Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4942
Title: Modeling of polarization of radio pulsars
Authors: Gangadhara, R. T
Keywords: Modeling of Polarization;Radio Pulsars;Low-Frequency Radio Universe
Issue Date: Sep-2009
Publisher: Astronomical Society of the Pacific
Citation: Saikia, D. J.,Green, D. A., Gupta, Y and Venturi, T., eds The Low-Frequency Radio Universe ASP Conference Series, Vol. 407, proceedings of the conference held 8 - 12 December 2008, at National Centre for Radio Astrophysics (NCRA), TIFR, Pune, India. pp. 328 – 332
Abstract: We have generalized the coherent curvature radiation model to include the detailed geometry of the emission region in pulsar magnetosphere, and deduced the polarization state in terms the Stokes parameters. By considering uniform and modulated emissions, we have simulated the profiles. The model predicts that the circular polarization of antisymmetric type is an intrinsic property of curvature radiation, and it survives only when there is modulation or discrete distribution in the emitting sources. Our model predicts a correlation between the polarization angle swing and sign reversal of circular polarization.
Description: Restricted Access
URI: http://hdl.handle.net/2248/4942
ISBN: 978-1-58381-694-3
???metadata.dc.rights???: © Astronomical Society of the Pacific
???metadata.dc.relation.uri???: http://www.aspbooks.org/a/volumes/article_details/?paper_id=30346
Appears in Collections:IIAP Publications

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