Polarization of pulsar radiation in the two-pole caustic model and in the outer gap model
arXiv:astro-ph/0403428
Abstract
We present linear polarization characteristics of pulsar radiation as predicted by two models of high-energy radiation from extended regions in the outer magnetosphere: the recently proposed two-pole caustic model, and the outer gap model.
11 pages, 7 figures, poster presented at the X-ray Polarimetry Workshop, SLAC, Stanford, California, 9 - 11 February 2004