1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1743
Full metadata record
DC FieldValueLanguage
dc.contributor.authorNagendra, K. N-
dc.contributor.authorPeraiah, A-
dc.date.accessioned2007-07-27T04:56:36Z-
dc.date.available2007-07-27T04:56:36Z-
dc.date.issued1984-09-
dc.identifier.citationAstrophysics & Space Science, Vol. 104, pp. 61-72en
dc.identifier.urihttp://hdl.handle.net/2248/1743-
dc.description.abstractA numerical solution is presented for the problem of continuum radiative transfer in a magnetoactive medium. The continuum opacities are calculated in the presence of a strong magnetic field (H = 10 MG) typical of magnetic white dwarfs. The LTE pure-absorption model is assumed for calculating the polarized radiation field emitted by a realistic model atmosphere in the plane-parallel approximation. The wavelength dependences of the linear and circular polarizations are calculated for both uniform and dipole field configurationsen
dc.format.extent749968 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1984Ap%26SS.104...61Nen
dc.subjectStellar modulesen
dc.subjectPolarized radationen
dc.titlePolarization of continuum radiation in magnetic atmospheresen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Nagendra.pdf732.39 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.