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<ri:Resource created="2023-03-02T08:51:39Z" 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>Quiescent coronal loops observed with CoMP</title><shortName>J/ApJ/919/74</shortName><identifier>ivo://CDS.VizieR/J/ApJ/919/74</identifier><altIdentifier>doi:10.26093/cds/vizier.19190074</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Tiwari A.K.</name></creator><creator><name>Morton R.J.</name></creator><creator><name>McLaughlin J.A.</name></creator><date role="Updated">2023-09-27T10:55:30Z</date><date role="Created">2023-03-02T08:51:39Z</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><description>The Coronal Multi-channel Polarimeter (CoMP) has opened up exciting opportunities to probe transverse MHD waves in the Sun's corona. The archive of CoMP data is utilized to generate a catalog of quiescent coronal loops that can be used for studying propagating kink waves. The catalog contains 120 loops observed between 2012 and 2014. This catalog is further used to undertake a statistical study of propagating kink waves in the quiet regions of the solar corona, investigating phase speeds, loop lengths, footpoint power ratio (a measure of wave power entering the corona through each footpoint of a loop) and equilibrium parameter (which provides a measure of the change in wave amplitude) values. The statistical study enables us to establish the presence of a relationship between the rate of damping and the length of the coronal loop, with longer coronal loops displaying weaker wave damping. We suggest the reason for this behavior is related to a decreasing average density contrast between the loop and ambient plasma as loop length increases. The catalog presented here will provide the community with the foundation for the further study of propagating kink waves in the quiet solar corona.</description><source format="bibcode">2021ApJ...919...74T</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/919/74</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/MNRAS/456/1542">J/MNRAS/456/1542 : Coronal mass ejections transit times (Sudar+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/587/A29">J/A+A/587/A29 : Time and positions of coronal bright points (Sudar+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/SoPh/294.144">J/other/SoPh/294.144 : Coronal hole parameters (Heinemann+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/241/31">J/ApJS/241/31 : Kink oscillations of solar coronal loops (Nechaeva+, 2019)</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/ApJ/919/74</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/919/74</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/919/74</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/919/74</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/919/74</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/919/74</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"/></coverage><tableset><schema><name>default</name><table><name>J/ApJ/919/74/table2</name><description>Measured loop parameters and wave parameters obtained from 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>Seq</name><description>[1/120] Internal loop index number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>X</name><description>[-1163/1140] Solar X position</description><unit>arcsec</unit><ucd>pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Y</name><description>[-1075/1060] Solar Y position</description><unit>arcsec</unit><ucd>pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Date</name><description>Observation date</description><ucd>time.epoch;obs</ucd><flag>nullable</flag></column><column><name>Length</name><description>[42/585] Half-loop length</description><unit>Mm</unit><ucd>phys.size</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Length</name><description>[3.23] Uncertainty in Length</description><unit>Mm</unit><ucd>stat.error;phys.size</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>xi</name><description>[-163/299] Equilibrium parameter</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_xi</name><description>[0.5/50] Uncertainty in xi</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PRatio</name><description>[0.45/2.61] Power ratio</description><ucd>phot.flux;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PRatio</name><description>[0.17/1.1] Uncertainty in PRatio</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PVel</name><description>[202/738] Phase velocity</description><unit>km/s</unit><ucd>phys.veloc;time.phase</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_PVel</name><description>[2/43] Uncertainty in PVel</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>