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Orthogonal Mode Polarization of Pulsar Radio Emission

Published online by Cambridge University Press:  19 July 2016

Q. Luo  and
D. B. Melrose
Q. Luo
Affiliation:
School of Physics, The University of Sydney, NSW 2006, Australia
D. B. Melrose
Affiliation:
School of Physics, The University of Sydney, NSW 2006, Australia

Abstract

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We discuss a model for polarization of pulsar radio emission, based on the assumption that waves propagate in two elliptically polarized natural modes. Some results from numerical simulation of single pulses are discussed with emphasis on circular polarization, microstructures and single pulse statistics.

Type
Part 8: Pulsar Electrodynamics and Emission Theory
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 381 - 382
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

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Melrose, D. B., & Luo, Q. 2004, MNRAS, submitted.Google Scholar