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. 2018 Feb 1;18(2):190–206. doi: 10.1089/ast.2017.1686

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© Michael A. Famiano et al., 2018; Published by Mary Ann Liebert, Inc.

This Open Access article is distributed under the terms of theCreative Commons Attribution Noncommercial License (http://creativecommons.org/licenses/by-nc/4.0/) which permits any noncommercialuse, distribution, and reproduction in any medium, provided the original author(s) and the source are credited.

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FIG. 3. — Polarization distribution for three example models. This figure compares the polarization distribution for various neutron star surface magnetic fields (Famiano et al., 2014; Famiano and Boyd, 2016).