J/A+A/482/989ivo://CDS.VizieR/J/A+A/482/989doi:10.26093/cds/vizier.34820989CDSStam D.M.2008-06-21T12:33:38Z2008-06-21T12:30:27ZCDS support team

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

cds-question@unistra.frsolar-system-planetsastronomical-modelspolarimetryWe present results of numerical simulations of flux F and degree of polarization P of light that is reflected by Earth-like extrasolar planets orbiting solar type stars. Our results are presented as functions of the wavelength (from 0.3 to 1.0{mu}m, with 0.001{mu}m spectral resolution) and as functions of the planetary phase angle. We use different surface coverages for our model planets, including vegetation and a Fresnel reflecting ocean, and clear and cloudy atmospheres.2008A&A...482..989Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/482/989CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/482/989https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/482/989http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/482/989https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/482/989https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/482/989http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/482/989GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/482/989/modelsResults of models for Lambertian, Forest and Ocean surfaceslambda[0.3,1.0] Wavelength (1)umem.wldoublea1Matrix element a1stat.paramdoubleb1Matrix element b1stat.paramdoublePolDegree of linear polarization (ratio -b1/a1)%phys.polarization.linearfloatPhase[0,180] Phase angle from 0 (full planet) to 180 (new planet)degsrc.orbitalintModelModel name (2)meta.id;stat.param;meta.modelledchar