The low-frequency profiles of some pulsars manifest temporal broadening due to scattering, usually accompanied by flat polarization position angle (PA) curves. Assuming that the scattering works on the 4 Stokes parameters in the same way, we have simulated the effect of scattering on polarization profiles and find that the scattering can indeed flatten the PA curves. Since the higher-frequency profiles suffer less from scattering, they are convolved with scattering models to fit the observed low-frequency profiles. The calculated flat PA curves exactly reproduce the corresponding observations.
CITATION STYLE
Li, X. H., & Han, J. L. (2003). The effect of scattering on pulsar polarization angle. Astronomy and Astrophysics, 410(1), 253–256. https://doi.org/10.1051/0004-6361:20031190
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