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    First Spectroscopic Imaging Observations of the Sun at Low Radio Frequencies with the Murchison Widefield Array Prototype

    249429_53574_Oberoietal2011_2041-8205_728_2_L27.pdf (2.123Mb)
    Access Status
    Open access
    Authors
    Oberoi, D.
    Matthews, L.
    Cairns, I.
    Emrich, David
    Lobzin, V.
    Lonsdale, C.
    Morgan, E.
    Prabu, T.
    Vedantham, H.
    Wayth, Randall
    Williams, A.
    Williams, C.
    White, S.
    Allen, G.
    Arcus, Wayne
    Barnes, D.
    Benkevitch, L.
    Bernardi, G.
    Bowman, J.
    Briggs, F.
    Bunton, J.
    Burns, S.
    Cappallo, R.
    Clark, M.
    Corey, B.
    Dawson, M.
    DeBoer, D.
    De Gans, A.
    DeSouza, L.
    Derome, M.
    Edgar, R.
    Elton, T.
    Goeke, R.
    Gopalakrishna, M.
    Greenhill, L.
    Hazelton, B.
    Herne, David
    Hewitt, J.
    Kamini, P.
    Kaplan, D.
    Kasper, J.
    Kennedy, R.
    Kincaid, B.
    Kocz, J.
    Koeing, R.
    Kowald, E.
    Lynch, Mervyn
    Madhavi, S.
    McWhirter, S.
    Mitchell, D.
    Morales, M.
    Ng, A.
    Ord, Stephen
    Pathikulangara, J.
    Rogers, A.
    Roshi, A.
    Salah, J.
    Sault, R.
    Schinckel, A.
    Udaya Shankar, N.
    Srivani, K.
    Stevens, J.
    Subrahmanyan, R.
    Thakkar, D.
    Tingay, Steven
    Tuthill, J.
    Vaccarella, A.
    Waterson, Mark
    Webster, R.
    Whitney, A.
    Date
    2011
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Oberoi, D. and Matthews, L. and Cairns, I. and Emrich, D. and Lobzin, V. and Lonsdale, C. and Morgan, E. et al. 2011. First Spectroscopic Imaging Observations of the Sun at Low Radio Frequencies with the Murchison Widefield Array Prototype. The Astrophysical Journal Letters. 728 (2): L27.
    Source Title
    The Astrophysical Journal Letters
    ISSN
    2041-8205
    School
    Curtin Institute of Radio Astronomy (Physics)
    URI
    http://hdl.handle.net/20.500.11937/49195
    Collection
    • Curtin Research Publications
    Abstract

    We present the first spectroscopic images of solar radio transients from the prototype for the Murchison Widefield Array, observed on 2010 March 27. Our observations span the instantaneous frequency band 170.9– 201.6 MHz. Though our observing period is characterized as a period of “low” to “medium” activity, one broadband emission feature and numerous short-lived, narrowband, non-thermal emission features are evident. Our data represent a significant advance in low radio frequency solar imaging, enabling us to follow the spatial, spectral, and temporal evolution of events simultaneously and in unprecedented detail. The rich variety of features seen here reaffirms the coronal diagnostic capability of low radio frequency emission and provides an early glimpse of the nature of radio observations that will become available as the next generation of low-frequency radio interferometers come online over the next few years.

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