Volume 421, Number 2, July II 2004
|Page(s)||681 - 691|
|Section||Stellar structure and evolution|
|Published online||22 June 2004|
Ellipticity and deviations from orthogonality in the polarization modes of PSR B0329+54*
Astronomical Institute “Anton Pannekoek”, University of Amsterdam, Kruislaan 403, 1098 SJ Amsterdam, The Netherlands
2 Stichting ASTRON, Postbus 2, 7990 AA Dwingeloo, The Netherlands
Corresponding author: R. T. Edwards, firstname.lastname@example.org
Accepted: 26 March 2004
We report on an analysis of the polarization of single pulses of PSR B0329+54 at 328 MHz. We find that the distribution of polarization orientations in the central component diverges strongly from the standard picture of orthogonal polarization modes (OPMs), making a remarkable partial annulus on the Poincaré sphere. A second, tightly clustered region of density appears in the opposite hemisphere, at a point antipodal to the centre of the annulus. We argue that this can be understood in terms of birefringent alterations in the relative phase of two elliptically polarized propagation modes in the pulsar magnetosphere (i.e. generalised Faraday rotation). The ellipticity of the modes implies a significant charge density in the plasma, while the presence of both senses of circular polarization, and the fact that only one mode shows the effect, supports the view that refracted ordinary-mode rays are involved in the production of the annulus. At other pulse longitudes the polarization (including the circular component) is broadly consistent with an origin in elliptical OPMs, shown here quantitatively for the first time, however considerable non-orthogonal contributions serve to broaden the orientation distribution in an isotropic manner.
Key words: plasmas / polarization / stars: pulsars: individual: PSR B0329+54 / waves
© ESO, 2004
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