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Postion angle jumps in pulsar linear polarization

Published online by Cambridge University Press:  12 April 2016

R.X. Xu ,
G.J. Qiao  and
J.L. Han
R.X. Xu
Affiliation:
Department of Geophysics, Peking University, Beijing 100871, China
G.J. Qiao
Affiliation:
Department of Geophysics, Peking University, Beijing 100871, China
J.L. Han
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100080, China

Abstract

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The position angle (PA) behaviour of linear polarization of pulsar emission is simulated after considering the relative retardation between the core and conal components, which are believed to be generated from different emission altitudes. The PA will jump 90° at some points where the complete depolarization occurs.

Type
Part 4 Radio Properties
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 261 - 262
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Lyne, A.G., Manchester, R.N., 1988, MNRAS 234, 477.CrossRefGoogle Scholar
Qiao, G.J., 1988, Vistas in Astronomy 31, 393.Google Scholar
Qiao, G.J., 1992, Proc. IAU Collo. 128, p419.Google Scholar
Qiao, G.J., Li, C.G., Li, M., 1992, Proc. IAU Collo. 128, p242.Google Scholar
Qiao, G.J., Manchester, R.N., Lyne, A.G., Gould, D.M., 1995, MNRAS 274, 572 Google Scholar
Radhakrishnan, V., Cooke, D.J., 1969, Ap. Let. 3, 225.Google Scholar
Rankin, J.M., 1983, ApJ 274, 333.Google Scholar
Rankin, J.M., 1988, ApJ 325, 314.CrossRefGoogle Scholar
Wu, X.J., Manchester, R.N., Lyne, A.G., Qiao, G.J., 1993, MNRAS 261, 630.Google Scholar