Proc. IAU volume 13, issue S337, P404-405 2017 DOI: 10.1017/s1743921317009486 View full text
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Joanna M. Rankin

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.