J/ApJS/169/439ivo://CDS.VizieR/J/ApJS/169/439doi:10.26093/cds/vizier.21690439CDSSocas-Navarro H.2017-07-11T13:08:13Z2009-06-04T13:55:10ZCDS support team

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

cds-question@unistra.frastronomical-modelsstellar-atmospheresthe-sunmagnetic-fieldsThis paper presents semiempirical models of various solar magnetic structures, extending from the photosphere to the chromosphere. The models have been derived from non-LTE inversions of high-resolution spectropolarimetric observations of four CaII and FeI lines. The observed targets are dark and bright components of a sunspot umbra; dark and bright components of a sunspot penumbra; a canopy between two sunspots; a facula; and a network element. These models may be employed, e.g., to compute realistic synthetic Stokes spectra of photospheric and chromospheric lines.2007ApJS..169..439Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/169/439CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/374/265 : LTE spectrum synthesis in magnetic atmospheres (Wade+, 2001)J/A+AS/110/329 : LTE model atmospheres coeff. (Diaz-cordoves+, 1995)J/A+A/274/555 : Asymmetry of FeI lines in solar spectrum (Stathopoulou+ 1993)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/169/439https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/169/439http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/169/439https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/169/439https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/169/439http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/169/439GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/ApJS/169/439/modelsCombined table from original tablesPelElectron pressure (dPa = dyn/cm^2^)dPaphys.pressuredoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMModel, with stray light fraction: A=0.06, B=0.05, C=0.23, D=2.27, E=0.43, F=0.55, G=0.29meta.id;stat.fitcharlog.tauLog of the optical depth at 500nmphys.absorption.opticalDepthfloatzHeight above surface (tau=1)kmsrc.redshiftdoubleTempTemperatureKphys.temperaturefloatDenDensityg.cm**-3phys.densitydoublePgasGas pressure (dPa = dyn/cm^2^)dPaphys.pressuredoubleVelLine-of-sight velocity (1)cm/sspect.dopplerVeloc;pos.heliocentricdoubleBfieldMagnetic field (in Gauss)0.0001Tphys.magFielddoubleIncInclinationdegsrc.orbital.inclinationdouble