J/A+A/491/561ivo://CDS.VizieR/J/A+A/491/561doi:10.26093/cds/vizier.34910561CDSDere K.P.2009-01-02T09:16:50Z2009-01-02T10:11:54ZCDS support team

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

cds-question@unistra.frthe-sunWe determine the volumetric plasma filling factor of coronal bright points. Rastered spectra of the regions of the quiet Sun were recorded by the Extreme ultraviolet Imaging Spectrometer (EIS) during operations with the Hinode satellite. Calibrated intensities of Fe XII lines were obtained and images of the quiet corona were constructed. From the imaged spectra, the emission measures and geometrical widths of coronal bright points were obtained. Electron densities were determined from density-sensitive line ratios. A comparison of the emission measure and bright point widths with the electron densities yielded the plasma-filling factor.2008A&A...491..561Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/491/561CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/491/561https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/491/561http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/491/561https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/491/561https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/491/561http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/491/561GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/491/561/table2Observed and derived properties of a set of coronal bright pointsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintLabelBright point labelmeta.id;meta.maincharRasterRaster labelmeta.idcharIntBright point intensitymW.m**-2.sr**-1spect.line.intensitydoubleLogNeLog (decimal) of the electron densitycm**-3phys.density;phys.electronfloatWidthObserved bright point widtharcsecphys.angSize;srcfloatFillFactorVolumetric plasma filling factorstat.fit.paramdouble