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<ri:Resource created="2014-06-06T14:20:23Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" 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/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd 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>Occultations through Saturn's C ring</title><shortName>J/AJ/146/12</shortName><identifier>ivo://CDS.VizieR/J/AJ/146/12</identifier><altIdentifier>doi:10.26093/cds/vizier.51460012</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Hedman M.M.</name></creator><creator><name>Nicholson P.D.</name></creator><date role="Updated">2021-08-23T06:55:24Z</date><date role="Created">2014-06-06T14:20:23Z</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>solar-system-planets</subject><subject>occultation</subject><description>Saturn's C ring contains multiple spiral patterns that appear to be density waves driven by periodic gravitational perturbations. In other parts of Saturn's rings, such waves are generated by Lindblad resonances with Saturn's various moons, but most of the wave-like C-ring features are not situated near any strong resonance with any known moon. Using stellar occultation data obtained by the Visual and Infrared Mapping Spectrometer on board the Cassini spacecraft, we investigate the origin of six unidentified C-ring waves located between 80900 and 87200km from Saturn's center. By measuring differences in the waves' phases among the different occultations, we are able to determine both the number of arms in each spiral pattern and the speeds at which these patterns rotate around the planet. We find that all six of these waves have between two and four arms and pattern speeds between 1660{deg}/day and 1861{deg}/day. These speeds are too large to be attributed to any satellite resonance. Instead, they are comparable to the predicted pattern speeds of waves generated by low-order normal-mode oscillations within the planet. The precise pattern speeds associated with these waves should therefore provide strong constraints on Saturn's internal structure. Furthermore, we identify multiple waves with the same number of arms and very similar pattern speeds, indicating that multiple m=3 and m=2 sectoral (l=m) modes may exist within the planet.</description><source format="bibcode">2013AJ....146...12H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/146/12</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>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/1183">J/A+A/493/1183 : Saturn major satellites observations (1874-2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/2214">J/AJ/136/2214 : Positions of Saturn and its satellites in 2002-2006</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/485/293">J/A+A/485/293 : Events of Saturn satellites during 2009 equinox (Arlot+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/422/377">J/A+A/422/377 : 1997-2000 Saturn's satellites astrometry (Qiao+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/383/1054">J/A+A/383/1054 : Astrometry of Pluto and Saturn in 1995-2001 (Rapaport+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/383/296">J/A+A/383/296 : Saturnian Satellites positions (1996-2000) (Peng+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/380/727">J/A+A/380/727 : 1995 Saturnian satellite observations (Vienne+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/139/47">J/A+AS/139/47 : 1995 Saturnian satellites mutual events (Emelianov+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/139/305">J/A+AS/139/305 : Position of Saturn's satellites (1982-1988) (Veiga+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/136/257">J/A+AS/136/257 : Saturn's satellites in 1995/97 (Harper+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/121/65">J/A+AS/121/65 : 1990-1994 Saturn's satellites astrometry (Harper+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/103/983">J/AJ/103/983 : Stellar occultation candidates of Saturn (Bosh+, 1992)</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/AJ/146/12</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/146/12</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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