<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2010-02-07T16:57:14Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Oxygen lines in solar granulation. II.</title><shortName>J/A+A/508/1403</shortName><identifier>ivo://CDS.VizieR/J/A+A/508/1403</identifier><altIdentifier>doi:10.26093/cds/vizier.35081403</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Pereira T.M.D.</name></creator><creator><name>Asplund M.</name></creator><creator><name>Kiselman D.</name></creator><date role="Updated">2010-02-07T16:05:38Z</date><date role="Created">2010-02-07T16:57:14Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>the-sun</subject><subject>spectroscopy</subject><description>There is a lively debate about the solar oxygen abundance and the role of 3D models in its recent downward revision. These models have been tested using high-resolution solar atlases of flux and disk-centre intensity. Further testing can be done using centre-to-limb variations. Using high-resolution and high S/N observations of neutral oxygen lines across the solar surface, we seek to test that the 3D and 1D models reproduce their observed centre-to-limb variation. In particular we seek to assess whether the latest generation of 3D hydrodynamical solar model atmospheres and NLTE line formation calculations are appropriate to derive the solar oxygen abundance.</description><source format="bibcode">2009A&amp;A...508.1403P</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/508/1403</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/507/417">J/A+A/507/417 : Oxygen lines in solar granulation (Pereira+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/274/555">J/A+A/274/555 : Asymmetry of FeI lines in solar spectrum (Stathopoulou+ 1993)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/304/563">J/A+A/304/563 : Cool X-ray flares of Sun with GOES (Phillips+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/113/71">J/A+AS/113/71 : Lines in the infrared solar spectrum (Ramsauer+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/113/237">J/A+AS/113/237 : Ultraviolet Spectrum of the Sun (Samain, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/309/655">J/A+A/309/655 : Solar chromospheric activity (HeI 10830A) (Shcherbakov+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/313/949">J/A+A/313/949 : Solar chromospheric structures. II. (Bocchialini+, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/126/281">J/A+AS/126/281 : Solar disk spectrum (660-1175A) (Curdt+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/129/41">J/A+AS/129/41 : Fe I line shifts in the Sun (Allende Prieto+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/131/431">J/A+AS/131/431 : Accurate wavelengths in Sun spectrum (Allende Prieto+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/375/591">J/A+A/375/591 : SUMER Spectral Atlas of Solar Disk Features (Curdt+, 2001)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/508/1403</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/508/1403</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/508/1403</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/508/1403</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/508/1403</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/508/1403</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/508/1403/table1</name><description>Observations</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>lambda</name><description>Approximate central wavelength of filter</description><unit>nm</unit><ucd>em.wl.central;instr.filter</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>JDstart</name><description>Julian date (start of observations)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>JDend</name><description>Julian date (end of observations)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>HLAT</name><description>Heliographic latitude in the Stony-Hurst coordinate system</description><unit>deg</unit><ucd>pos.az.alt</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HLON</name><description>Heliographic longitude in the Stony-Hurst coordinate system</description><unit>deg</unit><ucd>pos.eq.ha</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>mu</name><description>Cosine of the heliocentric angle</description><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_mu</name><description>Error in mu</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>S</name><description>Amount of straylight removed from the spectra. Expressed as a percentage of the pseudo-continuum intensity.</description><unit>%</unit><ucd>phot.calib;arith.zp</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>FileName</name><description>Path and filename of each spectrum</description><ucd>meta.id;meta.file</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column></table></schema></tableset></ri:Resource>