Radio Emission by Particles Accelerated in Pulsar Magnetosphere

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