J/A+AS/119/489ivo://CDS.VizieR/J/A+AS/119/489CDSMann G.Klassen A.Classen H.-T.Aurass H.Scholz D.,MacDowall R. J.Stone R. G.1998-02-24T16:38:06Z1998-02-24T17:37:52ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frthe-sunSolar type II radio bursts represent the radio signature of shock waves travelling through the solar corona. They are associated with flares, coronal mass ejections (CME's) and interplanetary shocks. Type II radio bursts appear as emission stripes slowly drifting from high to low frequencies in dynamic radio spectra. The spectral features of all solar type II radio bursts observed by the new radiospectrograph of the Astrophysikalisches Institut Potsdam in Tremsdorf during the time period from September 1, 1990 to December 31, 1993, i.e., during the first part of the ULYSSES spacecraft mission, are summarized and statistically investigated.1996A&AS..119..489Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/119/489CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/119/489https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/119/489http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/119/489https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/119/489https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/119/489http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/119/489GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/119/489/table1Solar type II radio bursts (Sep 1990-Dec 1993)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintOBSdateDate of observationtime.epochnullableOBShsStart time of observation (hours)htime.epochintOBSmsStart time of observation (minutes)mintime.epochfloatn_OBSms[EU] Note on start time of observation (1)meta.notecharOBSheEnd time of observation (hours)htime.epochintOBSmeEnd time of observation (minutes)mintime.epochfloatn_OBSme[EU] Note on end time of observation (1)meta.notecharEvenKind of event (2)meta.codecharLowFreqLower value of the frequence rangeMHzinstr.bandwidthintUppFreqUpper value of the frequence rangeMHzem.freqintJ/A+AS/119/489/table2Observed solar type II radio burstsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNo? Sequential numbermeta.idintnullablen_No[a] a for average (last line)meta.notecharDateObservation datetime.epochnullableDay? [1/365] Number of the daytime.epochintnullableUT? Begining of observation time (UT hours)time.epochnullableUT2? End of observation time (UT hours)time.epochnullableStructGeneral spectral structure (fundamental (F), harmonic (H))src.spTypechar<Deltaf/f>? Mean value of the instantaneous bandwidthinstr.paramfloatnullablee_<Deltaf/f>? rms uncertainty on Deltafstat.errorfloatnullable<Deltaf/f>F? Fundamental band instantaneous bandwidthinstr.paramfloatnullable<Deltaf/f>H? Harmonic band instantaneous bandwidthinstr.paramfloatnullable<Df>Mean value of the drift rateMHz/sarith.rate;em.freqfloate_<Df>rms uncertainty on <Df>MHz/sstat.errorfloat<DfF>? Fundamental band drift rateMHz/sarith.rate;em.freqfloatnullable<DfH>? Harmonic band drift rateMHz/sarith.rate;em.freqfloatnullablel_Freq[~] Limit flag on Freqmeta.code.errorcharFreq? Frequence or upper value of frequence rangeMHzem.freqintnullableFreq2? Lower value of frequence when frequence rangeMHzem.freqintnullable<fH/fF>? Mean value of the frequency ratio between the harmonic and fundamental bandem.freq;arith.ratiofloatnullablee_<fH/fF>? rms uncertainty on <fH/fF>stat.errorfloatnullable<fH/fF>u? Upper value of the frequency ratio between the harmonic and fundamental bandem.freq;arith.ratiofloatnullable<fH/fF>l? Lower value of the frequency ratio between the harmonic and fundamental bandem.freq;arith.ratiofloatnullable