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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astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
High-resolution FAST data reveal spike subpulses (strongly polarized, marginally resolved) in 21 pulsars and quasi-periodic subpulses (periods ~0.1-1 ms) in 13 pulsars, with checks for rotation period correlation.
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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FAST Pulsar Database IV. Spike subpulses and quasi-periodic subpulses of 25 pulsars observed by FAST
High-resolution FAST data reveal spike subpulses (strongly polarized, marginally resolved) in 21 pulsars and quasi-periodic subpulses (periods ~0.1-1 ms) in 13 pulsars, with checks for rotation period correlation.