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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2 Pith papers cite this work. Polarity classification is still indexing.
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Wave mode coupling reproduces diverse frequency evolutions of circular polarization in pulsar single pulses, constraining multiplicity to 1-100 and Lorentz factor to 3-100, though the model fails to quantitatively fit most observed spectra.
citing papers explorer
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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.
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On the Diversity of Pulsar's Frequency-Dependent Circular Polarization
Wave mode coupling reproduces diverse frequency evolutions of circular polarization in pulsar single pulses, constraining multiplicity to 1-100 and Lorentz factor to 3-100, though the model fails to quantitatively fit most observed spectra.