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Referencing the Polarization Orientation to the Emission-Region Magnetic Field
Published online by Cambridge University Press: 04 June 2018
Abstract
Using the proper-motion as a proxy for a pulsar’s rotation-axis orientation, the emission polarization can be related to the magnetic field direction in the emission region, providing a much more physical foundation for understanding orthogonal mode radiation.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 13 , Symposium S337: Pulsar Astrophysics the Next Fifty Years , September 2017 , pp. 404 - 405
- Copyright
- Copyright © International Astronomical Union 2018