A mode-coupling model reproduces the qualitative frequency-dependent circular polarization of selected FAST single pulses, but its Bayesian parameter constraints are undermined by the model's poor fits to most pulses.
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2 Pith papers cite this work, alongside 356 external citations. Polarity classification is still indexing.
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Pulsar radio emission beams from the two poles are generally dissimilar in azimuth width and often radius, based on rotating vector model fits to polarization data from eight double-pole interpulse pulsars.
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Pulsar electrodynamics inferred from frequency-dependent circular polarization diversity
A mode-coupling model reproduces the qualitative frequency-dependent circular polarization of selected FAST single pulses, but its Bayesian parameter constraints are undermined by the model's poor fits to most pulses.
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On the Difference Between Pulsar Radio Emission Beams from the Two Poles
Pulsar radio emission beams from the two poles are generally dissimilar in azimuth width and often radius, based on rotating vector model fits to polarization data from eight double-pole interpulse pulsars.