J/A+AS/105/77ivo://CDS.VizieR/J/A+AS/105/77CDSCornille M.Dubau J.Faucher P.Bely-Dubau F.Blancard C.2004-11-24T14:12:37Z2004-11-24T15:12:23ZCDS support team

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

cds-question@unistra.fratomic-physicsThe atomic data required to analyse low density coronal plasmas have been calculated and used to interpret X-ray spectra observed by the Flat Crystal Spectrometer of the SMM/NASA satellite in the 14-19 A wavelength range. The emission lines correspond mainly to Fe XVI, Fe XVII, Fe XVIII and some ones to O VII, O VIII.1994A&AS..105...77Chttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+AS/105/77CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+AS/105/77https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+AS/105/77http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+AS/105/77https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+AS/105/77https://vizier.iucaa.in/viz-bin/votable?-source=J/A+AS/105/77http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+AS/105/77GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+AS/105/77/table1Fe XVII energy levels and radiative transition probabilitiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIdidentification number corresponding to the following levelmeta.idintLevellevelphys.atmol.configurationEenergy levelcm**-1phys.energy;phys.atmol.levelintId.f1? final level of Ar1meta.idintnullableAr1? radiative transition probability (first of the two more important)s**-1phys.atmol.transProbdoublenullableId.f2? Final level of Ar2meta.idintnullableAr2? radiative transition probability (second of the two more important)s**-1phys.atmol.transProbdoublenullableSAr? Sum of all radiative probabilities from the level identified in the first two columnss**-1phys.atmol.transProbdoublenullableJ/A+AS/105/77/table2Fe XVII wavelengths and radiative transition probabilitiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintId1Upper level of transition (Id of table1)meta.idintId0Lower level of transition (Id of table1)meta.idintLambdaObsobserved wavelength from Phillips et al. (1982)0.1nmem.wlfloatLambda1observed wavelength from this work0.1nmem.wl.effectivefloatLambda2observed wavelength from Loulergue & Nussbaumer (1975)0.1nmem.wl.effectivefloatAr1radiative transition probability form this works**-1phys.atmol.transProbdoubleAr2radiative transition probability form Loulergue & Nussbaumer (1975)s**-1phys.atmol.transProbdoubleJ/A+AS/105/77/table3Fe XVII energy levelsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIdidentification number corresponding to the following levelmeta.idintLevellevelphys.atmol.configurationEenergy levelcm**-1phys.energy;phys.atmol.levelintId.f1? final level of Ar1meta.idintnullableAr1? radiative transition probability (first of the two more important)s**-1phys.atmol.transProbdoublenullableId.f2? Final level of Ar2meta.idintnullableAr2? radiative transition probability (second of the two more important)s**-1phys.atmol.transProbdoublenullableSAr? Sum of all radiative probabilities from the level identified in the first two columnss**-1phys.atmol.transProbdoublenullableJ/A+AS/105/77/table4Fe XVII fine structure collision strengthsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIdlevel identification number (from table1)meta.idintOmega70fine structure collision strength for an electron impact energy of 70 Ryphys.atmol.collStrengthdoubleOmega85fine structure collision strength for an electron impact energy of 85 Ryphys.atmol.collStrengthdoubleOmega200fine structure collision strength for an electron impact energy of 200 Ryphys.atmol.collStrengthdoubleOmega400fine structure collision strength for an electron impact energy of 400 Ryphys.atmol.collStrengthdoubleOmega600fine structure collision strength for an electron impact energy of 600 Ryphys.atmol.collStrengthdoubleOmega800fine structure collision strength for an electron impact energy of 800 Ryphys.atmol.collStrengthdoubleJ/A+AS/105/77/table5Fe XVI dielectronic satellite atomic datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTsautoionizing level s of the transition (s -> f)phys.atmol.configurationTffinal level f of the transition (s -> f)phys.atmol.configurationEsenergy of the corresponding captured electronRyphys.energy;phys.electronfloatlambdawavelength0.1nmem.wlfloatF*2(sf)Fe XVI dielectronic satellite atomic datas**-1phys.atmoldoublen_F*2(sf)relative importance of each F*2(sf) to this one of the strongest dielectronic line choosen as a reference linemeta.notefloatJ/A+AS/105/77/table6Fe XVI fine structure collision strengthsLevelexcited levelphys.atmol.configurationrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintOmega60fine structure collision strength for an electron impact energy of 60 Ryphys.atmol.collStrengthdoubleJ/A+AS/105/77/table7O VIII energy levels and radiative transition probabilitiesId.f2? Final level of Ar2meta.idintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIdidentification number corresponding to the following levelmeta.idintLevellevelphys.atmol.configurationEenergy levelcm**-1phys.energy;phys.atmol.levelintId.f1? final level of Ar1meta.idintnullableAr1? radiative transition probability (first of the two more important)s**-1phys.atmol.transProbdoublenullableAr2? radiative transition probability (second of the two more important)s**-1phys.atmol.transProbdoublenullableSAr? Sum of all radiative probabilities from the level identified in the first two columnss**-1phys.atmol.transProbdoublenullableJ/A+AS/105/77/table8O VIII fine structure collision strengthsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLevelexcited levelphys.atmol.configurationIdlevel identification number (see table7)meta.idintOmaga62fine structure collision strength for an electron impact energy of 62 Ryphys.atmol.collStrengthdoubleOmaga93fine structure collision strength for an electron impact energy of 93 Ryphys.atmol.collStrengthdoubleOmaga124fine structure collision strength for an electron impact energy of 124 Ryphys.atmol.collStrengthdoubleJ/A+AS/105/77/table9O VII dielectronic satellite atomic datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTsautoionizing level s of the transition (s -> f)phys.atmol.configurationTffinal level f of the transition (s -> f)phys.atmol.configurationEsenergy of the corresponding captured electronRyphys.energy;phys.electronfloatlambdawavelength0.1nmem.wlfloatF*2(sf)Fe XVI dielectronic satellite atomic datas**-1phys.atmoldoublen_F*2(sf)relative importance of each F*2(sf) to this one of the strongest dielectronic line choosen as a reference linemeta.notefloatJ/A+AS/105/77/table10aFe XVII line energy differential emissivity and relative differential emissivityIdentIdentificationmeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTransTransitionphys.atmol.configurationlambdawavelength0.1nmem.wlfloatEpsilon70line energy differential emissivity for an electron impact energy of 70 Ryph.s**-1.cm**-3phys.emissivitydoubleEpsilon85line energy differential emissivity for an electron impact energy of 85 Ryph.s**-1.cm**-3phys.emissivitydoubleEpsilon200line energy differential emissivity for an electron impact energy of 200 Ryph.s**-1.cm**-3phys.emissivitydoubleEpsilon400line energy differential emissivity for an electron impact energy of 400 Ryph.s**-1.cm**-3phys.emissivitydoubleEpsilon600line energy differential emissivity for an electron impact energy of 600 Ryph.s**-1.cm**-3phys.emissivitydoubleEpsilon800line energy differential emissivity for an electron impact energy of 800 Ryph.s**-1.cm**-3phys.emissivitydoubleDE70/E? relative energy differential emissivity for an electron impact energy of 70 Ryphys.atmol.collisionaldoublenullableDE85/E? relative energy differential emissivity for an electron impact energy of 85 Ryphys.atmol.collisionaldoublenullableDE200/E? relative energy differential emissivity for an electron impact energy of 200 Ryphys.atmol.collisionaldoublenullableDE400/E? relative energy differential emissivity for an electron impact energy of 400 Ryphys.atmol.collisionaldoublenullableDE600/E? relative energy differential emissivity for an electron impact energy of 600 Ryphys.atmol.collisionaldoublenullableDE800/E? relative energy differential emissivity for an electron impact energy of 800 Ryphys.atmol.collisionaldoublenullableJ/A+AS/105/77/table10bO VIII line energy differential emissivity and relative differential emissivityrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTransTransitionphys.atmol.configurationLambdawavelength0.1nmem.wlfloatEpsilon62? line energy differential emissivity for an electron impact energy of 62 Ryph.s**-1.cm**-3phys.emissivitydoublenullableEpsilon93? line energy differential emissivity for an electron impact energy of 93 Ryph.s**-1.cm**-3phys.emissivitydoublenullableEpsilon124? line energy differential emissivity for an electron impact energy of 124 Ryph.s**-1.cm**-3phys.emissivitydoublenullableDE62/E? relative energy differential emissivity for an electron impact energy of 62 Ryphys.atmol.collisionalfloatnullableDE93/E? relative energy differential emissivity for an electron impact energy of 93 Ryphys.atmol.collisionalfloatnullableDE124/E? relative energy differential emissivity for an electron impact energy of 124 Ryphys.atmol.collisionalfloatnullableJ/A+AS/105/77/table10cMost important Fe XVI inner-shell line energy differential emissivities and relative differential emissivityrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintTranstransitionphys.atmol.configurationLambdawavelength0.1nmem.wlfloatEpsilon60most important inner-shell line energy differential emissivity for an electron impact energy of 60 Ryph.s**-1.cm**-3phys.emissivitydoubleDE60/Emost important relative energy differential emissivity for an electron impact energy of 60 Ryphys.atmol.collisionalfloat