Answers are grounded in this paper and cite their sources.
Mean pulse profiles and polarization parameters at 435, 660 or 1500 MHz obtained using the ATNF Parkes radio telescope are presented for 66 southern pulsars. About half of these pulsars were discovered in the Parkes southern pulsar survey and most have no previously published polarization parameters. Where possible, beam impact parameters and inclination angles are computed assuming a circular beam geometry and the rotating-vector model. Implications of the results for models of the pulse emission mechanism are briefly discussed.
No takes yet. Share an insight, caveat, or question.
Manchester et al. (1998) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: