Centrifugal Acceleration in Pulsar Magnetospheres

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3570

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DC Field	Value	Language
dc.contributor.author	Thomas, R. M. C	-
dc.contributor.author	Gangadhara, R. T	-
dc.date.accessioned	2008-09-12T10:32:11Z	-
dc.date.available	2008-09-12T10:32:11Z	-
dc.date.issued	2004	-
dc.identifier.citation	IAU Symposium, No. 218, pp. 375 - 376	en
dc.identifier.issn	0074-1809	-
dc.identifier.uri	http://hdl.handle.net/2248/3570	-
dc.description.abstract	We present a relativistic model of pulsar radio emission by plasma accelerated along the rotating magnetic field lines projected on to a 2D plane perpendicular to the rotation axis. We have derived the expression for the trajectory of a particle, and estimated the spectrum of radio emission by the plasma bunches. We used the parameters given by Peyman &Gangadhara (2002). The analytical expressions for the Stokes parameters are obtained, and their values compared with the observed profiles. The one sense of circular polarization, observed in many pulsars, can be explained in light of our model.	en
dc.language.iso	en	en
dc.publisher	International Astronomical Union	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/0310486	en
dc.subject	Centrifugal Acceleration	en
dc.subject	Pulsar Magnetospheres	en
dc.title	Centrifugal Acceleration in Pulsar Magnetospheres	en
dc.type	Article	en
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