Properties of Intrinsic Polarization Angle Ambiguities in Faraday Tomography
arXiv:1402.0612 · doi:10.1093/pasj/psu030
Abstract
Faraday tomography is a powerful method to diagnose polarizations and Faraday rotations along the line of sight. The quality of Faraday tomography is, however, limited by several conditions. Recently, it is reported that Faraday tomography indicates false signals in some specific situations. In this paper, we systematically investigate the condition of the appearance of false signals in Faraday tomography. We study this by pseudo-observing two sources within a beam, and change in the intrinsic polarization angles, rotation measures, intensities, and frequency coverage. We find that false signals arise when rotation measure between the sources is less than 1.5 times the full width at half maximum of the rotation measure spread function. False signals also depend on the intensity ratio between the sources and are reduced for large ratio. On the other hand, the appearance of false signals does not depend on frequency coverage, meaning that the uncertainty should be correctly understood and taken into consideration even with future wide-band observations such as Square Kilometer Array (SKA).
21 pages, 10 figures, accepted for publication in PASJ
References in corpus (6)
- Lower Bounds on Magnetic Fields in Intergalactic Voids from Long-Term GeV-TeV Light Curves of the Blazar Mrk 421
- Dynamo activities driven by magneto-rotational instability and Parker instability in galactic gaseous disk
- Fisher Analysis on Wide-Band Polarimetry for Probing the Intergalactic Magnetic Field
- N-body + Magnetohydrodynamical Simulations of Merging Clusters of Galaxies: Characteristic Magnetic Field Structures Generated by Bulk Flow Motion
- Stability Analysis for Cosmic-Ray Heating of Cool Cores in Galaxy Clusters
- MUSIC for Faraday Rotation Measure Synthesis
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