncharn_LabLam[St] When 'St' the line is used or recommended as reference wavelength standardmeta.notecharr_LabLamReferences of the wavelength sources (6)meta.refcharDLam[]? Difference between the observed wavelength and the laboratory wavelength: dlambda=lambda(Sun or O2) - lambda(lab)0.1nmem.wl;arith.difffloat