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    Improving the Murchison Widefield Array tile model for polarimetry

    202774_202774.pdf (636.3Kb)
    Access Status
    Open access
    Authors
    Sutinjo, Adrian
    Padhi, Shantanu
    Wayth, Randall
    Hall, Peter
    Tingay, Steven
    O’Sullivan, J.
    Lenc, E.
    Date
    2014
    Type
    Conference Paper
    
    Metadata
    Show full item record
    Citation
    Sutinjo, A. and Padhi, S. and Wayth, R. and Hall, P. and Tingay, S. and O’Sullivan, J. and Lenc, E. 2014. Improving the Murchison Widefield Array tile model for polarimetry, in Proceedings of 16th International Symposium on Antenna Technology and Applied Electromagnetics (ANTEM 2014), Jul 13 2014, pp. 1-2. Victoria, BC; Canada: IEEE Computer Society.
    Source Title
    International Symposium on Antenna Technology and Applied Electromagnetics
    Source Conference
    Proceedings - ANTEM 2014: 2014 16th International Symposium on Antenna Technology and Applied Electromagnetics
    DOI
    10.1109/ANTEM.2014.6887732
    ISBN
    978-147992225-3
    School
    Curtin Institute of Radio Astronomy
    Remarks

    Copyright © 2014 IEEE. Personal use of this material is permitted. Permission from IEEE must be obtained for all other uses, in any current or future media, including reprinting/republishing this material for advertising or promotional purposes, creating new collective works, for resale or redistribution to servers or lists, or reuse of any copyrighted component of this work in other works.

    URI
    http://hdl.handle.net/20.500.11937/29327
    Collection
    • Curtin Research Publications
    Abstract

    This paper summarizes the progress to date in improving the Murchison Widefield Array’s (MWA) “tile” model for polarimetry. A simple model that accounts for inter-element mutual coupling is presented which explains the false polarization leakage in Stokes Q (“false Q”) seen when the array is scanned away from zenith in the principal planes. On these planes the model predicts current imbalance in the X (E-W) and Y (N-S) dipoles and hence the false Q. More sophisticated models intended to calibrate actual observation data will be briefly discussed.

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