Radio Emission by Particles Accelerated in Pulsar Magnetosphere

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2420

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DC Field	Value	Language
dc.contributor.author	Thomas, R. M. C	-
dc.contributor.author	Gangadhara, R. T	-
dc.date.accessioned	2008-06-06T09:37:43Z	-
dc.date.available	2008-06-06T09:37:43Z	-
dc.date.issued	2003	-
dc.identifier.citation	BASI, Vol. 31, No. 3&4, pp. 361 - 362	en
dc.identifier.uri	http://hdl.handle.net/2248/2420	-
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 in the paper by Peyman and Gangadhara (2002). Further the analystical expressions for the Stokes parameters are derived, and compared them with the observed profiles. The one sense of circular polarization, observed in many pulsars, can be explained in the light of our model.	en
dc.format.extent	55044 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2003BASI...31..361T	en
dc.subject	Pulsar	en
dc.subject	Emission mechanism	en
dc.title	Radio Emission by Particles Accelerated in Pulsar Magnetosphere	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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