Manifestations of propagation effects in the individual pulse polarization of radio pulsars

Details Manifestations of propagation effects in the individual pulse polarization of radio pulsars Manifestations of propagation effects in the individual pulse polarization of radio pulsars

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..801..282p&link_type=abstract

ASTROPHYSICAL SOURCES OF HIGH ENERGY PARTICLES AND RADIATION. AIP Conference Proceedings, Volume 801, pp. 282-285 (2005).

Astronomy and Astrophysics

Astrophysics

1

Pulsars, Polarisation, Astrophysical Plasma, Stellar Atmospheres, Pulsars, Magnetic And Electric Fields, Polarization Of Starlight, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

Polarization transfer in the plasma of pulsar magnetosphere is considered. It is shown that as the two natural waves of orthogonal linear polarization pass through the regions of mode coupling and cyclotron resonance, they become elliptical and non-orthogonal. Formation of pulsar polarization as a result of propagation effects implies a correlation between the ellipticity and position angle of the waves, which is proved by observations. Propagation model of pulsar polarization provides a unique possibility of diagnostics of pulsar plasma.

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