Waves in the sky: Probing the ionosphere with the Murchison Widefield Array

© 2015 International Union of Radio Science (URSI). 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...

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Main Authors: Loi, S., Murphy, T., Cairns, I., Trott, Cathryn, Bell, M., Hurley-Walker, Natasha, Morgan, John, Lenc, E., Offringa, A., Menk, F., Waters, C., Feng, L., Hancock, Paul, Kaplan, D., Kudryavtseva, N., Lonsdale, C., Erickson, P., Coster, A., Ekers, R., Bernardi, G., Bowman, J., Briggs, F., Cappallo, R., Deshpande, A., Gaensler, B., Greenhill, L., Hazelton, B., Johnston-Hollitt, M., McWhirter, S., Mitchell, D., Morales, M., Morgan, E., Oberoi, D., Ord, S., Prabu, T., Shankar, N., Srivani, K., Subrahmanyan, R., Tingay, Steven, Wayth, Randall, Webster, R., Williams, Andrew, Williams, C.
Format: Conference Paper
Published: 2015
Online Access:http://hdl.handle.net/20.500.11937/17639
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author Loi, S.
Murphy, T.
Cairns, I.
Trott, Cathryn
Bell, M.
Hurley-Walker, Natasha
Morgan, John
Lenc, E.
Offringa, A.
Menk, F.
Waters, C.
Feng, L.
Hancock, Paul
Kaplan, D.
Kudryavtseva, N.
Lonsdale, C.
Erickson, P.
Coster, A.
Ekers, R.
Bernardi, G.
Bowman, J.
Briggs, F.
Cappallo, R.
Deshpande, A.
Gaensler, B.
Greenhill, L.
Hazelton, B.
Johnston-Hollitt, M.
McWhirter, S.
Mitchell, D.
Morales, M.
Morgan, E.
Oberoi, D.
Ord, S.
Prabu, T.
Shankar, N.
Srivani, K.
Subrahmanyan, R.
Tingay, Steven
Wayth, Randall
Webster, R.
Williams, Andrew
Williams, C.
author_facet Loi, S.
Murphy, T.
Cairns, I.
Trott, Cathryn
Bell, M.
Hurley-Walker, Natasha
Morgan, John
Lenc, E.
Offringa, A.
Menk, F.
Waters, C.
Feng, L.
Hancock, Paul
Kaplan, D.
Kudryavtseva, N.
Lonsdale, C.
Erickson, P.
Coster, A.
Ekers, R.
Bernardi, G.
Bowman, J.
Briggs, F.
Cappallo, R.
Deshpande, A.
Gaensler, B.
Greenhill, L.
Hazelton, B.
Johnston-Hollitt, M.
McWhirter, S.
Mitchell, D.
Morales, M.
Morgan, E.
Oberoi, D.
Ord, S.
Prabu, T.
Shankar, N.
Srivani, K.
Subrahmanyan, R.
Tingay, Steven
Wayth, Randall
Webster, R.
Williams, Andrew
Williams, C.
author_sort Loi, S.
building Curtin Institutional Repository
collection Online Access
description © 2015 International Union of Radio Science (URSI). 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.
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spelling curtin-20.500.11937-176392017-09-13T15:43:05Z Waves in the sky: Probing the ionosphere with the Murchison Widefield Array Loi, S. Murphy, T. Cairns, I. Trott, Cathryn Bell, M. Hurley-Walker, Natasha Morgan, John Lenc, E. Offringa, A. Menk, F. Waters, C. Feng, L. Hancock, Paul Kaplan, D. Kudryavtseva, N. Lonsdale, C. Erickson, P. Coster, A. Ekers, R. Bernardi, G. Bowman, J. Briggs, F. Cappallo, R. Deshpande, A. Gaensler, B. Greenhill, L. Hazelton, B. Johnston-Hollitt, M. McWhirter, S. Mitchell, D. Morales, M. Morgan, E. Oberoi, D. Ord, S. Prabu, T. Shankar, N. Srivani, K. Subrahmanyan, R. Tingay, Steven Wayth, Randall Webster, R. Williams, Andrew Williams, C. © 2015 International Union of Radio Science (URSI). 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. 2015 Conference Paper http://hdl.handle.net/20.500.11937/17639 10.1109/URSI-AT-RASC.2015.7303197 restricted
spellingShingle Loi, S.
Murphy, T.
Cairns, I.
Trott, Cathryn
Bell, M.
Hurley-Walker, Natasha
Morgan, John
Lenc, E.
Offringa, A.
Menk, F.
Waters, C.
Feng, L.
Hancock, Paul
Kaplan, D.
Kudryavtseva, N.
Lonsdale, C.
Erickson, P.
Coster, A.
Ekers, R.
Bernardi, G.
Bowman, J.
Briggs, F.
Cappallo, R.
Deshpande, A.
Gaensler, B.
Greenhill, L.
Hazelton, B.
Johnston-Hollitt, M.
McWhirter, S.
Mitchell, D.
Morales, M.
Morgan, E.
Oberoi, D.
Ord, S.
Prabu, T.
Shankar, N.
Srivani, K.
Subrahmanyan, R.
Tingay, Steven
Wayth, Randall
Webster, R.
Williams, Andrew
Williams, C.
Waves in the sky: Probing the ionosphere with the Murchison Widefield Array
title Waves in the sky: Probing the ionosphere with the Murchison Widefield Array
title_full Waves in the sky: Probing the ionosphere with the Murchison Widefield Array
title_fullStr Waves in the sky: Probing the ionosphere with the Murchison Widefield Array
title_full_unstemmed Waves in the sky: Probing the ionosphere with the Murchison Widefield Array
title_short Waves in the sky: Probing the ionosphere with the Murchison Widefield Array
title_sort waves in the sky: probing the ionosphere with the murchison widefield array
url http://hdl.handle.net/20.500.11937/17639