Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1790
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dc.contributor.authorMohan Rao, D-
dc.contributor.authorRangarajan, K. E-
dc.contributor.authorAbhyankar, K. D-
dc.date.accessioned2007-09-14T09:15:52Z-
dc.date.available2007-09-14T09:15:52Z-
dc.date.issued1995-
dc.identifier.citationBASI, Vol. 23, No. 2, pp. 211-225en
dc.identifier.urihttp://hdl.handle.net/2248/1790-
dc.description.abstractWe consider non-conservative Rayleigh scattering in finite atmospheres and study the polarization in the molecular lines both in the transmitted and reflected sunlight. We first investigate the parameterized models to estimate the effects of optical thickness, line strength, continuous absorption etc. on line polarization. This study helped us to analyse some typical O2 and H20 band lines in the earth's atmosphere. For the chosen parameters, we find that the polarization is more sensitive to optical thickness than the line strength. The continuous absorption affects the wing polarization selectively.en
dc.format.extent818003 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1995BASI...23..211Men
dc.subjectpolarizationen
dc.subjectearth's atmosphereen
dc.subjecttelluric linesen
dc.titleNon-conservative Rayleigh scattering in a finite atmosphere - II. Polarization in telluric linesen
dc.typeArticleen
Appears in Collections:BASI Publications

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