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dc.contributor.authorLoi, S.
dc.contributor.authorCairns, I.
dc.contributor.authorMurphy, T.
dc.contributor.authorErickson, P.
dc.contributor.authorBell, M.
dc.contributor.authorRowlinson, A.
dc.contributor.authorArora, Balwinder Singh
dc.contributor.authorMorgan, John
dc.contributor.authorEkers, Ronald
dc.contributor.authorHurley-Walker, Natasha
dc.contributor.authorKaplan, D.
dc.date.accessioned2017-01-30T12:36:21Z
dc.date.available2017-01-30T12:36:21Z
dc.date.created2016-03-14T19:30:24Z
dc.date.issued2016
dc.identifier.citationLoi, S. and Cairns, I. and Murphy, T. and Erickson, P. and Bell, M. and Rowlinson, A. and Arora, B. et al. 2016. Density duct formation in the wake of a travelling ionospheric disturbance: Murchison Widefield Array observations. Journal of Geophysical Research: Space Physics. 121 (2): pp. 1569-1586.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/23256
dc.identifier.doi10.1002/2015JA022052
dc.description.abstract

©2016. American Geophysical Union. Geomagnetically aligned density structures with a range of sizes exist in the near-Earth plasma environment, including 10-100 km wide VLF/HF wave-ducting structures. Their small diameters and modest density enhancements make them difficult to observe, and there is limited evidence for any of the several formation mechanisms proposed to date. We present a case study of an event on 26 August 2014 where a travelling ionospheric disturbance (TID) shortly precedes the formation of a complex collection of field-aligned ducts, using data obtained by the Murchison Widefield Array (MWA) radio telescope. Their spatiotemporal proximity leads us to suggest a causal interpretation. Geomagnetic conditions were quiet at the time, and no obvious triggers were noted. Growth of the structures proceeds rapidly, within 0.5 h of the passage of the TID, attaining their peak prominence 1-2 h later and persisting for several more hours until observations ended at local dawn. Analyses of the next 2 days show field-aligned structures to be preferentially detectable under quiet rather than active geomagnetic conditions. We used a raster scanning strategy facilitated by the speed of electronic beamforming to expand the quasi-instantaneous field of view of the MWA by a factor of 3. These observations represent the broadest angular coverage of the ionosphere by a radio telescope to date.

dc.publisherWiley-Blackwell Publishing
dc.titleDensity duct formation in the wake of a travelling ionospheric disturbance: Murchison Widefield Array observations
dc.typeJournal Article
dcterms.source.issn2169-9380
dcterms.source.titleJournal of Geophysical Research: Space Physics
curtin.note

Copyright © 2016 The American Geophysical Union

curtin.departmentCurtin Institute of Radio Astronomy (Engineering)
curtin.accessStatusOpen access


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