Answers are grounded in this paper and cite their sources.
We present mean pulse profiles and polarization parameters at frequencies near 660 and 1440 MHz for 29 and 40 pulsars respectively, with some pulsars being observed at both frequencies. Measurements of Faraday rotation for 48 pulsars are also presented. The observations were made during 1990 with the Parkes radio telescope using filterbank polarimeter systems. Implications of the results for pulsar emission mechanisms and the Galactic magnetic field are briefly discussed.
No takes yet. Share an insight, caveat, or question.
Manchester et al. (1995) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: