1. RRI Digital Repository
  2. 04. Astronomy and Astrophysics
  3. Research Papers (A&A)
Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/6636
Full metadata record
DC FieldValueLanguage
dc.contributor.authorLoi, Shyeh Tjing-
dc.contributor.authorMurphy, Tara-
dc.contributor.authorDeshpande, A.A.-
dc.contributor.authorPrabu, T.-
dc.contributor.authorUdaya Shankar, N.-
dc.contributor.authorSrivani, K.S.-
dc.contributor.authorSubrahmanyan, Ravi-
dc.contributor.author+45 Co-authors-
dc.date.accessioned2017-03-14T13:45:00Z-
dc.date.available2017-03-14T13:45:00Z-
dc.date.issued2016-01-
dc.identifier.citationProceedings of a 1st URSI Atlantic Radio Science Conference (URSI AT-RASC 2015) meeting held 16-24 May 2015, Gran Canaria, Spain.en_US
dc.identifier.isbn9781479968718-
dc.identifier.urihttp://hdl.handle.net/2289/6636-
dc.descriptionRestricted Access.en_US
dc.description.abstractSummary form only given. Low-frequency, wide-field radio telescopes such as the Murchison Widefield Array (MWA) enable the dense spatial sampling of the ionosphere and plasmasphere on regional scales. For a physically compact array such as the MWA, the refractive shifts in the positions of celestial sources in the synthesised radio images are proportional to spatial gradients in the total electron content (TEC) transverse to the line of sight. By measuring the angular position shifts of celestial radio sources, one can probe waves and disturbances in the intervening plasma. Radio telescopes differ fundamentally from other techniques for measuring plasma fluctuations in that they are sensitive to TEC gradients/differences rather than absolute TEC. This makes them sensitive specifically to fluctuations about the ambient density, and therefore powerful probes of plasma density waves and irregularities. The authors present the results of an analysis of plasma fluctuations detected by the MWA, which can measure TEC gradients to a precision of ~1 mTECU/km at observing frequencies of ~150MHz. Around 2000-3000 point sources are visible instantaneously to the MWA, each functioning as a measurement point for the TEC gradient across the field-of-view (FoV). The spatial sampling completeness achieved by the MWA is unparalleled among interferometer observations of the ionosphere/plasmasphere to date, which have been limited both to smaller fields of view and at most several tens of measurement points (e.g. J. F. Helmboldt, W. M. Lane & W. D. Cotton, 2012, Radio Sci., 47, RS5008). This ~100-fold improvement in sampling completeness has permitted the first detailed imaging of the near-Earth plasma by a radio telescope.en_US
dc.language.isoenen_US
dc.publisherIEEEen_US
dc.relation.urihttp://dx.doi.org/10.1109/URSI-AT-RASC.2015.7303197en_US
dc.rights2016 Institute of Electrical and Electronics Engineers ( IEEE )en_US
dc.titleWaves in the sky: Probing the ionosphere with the Murchison widefield arrayen_US
dc.typeArticleen_US
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
2015_IeeeConProc_URSIA_.pdf
  Restricted Access		Restricted Access589.97 kBAdobe PDFView/Open Request a copy
Show simple item record


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.