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<ri:Resource created="2012-04-17T12:44:26Z" 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>Observations of interplanetary shocks</title><shortName>J/ApJ/710/1111</shortName><identifier>ivo://CDS.VizieR/J/ApJ/710/1111</identifier><altIdentifier>doi:10.26093/cds/vizier.17101111</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gopalswamy N.</name></creator><creator><name>Xie H.</name></creator><creator><name>Makela P.</name></creator><creator><name>Akiyama S.</name></creator><creator><name>Yashiro S.</name></creator><creator><name>Kaiser M.L.,Howard R.A.</name></creator><creator><name>Bougeret J.-L.</name></creator><date role="Updated">2018-02-27T10:36:58Z</date><date role="Created">2012-04-17T12:44:26Z</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>We report on the radio-emission characteristics of 222 interplanetary (IP) shocks detected by spacecraft at Sun-Earth L1 during solar cycle 23 (1996 to 2006, inclusive). A surprisingly large fraction of the IP shocks (~34%) was radio quiet (RQ; i.e., the shocks lacked type II radio bursts). We examined the properties of coronal mass ejections (CMEs) and soft X-ray flares associated with such RQ shocks and compared them with those of the radio-loud (RL) shocks. The CMEs associated with the RQ shocks were generally slow (average speed ~535km/s) and only ~40% of the CMEs were halos. The corresponding numbers for CMEs associated with RL shocks were 1237km/s and 72%, respectively. Thus, the CME kinetic energy seems to be the deciding factor in the radio-emission properties of shocks.</description><source format="bibcode">2010ApJ...710.1111G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/710/1111</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/709/1238">J/ApJ/709/1238 : Comparison of global model with CMEs (Yeates+, 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 ivo-id="ivo://CDS.VizieR/J/A+A/304/563">J/A+A/304/563 : Cool X-ray flares of Sun with GOES (Phillips+, 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/110/99">J/A+AS/110/99 : White-light flares models (Fang+, 1995)</relatedResource><relatedResource>http://wind.nasa.gov/mfi/ : WIND spacecraft Magnetic Field Investigation</relatedResource><relatedResource>http://www.cfa.harvard.edu/shocks/ : CfA interplanetary shock database</relatedResource><relatedResource>http://cdaw.gsfc.nasa.gov/CME_list/ : SOHO LASCO CME catalog online</relatedResource><relatedResource>http://cdaw.gsfc.nasa.gov/CME_list/radio/waves_type2.html : Wind/WAVES type</relatedResource><relatedResource>ftp://ftp.ngdc.noaa.gov/STP/SOLAR_DATA/SOLAR_RADIO/SPECTRAL/</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/Type_II/Type_II_1994-2009">Type_II/Type_II_1994-2009 : type II burst data available on line at the</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/710/1111</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/710/1111</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/710/1111</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/710/1111</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/710/1111</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/710/1111</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/ApJ/710/1111/table1</name><description>List of IP shocks observed during solar cycle 23 and their source information</description><column><name>CMEtime</name><description>IP CME arrival time</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>SF-Size</name><description>Solar Flare size in soft X-rays (5)</description><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</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>IP</name><description>Interplanetary shock arrival date</description><unit>s</unit><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Inst</name><description>[WAS, ] shock observing spacecrafts (Wind, ACE or SOHO)</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>IP-Vel</name><description>Interplanetary shock speed</description><unit>km/s</unit><ucd>phys.veloc;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ma</name><description>Interplanetary shock Alfvenic Mach number (M_A_; Eq. 1 and section 3.1)</description><ucd>phys.veloc;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_Ma</name><description>Source of Mach number computation (2)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CMEt</name><description>Coronal Mass Ejection (CME) type (3)</description><ucd>meta.code.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Tstd</name><description>? IP CME shock standoff distance expressed as arrival time difference</description><unit>h</unit><ucd>time;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_CMEtime</name><description>[*] Flag indicating CMEtime was the next day</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>CME-Vel</name><description>? IP CME shock speed</description><unit>km/s</unit><ucd>phys.veloc;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>CME</name><description>Coronal Mass Ejection white-light date</description><unit>s</unit><ucd>phys.mass</ucd><flag>nullable</flag></column><column><name>PA</name><description>? Coronal Mass Ejection white-light central position angle</description><unit>deg</unit><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>f_PA</name><description>[H/D]? H: Halo ; D: DG (4)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>l_CME-W</name><description>Limit flag on CME-W</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>CME-W</name><description>? Coronal Mass Ejection white-light width</description><unit>deg</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>CME-V</name><description>? Coronal Mass Ejection white-light speed</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>CME-a</name><description>? Coronal Mass Ejection white-light acceleration</description><unit>m.s**-2</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SF-Loc</name><description>Solar Flare location</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>SF-Dur</name><description>Solar Flare duration (hhmm-hhmm)</description><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>MC</name><description>[0/1]? Type II Burst metric type II code (1: metric emission or 0: no metric)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>IIBtime</name><description>Type II Burst metric onset time</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>DH</name><description>[0,3]? Type II Burst decameter-hectometric type II code (6)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>DHtime</name><description>Type II Burst decameter-hectometric onset time</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>Note</name><description>Comment number(s) (see notes.dat file)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column></table><table><name>J/ApJ/710/1111/notes</name><description>Notes</description><column><name>Note</name><description>Code of note</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Text</name><description>Text of note</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="72*">char</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></table></schema></tableset></ri:Resource>