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<ri:Resource created="2012-05-21T13:50:33Z" status="active" updated="2025-06-13T15:25:00Z" 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>Faraday rotation at high Galactic latitude</title><shortName>J/ApJ/714/1170</shortName><identifier>ivo://CDS.VizieR/J/ApJ/714/1170</identifier><altIdentifier>doi:10.26093/cds/vizier.17141170</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Mao S.A.</name></creator><creator><name>Gaensler B.M.</name></creator><creator><name>Haverkorn M.</name></creator><creator><name>Zweibel E.G.</name></creator><creator><name>Madsen G.J.,McClure-Griffiths N.M.</name></creator><creator><name>Shukurov A.</name></creator><creator><name>Kronberg P.P.</name></creator><date role="Updated">2017-06-20T13:16:13Z</date><date role="Created">2012-05-21T13:50:33Z</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>milky-way-galaxy</subject><subject>magnetic-fields</subject><subject>radio-sources</subject><subject>polarimetry</subject><subject>galaxy-rotation</subject><description>We present a study of the vertical magnetic field of the Milky Way toward the Galactic poles, determined from observations of Faraday rotation toward more than 1000 polarized extragalactic radio sources at Galactic latitudes |b|&gt;=77{deg}, using the Westerbork Radio Synthesis Telescope and the Australia Telescope Compact Array. We find median rotation measures (RMs) of 0.0+/-0.5rad/m^2^ and +6.3+/-0.7rad/m^2^ toward the north and south Galactic poles, respectively, demonstrating that there is no coherent vertical magnetic field in the Milky Way at the Sun's position. If this is a global property of the Milky Way's magnetism, then the lack of symmetry across the disk rules out pure dipole or quadrupole geometries for the Galactic magnetic field. The angular fluctuations in RM seen in our data show no preferred scale within the range ~0.1{deg} to ~25{deg}. The observed standard deviation in RM of ~9rad/m^2^ then implies an upper limit of ~1uG on the strength of the random magnetic field in the warm ionized medium at high Galactic latitudes.</description><source format="bibcode">2010ApJ...714.1170M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/714/1170</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/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/513/A65">J/A+A/513/A65 : Rotation measures in the fourth Galactic quadrant (Nota+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/702/1230">J/ApJ/702/1230 : Rotation measure image of the sky (Taylor+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/386/1881">J/MNRAS/386/1881 : New pulsar rotation measures (Noutsos+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/663/258">J/ApJ/663/258 : Rotation measures of extragalactic sources in SGPS (Brown+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/642/868">J/ApJ/642/868 : Rotation measures for 223 pulsars (Han+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/145/213">J/ApJS/145/213 : Rotation measures of compact sources in CGPS (Brown+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/276">J/A+A/372/276 : Polarization catalogue for NGP area (Berdyugin+, 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/ApJ/714/1170</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/714/1170</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/714/1170</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/714/1170</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/714/1170</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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