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<ri:Resource created="2016-11-10T12:18:38Z" 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>Predicting coronal mass ejections transit times</title><shortName>J/MNRAS/456/1542</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/456/1542</identifier><altIdentifier>doi:10.26093/cds/vizier.74561542</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sudar D.</name></creator><creator><name>Vrsnak B.</name></creator><creator><name>Dumbovic M.</name></creator><date role="Updated">2024-08-15T20:17:16Z</date><date role="Created">2016-11-10T12:18:38Z</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>Predicting transit times (TT) of coronal mass ejections (CMEs) from their initial parameters is a very important subject, not only from the scientific perspective, but also because CMEs represent a hazard for human technology. We used a neural network (NN) to analyse TT for 153 events with only two input parameters: initial velocity of the CME, v, and central meridian distance, CMD, of its associated flare. We found that transit time dependence on v is showing a typical drag-like pattern in the solar wind. The results show that the speed at which acceleration by drag changes to deceleration is v~500km/s. TT are also found to be shorter for CMEs associated with flares on the western hemisphere than those originating on the eastern side of the Sun. We attribute this difference to the eastward deflection of CMEs on their path to 1 au. The average error of the NN prediction in comparison to observations is ~12h which is comparable to other studies on the same subject.</description><source format="bibcode">2016MNRAS.456.1542S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/456/1542</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/A+A/422/337">J/A+A/422/337 : Solar EUV Post-Eruptive Arcades (Tripathi+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/440/373">J/A+A/440/373 : Earthbound interplanetary shocks (Howard+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/709/1238">J/ApJ/709/1238 : Solar Coronal Mass Ejection (Yeates+, 2010)</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/MNRAS/456/1542</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/456/1542</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/456/1542</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/456/1542</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/456/1542</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/456/1542</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/MNRAS/456/1542/table1</name><description>CME transit time data</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>ObsS</name><description>Start date</description><unit>s</unit><ucd>time.start</ucd><flag>nullable</flag></column><column><name>ObsA</name><description>Arrival date</description><unit>s</unit><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>TT</name><description>Transit time</description><unit>h</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>v</name><description>CME velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NS</name><description>[N/S] North/South</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>LAT</name><description>Latitude</description><unit>deg</unit><ucd>pos.earth.lat</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>EW</name><description>[E/W] East/West</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>CMD</name><description>Central meridian distance</description><unit>deg</unit><ucd>pos.angDistance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>