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<ri:Resource created="2005-03-24T14:09:21Z" 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>Center-to-limb variation of quiet Sun</title><shortName>J/A+A/423/1109</shortName><identifier>ivo://CDS.VizieR/J/A+A/423/1109</identifier><altIdentifier>doi:10.26093/cds/vizier.34231109</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Allende Prieto C.</name></creator><creator><name>Asplund M.</name></creator><creator><name>Fabiani Bendicho P.</name></creator><date role="Updated">2017-07-06T06:26:00Z</date><date role="Created">2005-03-24T14:09:21Z</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>We present new observations of the center-to-limb variation of spectral lines in the quiet Sun. Our long-slit spectra are corrected for scattered light, which amounts to 4-8% of the continuum intensity, by comparison with a Fourier transform spectrum of the disk center. Different spectral lines exhibit different behaviors, depending on their sensitivity to the physical conditions in the photosphere and the range of depths they probe as a function of the observing angle, providing a rich database to test models of the solar photosphere and line formation.</description><source format="bibcode">2004A&amp;A...423.1109A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/423/1109</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/423/1109</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/423/1109</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/423/1109</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/423/1109</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/423/1109</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/423/1109</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/423/1109/table1</name><description>Observations</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Lambda</name><description>Central wavelength</description><unit>nm</unit><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R'</name><description>Resolving power measured relative to that of the Fourier transform spectrograph (FTS) spectra</description><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>S</name><description>Amount of scattered light expressed as a fraction of the pseudo-continuum intensity.</description><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>thetamax</name><description>Maximum value of the observing heliocentric angle, theta</description><unit>deg</unit><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FTS00</name><description>theta=00{deg} FTS spectrum file name, in sp/</description><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>FTS15</name><description>theta=15{deg} FTS spectrum file name, in sp/</description><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>FTS30</name><description>theta=30{deg} FTS spectrum file name, in sp/</description><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>FTS45</name><description>theta=45{deg} FTS spectrum file name, in sp/</description><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>FTS60</name><description>theta=60{deg} FTS spectrum file name, in sp/</description><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>FTSmax</name><description>theta=thetamax, 75 or 80{deg}, FTS spectra file name, in sp/</description><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column></table></schema></tableset></ri:Resource>