Litcius/Paper detail

Single pulse polarization study of pulsars B0950 + 08 and B1642 − 03: micropulse properties and mixing of orthogonal modes

Shubham Singh, Yashwant Gupta, Kishalay De

2023Monthly Notices of the Royal Astronomical Society12 citationsDOIOpen Access PDF

Abstract

ABSTRACT We present the results of a high-time resolution polarization study of single pulses from pulsars B0950 + 08 and B1642 − 03. Single pulses from pulsar B0950 + 08 sometimes show isolated micropulses without any significant associated subpulse emission. Assuming that the properties of such micropulses represent the intrinsic nature of micropulse emission, we characterize the width and polarization properties of these ‘intrinsic’ microstructures. Most of the ‘intrinsic’ micropulses ($\sim 90~{{\ \rm per\ cent}}$) follow common characteristic polarization properties, while the average width of these micropulses is consistent with the general micropulse population from this pulsar. Single pulses from these pulsars show a diverse range of polarization properties, including depolarization and mixing of two orthogonal modes resulting in polarization position angle jumps. We present a superposition model of the two orthogonal modes which can explain depolarization, the observed position angle jumps, and associated changes in other polarization parameters.

Topics & Concepts

PulsarPhysicsPolarization (electrochemistry)Superposition principleOpticsPosition angleAstrophysicsOrthogonal polarization spectral imagingDegree of polarizationLinear polarizationPopulationDepolarizationComputational physicsLaserScatteringSociologyEndocrinologyQuantum mechanicsGalaxyDemographyMedicineChemistryPhysical chemistryHigh-pressure geophysics and materialsPulsars and Gravitational Waves ResearchAcoustic Wave Resonator Technologies
Single pulse polarization study of pulsars B0950 + 08 and B1642 − 03: micropulse properties and mixing of orthogonal modes | Litcius