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<ri:Resource created="2012-04-20T07:46:38Z" 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>Coronal type II radio bursts in 2002</title><shortName>J/ApJ/710/L58</shortName><identifier>ivo://CDS.VizieR/J/ApJ/710/L58</identifier><altIdentifier>doi:10.26093/cds/vizier.17109058</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lobzin V.V.</name></creator><creator><name>Cairns I.H.</name></creator><creator><name>Robinson P.A.</name></creator><creator><name>Steward G.</name></creator><creator><name>Patterson G.</name></creator><date role="Updated">2012-05-07T10:05:52Z</date><date role="Created">2012-04-20T07:46:38Z</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><subject>radio-sources</subject><description>Major space weather events such as solar flares and coronal mass ejections are usually accompanied by solar radio bursts, which can potentially be used for real-time space weather forecasts. Type II radio bursts are produced near the local plasma frequency and its harmonic by fast electrons accelerated by a shock wave moving through the corona and solar wind with a typical speed of ~1000km/s. The coronal bursts have dynamic spectra with frequency gradually falling with time and durations of several minutes. This Letter presents a new method developed to detect type II coronal radio bursts automatically and describes its implementation in an extended Automated Radio Burst Identification System (ARBIS 2). Preliminary tests of the method with spectra obtained in 2002 show that the performance of the current implementation is quite high, ~80%, while the probability of false positives is reasonably low, with one false positive per 100-200hr for high solar activity and less than one false event per 10000hr for low solar activity periods. The first automatically detected coronal type II radio burst is also presented.</description><source format="bibcode">2010ApJ...710L..58L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/710/L58</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/ApJ/710/1111">J/ApJ/710/1111 : Interplanetary shocks radio bursts (Gopalswamy+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/119/489">J/A+AS/119/489 : Solar Type II Radio Bursts, 1990.09 - 1993.12 (Mann+ 1996)</relatedResource><relatedResource>ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SOLAR_RADIO/SPECTRAL/2002/SPEC_NEW.02 :</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/710/L58</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/710/L58</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/710/L58</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/710/L58</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/710/L58</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/710/L58</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"/><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/710/L58/table1</name><description>Type II radio bursts observed at Learmonth observatory in 2002</description><column><name>Int</name><description>[1,3] Intensity</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><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>? Event number (1)</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>m_Seq</name><description>[ab] Combined events have the same "Seq" number followed by letters a and b</description><ucd>meta.code.multip</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Obs</name><description>Date of the observation</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Stime</name><description>UT start time</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Etime</name><description>UT end time</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Sfreq</name><description>Start frequency</description><unit>MHz</unit><ucd>time.start;em.freq</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>u_Sfreq</name><description>[:] Uncertainty flag on Sfreq</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Efreq</name><description>End frequency</description><unit>MHz</unit><ucd>time.end;em.freq</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>u_Efreq</name><description>[:] Uncertainty flag on Efreq</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>True</name><description>[0/1]? Number of true positives in daily spectra</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_True</name><description>[dn] event not taken into account (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>False</name><description>[0,3]? Number of false alarms in daily spectra</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_False</name><description>[dn] event not taken into account (2)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column></table></schema></tableset></ri:Resource>