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<ri:Resource created="2011-02-23T05:47:30Z" 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>Global plasma parameter simulation of Comet 67P</title><shortName>J/A+A/520/A92</shortName><identifier>ivo://CDS.VizieR/J/A+A/520/A92</identifier><altIdentifier>doi:10.26093/cds/vizier.35200092</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gortsas N.</name></creator><creator><name>Motschmann U.</name></creator><creator><name>Kuehrt E.</name></creator><creator><name>Glassmeier K.-H.</name></creator><creator><name>Hansen K.C.,Mueller J.</name></creator><creator><name>Schmidt A.</name></creator><date role="Updated">2017-06-20T13:16:26Z</date><date role="Created">2011-02-23T05:47:30Z</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>comets</subject><description>The evolution of the plasma environment of comet 67P/Churyumov-Gerasimenko (CG) the target comet of the European Space Agency's (ESA) Rosetta mission is investigated as the comet approaches the Sun. The plasma environment is calculated in three dimensions with a hybrid plasma model. The model treats the dynamics of the solar wind protons and the cometary ions in the framework of the macroparticle approach while the electrons are treated as a massless, charge-neutralizing fluid. The simulation starts at 4.2AU and finishes at 1.3AU, when the comet is at its perihelion position. Two dimensional contour plots of the absolute value of the cometary ion mass flux and the magnetic field in the orthogonal plane of the interplanetary magnetic field are shown. The undisturbed solar wind flows from left to right. The convective electric field points downwards. The nucleus is in the middle of the simulation box. The coma is assumed to consist of water vapor and it increases by several orders of magnitude as the comet approaches the Sun. Therefore, the size of the simulation box is adapted as an animation above the contour plots shows.</description><source format="bibcode">2010A&amp;A...520A..92G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/520/A92</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/B/comets">B/comets : Database of the orbital elements of comets (Rocher, 2007)</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/520/A92</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/520/A92</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/520/A92</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/520/A92</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/520/A92</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/520/A92</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/A+A/520/A92/object</name><description>67P P/Churyumov-Gerasimenko data from B/comets catalog</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>Code</name><description>IAU code for the comet</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>Name</name><description>IAU Name of the comet</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Elem</name><description>Epoch of the computed elements (JD)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>n_Elem</name><description>[0,1] relativistic effects (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>q</name><description>Perihelion distance</description><unit>AU</unit><ucd>pos.distance;src.orbital.periastron</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e</name><description>Orbit eccentricity</description><ucd>src.orbital.eccentricity</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>i</name><description>Inclination of the orbit</description><unit>deg</unit><ucd>src.orbital.inclination</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>H1</name><description>Constant term for magnitude</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>