Polarization position angles of repeating FRBs are Gaussian distributed with no periodicity, arising from geometric projection in a stochastically varying magnetosphere that also explains non-repeating FRBs.
The time-averaged properties of the observed pulsar population
2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 2years
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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.
citing papers explorer
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Random Polarization Position Angle Behaviors across Bursts of Repeating Fast Radio Bursts
Polarization position angles of repeating FRBs are Gaussian distributed with no periodicity, arising from geometric projection in a stochastically varying magnetosphere that also explains non-repeating FRBs.
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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.