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    Evaluating Receiver Noise Temperature of a Radio Telescope in the Presence of Mutual Coupling: Comparison of Current Methodologies

    76396.pdf (266.0Kb)
    Access Status
    Open access
    Authors
    Ung, Daniel
    Sutinjo, Adrian
    Davidson, D.
    Date
    2019
    Type
    Conference Paper
    
    Metadata
    Show full item record
    Citation
    Ung, D. and Sutinjo, A. and Davidson, D. 2019. Evaluating Receiver Noise Temperature of a Radio Telescope in the Presence of Mutual Coupling: Comparison of Current Methodologies. In 13th European Conference on Antennas and Propagation, Krakow, Poland, 31 Mar-5 Apr 2019.
    Source Title
    13th European Conference on Antennas and Propagation, EuCAP
    Additional URLs
    https://ieeexplore.ieee.org/abstract/document/8739942
    ISBN
    9788890701887
    Faculty
    Faculty of Science and Engineering
    School
    School of Elec Eng, Comp and Math Sci (EECMS)
    Remarks

    © 2019 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/20.500.11937/76135
    Collection
    • Curtin Research Publications
    Abstract

    © 2019 European Association on Antennas and Propagation. We present the computation of receiver noise temperature which includes the effects of mutual coupling of two different radio telescopes deployed in the Murchison Radio-astronomy Observatory, namely the Murchison Widefield Array and the prototype Engineering Development Array. We used three different formulations that only require information of measured noise parameters of the low noise amplifier as used in the radio telescope and simulated S-parameter of the array to perform the calculation. In addition, we show convergence in computed receiver noise temperature for various pointing angles and array configurations (uniform and pseudo-random) that indicate agreement with existing literature.

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