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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4612
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dc.contributor.authorThomas, R. M. C-
dc.contributor.authorGangadhara, R. T-
dc.date.accessioned2009-07-02T13:35:34Z-
dc.date.available2009-07-02T13:35:34Z-
dc.date.issued2008-
dc.identifier.citationHasan, S. S., Gangadhara, R. T. and Krishan, V. eds., Turbulence, dynamos, accretion disks, pulsars and collective plasma processes, First Kodai-Trieste workshop on plasma astrophysics held at the Kodaikanal Observatory., Astrophysics and space science proceedings., Kodaikanal., India, 2007., pp. 177 – 187en
dc.identifier.isbn978-1-4020-8867-4-
dc.identifier.urihttp://hdl.handle.net/2248/4612-
dc.descriptionRestricted Access-
dc.descriptionThe original publication is available at springerlink.com-
dc.description.abstractWe consider the coherent curvature radiation by relativistic plasma in pulsar magnetosphere. The radiation emitted by relativistic particle bunches is beamed in the direction of field line tangents. For the first time, we have derived analytical expressions for the Stokes parameters of the coherent curvature emission, taking the detailed geometry into account. The emissions from individual bunches are incoherently superposed to find the net emission within the solid angle of radius 1/γ (beaming region) around the line of sight. By taking into account of the viewing geometry, we have estimated the polarization state of the emitted radiation.en
dc.language.isoenen
dc.publisherSpringer Netherlandsen
dc.relation.urihttp://dx.doi.org/10.1007/978-1-4020-8868-1_12en
dc.relation.urihttp://adsabs.harvard.edu/abs/2008tdad.conf..177Ten
dc.rights© Springeren
dc.subjectAstrophysical Turbulenceen
dc.subjectPulsarsen
dc.subjectDynamosen
dc.subjectSolar and Space Plasmasen
dc.subjectPolarizationen
dc.subjectCoherent Curvature Radiationen
dc.titlePolarization of coherent curvature radiation in pulsarsen
dc.typeArticleen
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