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Title: The Statistics of Radio Astronomical Polarimetry: Disjoint, Superposed, and Composite Samples

Abstract

A statistical framework is presented for the study of the orthogonally polarized modes of radio pulsar emission via the covariances between the Stokes parameters. To accommodate the typically heavy-tailed distributions of single-pulse radio flux density, the fourth-order joint cumulants of the electric field are used to describe the superposition of modes with arbitrary probability distributions. The framework is used to consider the distinction between superposed and disjoint modes, with particular attention to the effects of integration over finite samples. If the interval over which the polarization state is estimated is longer than the timescale for switching between two or more disjoint modes of emission, then the modes are unresolved by the instrument. The resulting composite sample mean exhibits properties that have been attributed to mode superposition, such as depolarization. Because the distinction between disjoint modes and a composite sample of unresolved disjoint modes depends on the temporal resolution of the observing instrumentation, the arguments in favor of superposed modes of pulsar emission are revisited, and observational evidence for disjoint modes is described. In principle, the four-dimensional covariance matrix that describes the distribution of sample mean Stokes parameters can be used to distinguish between disjoint modes, superposed modes, and a compositemore » sample of unresolved disjoint modes. More comprehensive and conclusive interpretation of the covariance matrix requires more detailed consideration of various relevant phenomena, including temporally correlated subpulse modulation (e.g., jitter), statistical dependence between modes (e.g., covariant intensities and partial coherence), and multipath propagation effects (e.g., scintillation and scattering).« less

Authors:
 [1];  [2]
  1. Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Hawthorn, VIC 3122 (Australia)
  2. Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn (Germany)
Publication Date:
OSTI Identifier:
22663964
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal; Journal Volume: 835; Journal Issue: 2; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; DATA ANALYSIS; DEPOLARIZATION; DISTRIBUTION; ELECTRIC FIELDS; EMISSION; FLUX DENSITY; FOUR-DIMENSIONAL CALCULATIONS; POLARIMETRY; POLARIZATION; PROBABILITY; PULSARS; RESOLUTION; SCATTERING; SCINTILLATIONS; STATISTICS; STOKES PARAMETERS

Citation Formats

Straten, W. van, and Tiburzi, C., E-mail: willem.van.straten@aut.ac.nz. The Statistics of Radio Astronomical Polarimetry: Disjoint, Superposed, and Composite Samples. United States: N. p., 2017. Web. doi:10.3847/1538-4357/835/2/293.
Straten, W. van, & Tiburzi, C., E-mail: willem.van.straten@aut.ac.nz. The Statistics of Radio Astronomical Polarimetry: Disjoint, Superposed, and Composite Samples. United States. doi:10.3847/1538-4357/835/2/293.
Straten, W. van, and Tiburzi, C., E-mail: willem.van.straten@aut.ac.nz. Wed . "The Statistics of Radio Astronomical Polarimetry: Disjoint, Superposed, and Composite Samples". United States. doi:10.3847/1538-4357/835/2/293.
@article{osti_22663964,
title = {The Statistics of Radio Astronomical Polarimetry: Disjoint, Superposed, and Composite Samples},
author = {Straten, W. van and Tiburzi, C., E-mail: willem.van.straten@aut.ac.nz},
abstractNote = {A statistical framework is presented for the study of the orthogonally polarized modes of radio pulsar emission via the covariances between the Stokes parameters. To accommodate the typically heavy-tailed distributions of single-pulse radio flux density, the fourth-order joint cumulants of the electric field are used to describe the superposition of modes with arbitrary probability distributions. The framework is used to consider the distinction between superposed and disjoint modes, with particular attention to the effects of integration over finite samples. If the interval over which the polarization state is estimated is longer than the timescale for switching between two or more disjoint modes of emission, then the modes are unresolved by the instrument. The resulting composite sample mean exhibits properties that have been attributed to mode superposition, such as depolarization. Because the distinction between disjoint modes and a composite sample of unresolved disjoint modes depends on the temporal resolution of the observing instrumentation, the arguments in favor of superposed modes of pulsar emission are revisited, and observational evidence for disjoint modes is described. In principle, the four-dimensional covariance matrix that describes the distribution of sample mean Stokes parameters can be used to distinguish between disjoint modes, superposed modes, and a composite sample of unresolved disjoint modes. More comprehensive and conclusive interpretation of the covariance matrix requires more detailed consideration of various relevant phenomena, including temporally correlated subpulse modulation (e.g., jitter), statistical dependence between modes (e.g., covariant intensities and partial coherence), and multipath propagation effects (e.g., scintillation and scattering).},
doi = {10.3847/1538-4357/835/2/293},
journal = {Astrophysical Journal},
number = 2,
volume = 835,
place = {United States},
year = {Wed Feb 01 00:00:00 EST 2017},
month = {Wed Feb 01 00:00:00 EST 2017}
}
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