Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2974
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dc.contributor.authorNagendra, K. N-
dc.date.accessioned2008-08-01T06:01:55Z-
dc.date.available2008-08-01T06:01:55Z-
dc.date.issued1996-03-
dc.identifier.citationSolar Physics, Vol. 164, No. 1 - 2, pp. 67 - 78en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/2974-
dc.descriptionRestricted Access-
dc.description.abstractVelocity fields in line formation regions strongly affect the line polarization. The conventionally used observer's frame method of solving the polarized transfer equation becomes expensive and inaccurate for partial redistribution problems, when large amplitude velocity fields have to be considered in the observer's frame. An alternative method of solution is the comoving frame method. Partial redistribution problems are solved using comoving frame formalism for line polarization caused by resonance scattering.en
dc.format.extent3894 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherSpringeren
dc.subjectLine Polarizationen
dc.subjectRadiative transferen
dc.subjectComoving frame methoden
dc.titlePartial redistribution effects on line polarization in the presence of velocity fieldsen
dc.typeArticleen
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