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    Power spectrum analysis of ionospheric fluctuations with the Murchison Widefield Array

    232254_232254.pdf (2.771Mb)
    Access Status
    Open access
    Authors
    Loi, S.
    Trott, Cathryn
    Murphy, T.
    Cairns, I.
    Bell, M.
    Hurley-Walker, Natasha
    Morgan, John
    Lenc, E.
    Offringa, A.
    Feng, L.
    Hancock, P.
    Kaplan, D.
    Kudryavtseva, N.
    Bernardi, G.
    Bowman, J.
    Briggs, F.
    Cappallo, R.
    Corey, B.
    Deshpande, A.
    Emrich, D.
    Gaensler, B.
    Goeke, R.
    Greenhill, L.
    Hazelton, B.
    Johnston-Hollitt, M.
    Kasper, J.
    Kratzenberg, E.
    Lonsdale, C.
    Lynch, Mervyn
    Mcwhirter, S.
    Mitchell, D.
    Morales, M.
    Morgan, E.
    Oberoi, D.
    Ord, S.
    Prabu, T.
    Rogers, A.
    Roshi, A.
    Shankar, N.
    Srivani, K.
    Subrahmanyan, R.
    Tingay, Steven
    Waterson, M.
    Wayth, Randall
    Webster, R.
    Whitney, A.
    Williams, A.
    Williams, C.
    Date
    2015
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Loi, S. and Trott, C. and Murphy, T. and Cairns, I. and Bell, M. and Hurley-Walker, N. and Morgan, J. et al. 2015. Power spectrum analysis of ionospheric fluctuations with the Murchison Widefield Array. Radio Science. 50 (7): pp. 574-597.
    Source Title
    Radio Science
    DOI
    10.1002/2015RS005711
    ISSN
    0048-6604
    School
    Curtin Institute of Radio Astronomy (Physics)
    Funding and Sponsorship
    http://purl.org/au-research/grants/arc/DE140100316
    Remarks

    An edited version of this paper was published by AGU. Copyright 2015 American Geophysical Union

    URI
    http://hdl.handle.net/20.500.11937/5549
    Collection
    • Curtin Research Publications
    Abstract

    Low-frequency, wide field-of-view (FOV) radio telescopes such as the Murchison Widefield Array (MWA) enable the ionosphere to be sampled at high spatial completeness. We present the results of the first power spectrum analysis of ionospheric fluctuations in MWA data, where we examined the position offsets of radio sources appearing in two data sets. The refractive shifts in the positions of celestial sources are proportional to spatial gradients in the electron column density transverse to the line of sight. These can be used to probe plasma structures and waves in the ionosphere. The regional (10–100 km) scales probed by the MWA, determined by the size of its FOV and the spatial density of radio sources (typically thousands in a single FOV), complement the global (100–1000 km) scales of GPS studies and local (0.01–1 km) scales of radar scattering measurements. Our data exhibit a range of complex structures and waves. Some fluctuations have the characteristics of traveling ionospheric disturbances, while others take the form of narrow, slowly drifting bands aligned along the Earth's magnetic field.

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