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Curvature Radiation and Polarized Emission from PSR 2303+30

Published online by Cambridge University Press:  27 September 2017

J. A. Gil*
Affiliation:
Thp Astronomical Centre of Zielona Gòra and Institute of Physics, Pedagogical University

Abstract

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We present 430-M Hz Arecibo single pulse polarization measurements for PSR 2303+30. Single pulses typically consist of one or two subpulses. Each subpulse is associated with circular polarization which reverses sense near the subpulse peak and with its own swing of the position angle which does not coincide with the average position-angle curve. We attempt to explain these complicated characteristics within the framework of a coherent curvature radiation model of pulsar emission.

Type
Part IX Polarization phenomena
Copyright
Copyright © United States Naval Observatory 1992