Circular polarization in radio pulsar PSR B1451-68: coherent mode transitions and intrabeam interference
J. Dyks, P. Weltevrede, C. Ilie

TL;DR
This paper investigates the polarization properties of pulsar PSR B1451-68, revealing that coherent mode transitions and interference patterns explain observed polarization behaviors and profile features.
Contribution
It introduces the concept of coherent OPM transitions (COMTs) and demonstrates their role in circular polarization and profile minima, advancing understanding of pulsar polarization mechanisms.
Findings
Coherent mode transitions cause circular polarization and profile minima.
Interference of orthogonal modes explains polarization enhancements.
Frequency-dependent superposition produces apparent pulse components.
Abstract
The radio emission of pulsar B1451-68 contains two polarization modes of similar strength, which produce two clear orthogonal polarization angle tracks. When viewed on a Poincare sphere, the emission is composed of two flux patches that rotate meridionally as function of pulse longitude and pass through the Stokes V poles, which results in transitions between orthogonal polarization modes (OPMs). Moreover, the ratio of power in the patches is inversed once within the profile window. It is shown that the meridional circularization is caused by a coherent OPM transition (COMT) produced by a varying mode ratio at a fixed quarter-wave phase lag. The COMTs may be ubiquitous and difficult to detect in radio pulsar data, because they can leave no trace in polarized fractions and they are described by equation similar to the rotating vector model. The circularization, which coincides with flux…
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