Hostname: page-component-745bb68f8f-s22k5 Total loading time: 0 Render date: 2025-01-12T20:55:15.977Z Has data issue: false hasContentIssue false
  • English
  • Français

Polarization Angle Swings Rediscussed

Published online by Cambridge University Press:  04 August 2017

W. Sieber
W. Sieber*
Affiliation:
Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-5300 Bonn 1, Federal Republic of Germany

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The polarization angle swing observed in some pulsars, e.g. PSR 0833-45, may be understood as the pattern which results when our line of sight cuts through the magnetic dipole field of a pulsar. In such a geometry the polarization angle χ is a function of μ, the angle between rotation axis and magnetic field axis and Δ, the angle between magnetic field and line of sight to the observer.

Type
I. Rotation-Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 57
Copyright
Copyright © Reidel 1987 

References

Backer, D.C., Rankin, J.M.: 1980, Astrophys. J. Suppl. 42, 143.Google Scholar
Bartel, N., Morris, D., Sieber, W. et al. 1982, Astrophys. J. 258, 776.CrossRefGoogle Scholar
Narayan, R., Vivekanand, M.: 1983. Astron. Astrophys. 122, 45.Google Scholar