The murchison widefield array: Solar science with the low frequency SKA precursor

S. J. Tingay; D. Oberoi; I. Cairns; A. Donea; R. Duffin; W. Arcus; G. Bernardi; J. D. Bowman; F. Briggs; J. D. Bunton; R. J. Cappallo; B. E. Corey; A. Deshpande; L. Desouza; D. Emrich; B. M. Gaensler; R. Goeke; L. J. Greenhill; B. J. Hazelton; D. Herne; J. N. Hewitt; M. Johnston-Hollitt; D. L. Kaplan; J. C. Kasper; J. A. Kennewell; B. B. Kincaid; R. Koenig; E. Kratzenberg; C. J. Lonsdale; M. J. Lynch; S. R. McWhirter; D. A. Mitchell; M. F. Morales; E. Morgan; S. M. Ord; J. Pathikulangara; T. Prabu; R. A. Remillard; A. E.E. Rogers; A. Roshi; J. E. Salah; R. J. Sault; N. Udaya-Shankar; K. S. Srivani; J. Stevens; R. Subrahmanyan; M. Waterson; R. B. Wayth; R. L. Webster; A. R. Whitney; A. Williams; C. L. Williams; J. S.B. Wyithe

doi:10.1088/1742-6596/440/1/012033

The murchison widefield array: Solar science with the low frequency SKA precursor

S. J. Tingay, D. Oberoi, I. Cairns, A. Donea, R. Duffin, W. Arcus, G. Bernardi, J. D. Bowman, F. Briggs, J. D. Bunton, R. J. Cappallo, B. E. Corey, A. Deshpande, L. Desouza, D. Emrich, B. M. Gaensler, R. Goeke, L. J. Greenhill, B. J. Hazelton, D. HerneJ. N. Hewitt, M. Johnston-Hollitt, D. L. Kaplan, J. C. Kasper, J. A. Kennewell, B. B. Kincaid, R. Koenig, E. Kratzenberg, C. J. Lonsdale, M. J. Lynch, S. R. McWhirter, D. A. Mitchell, M. F. Morales, E. Morgan, S. M. Ord, J. Pathikulangara, T. Prabu, R. A. Remillard, A. E.E. Rogers, A. Roshi, J. E. Salah, R. J. Sault, N. Udaya-Shankar, K. S. Srivani, J. Stevens, R. Subrahmanyan, M. Waterson, R. B. Wayth, R. L. Webster, A. R. Whitney, A. Williams, C. L. Williams, J. S.B. Wyithe

Research output: Contribution to journal › Conference article › peer-review

21 Citations (Scopus)

Abstract

The Murchison Widefield Array is a low frequency (80-300 MHz) SKA Precursor, comprising 128 aperture array elements (known as tiles) distributed over an area of 3 km diameter. The MWA is located at the extraordinarily radio quiet Murchison Radioastronomy Observatory in the mid-west of Western Australia, the selected home for the Phase 1 and Phase 2 SKA low frequency arrays. The MWA science goals include: 1) detection of fluctuations in the brightness temperature of the diffuse redshifted 21 cm line of neutral hydrogen from the epoch of reionisation; 2) studies of Galactic and extragalactic processes based on deep, confusion-limited surveys of the full sky visible to the array; 3) time domain astrophysics through exploration of the variable radio sky; and 4) solar imaging and characterisation of the heliosphere and ionosphere via propagation effects on background radio source emission. This paper concentrates on the capabilities of the MWA for solar science and summarises some of the solar science results to date, in advance of the initial operation of the final instrument in 2013.

Original language	English
Article number	012033
Journal	Journal of Physics: Conference Series
Volume	440
Issue number	1
DOIs	https://doi.org/10.1088/1742-6596/440/1/012033
Publication status	Published - 2013
Event	Eclipse on the Coral Sea: Cycle 24 Ascending - Palm Cove, QLD, Australia Duration: 12 Nov 2012 → 16 Nov 2012

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10.1088/1742-6596/440/1/012033

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Tingay, S. J., Oberoi, D., Cairns, I., Donea, A., Duffin, R., Arcus, W., Bernardi, G., Bowman, J. D., Briggs, F., Bunton, J. D., Cappallo, R. J., Corey, B. E., Deshpande, A., Desouza, L., Emrich, D., Gaensler, B. M., Goeke, R., Greenhill, L. J., Hazelton, B. J., ... Wyithe, J. S. B. (2013). The murchison widefield array: Solar science with the low frequency SKA precursor. Journal of Physics: Conference Series, 440(1), Article 012033. https://doi.org/10.1088/1742-6596/440/1/012033

@article{274d6b9712eb44d987e8f2025fb73cf5,

title = "The murchison widefield array: Solar science with the low frequency SKA precursor",

abstract = "The Murchison Widefield Array is a low frequency (80-300 MHz) SKA Precursor, comprising 128 aperture array elements (known as tiles) distributed over an area of 3 km diameter. The MWA is located at the extraordinarily radio quiet Murchison Radioastronomy Observatory in the mid-west of Western Australia, the selected home for the Phase 1 and Phase 2 SKA low frequency arrays. The MWA science goals include: 1) detection of fluctuations in the brightness temperature of the diffuse redshifted 21 cm line of neutral hydrogen from the epoch of reionisation; 2) studies of Galactic and extragalactic processes based on deep, confusion-limited surveys of the full sky visible to the array; 3) time domain astrophysics through exploration of the variable radio sky; and 4) solar imaging and characterisation of the heliosphere and ionosphere via propagation effects on background radio source emission. This paper concentrates on the capabilities of the MWA for solar science and summarises some of the solar science results to date, in advance of the initial operation of the final instrument in 2013.",

author = "Tingay, {S. J.} and D. Oberoi and I. Cairns and A. Donea and R. Duffin and W. Arcus and G. Bernardi and Bowman, {J. D.} and F. Briggs and Bunton, {J. D.} and Cappallo, {R. J.} and Corey, {B. E.} and A. Deshpande and L. Desouza and D. Emrich and Gaensler, {B. M.} and R. Goeke and Greenhill, {L. J.} and Hazelton, {B. J.} and D. Herne and Hewitt, {J. N.} and M. Johnston-Hollitt and Kaplan, {D. L.} and Kasper, {J. C.} and Kennewell, {J. A.} and Kincaid, {B. B.} and R. Koenig and E. Kratzenberg and Lonsdale, {C. J.} and Lynch, {M. J.} and McWhirter, {S. R.} and Mitchell, {D. A.} and Morales, {M. F.} and E. Morgan and Ord, {S. M.} and J. Pathikulangara and T. Prabu and Remillard, {R. A.} and Rogers, {A. E.E.} and A. Roshi and Salah, {J. E.} and Sault, {R. J.} and N. Udaya-Shankar and Srivani, {K. S.} and J. Stevens and R. Subrahmanyan and M. Waterson and Wayth, {R. B.} and Webster, {R. L.} and Whitney, {A. R.} and A. Williams and Williams, {C. L.} and Wyithe, {J. S.B.}",

year = "2013",

doi = "10.1088/1742-6596/440/1/012033",

language = "English",

volume = "440",

journal = "Journal of Physics: Conference Series",

issn = "1742-6588",

publisher = "IOP Publishing Ltd.",

number = "1",

note = "Eclipse on the Coral Sea: Cycle 24 Ascending ; Conference date: 12-11-2012 Through 16-11-2012",

}

Tingay, SJ, Oberoi, D, Cairns, I, Donea, A, Duffin, R, Arcus, W, Bernardi, G, Bowman, JD, Briggs, F, Bunton, JD, Cappallo, RJ, Corey, BE, Deshpande, A, Desouza, L, Emrich, D, Gaensler, BM, Goeke, R, Greenhill, LJ, Hazelton, BJ, Herne, D, Hewitt, JN, Johnston-Hollitt, M, Kaplan, DL, Kasper, JC, Kennewell, JA, Kincaid, BB, Koenig, R, Kratzenberg, E, Lonsdale, CJ, Lynch, MJ, McWhirter, SR, Mitchell, DA, Morales, MF, Morgan, E, Ord, SM, Pathikulangara, J, Prabu, T, Remillard, RA, Rogers, AEE, Roshi, A, Salah, JE, Sault, RJ, Udaya-Shankar, N, Srivani, KS, Stevens, J, Subrahmanyan, R, Waterson, M, Wayth, RB, Webster, RL, Whitney, AR, Williams, A, Williams, CL & Wyithe, JSB 2013, 'The murchison widefield array: Solar science with the low frequency SKA precursor', Journal of Physics: Conference Series, vol. 440, no. 1, 012033. https://doi.org/10.1088/1742-6596/440/1/012033

TY - JOUR

T1 - The murchison widefield array

T2 - Eclipse on the Coral Sea: Cycle 24 Ascending

AU - Tingay, S. J.

AU - Oberoi, D.

AU - Cairns, I.

AU - Donea, A.

AU - Duffin, R.

AU - Arcus, W.

AU - Bernardi, G.

AU - Bowman, J. D.

AU - Briggs, F.

AU - Bunton, J. D.

AU - Cappallo, R. J.

AU - Corey, B. E.

AU - Deshpande, A.

AU - Desouza, L.

AU - Emrich, D.

AU - Gaensler, B. M.

AU - Goeke, R.

AU - Greenhill, L. J.

AU - Hazelton, B. J.

AU - Herne, D.

AU - Hewitt, J. N.

AU - Johnston-Hollitt, M.

AU - Kaplan, D. L.

AU - Kasper, J. C.

AU - Kennewell, J. A.

AU - Kincaid, B. B.

AU - Koenig, R.

AU - Kratzenberg, E.

AU - Lonsdale, C. J.

AU - Lynch, M. J.

AU - McWhirter, S. R.

AU - Mitchell, D. A.

AU - Morales, M. F.

AU - Morgan, E.

AU - Ord, S. M.

AU - Pathikulangara, J.

AU - Prabu, T.

AU - Remillard, R. A.

AU - Rogers, A. E.E.

AU - Roshi, A.

AU - Salah, J. E.

AU - Sault, R. J.

AU - Udaya-Shankar, N.

AU - Srivani, K. S.

AU - Stevens, J.

AU - Subrahmanyan, R.

AU - Waterson, M.

AU - Wayth, R. B.

AU - Webster, R. L.

AU - Whitney, A. R.

AU - Williams, A.

AU - Williams, C. L.

AU - Wyithe, J. S.B.

PY - 2013

Y1 - 2013

N2 - The Murchison Widefield Array is a low frequency (80-300 MHz) SKA Precursor, comprising 128 aperture array elements (known as tiles) distributed over an area of 3 km diameter. The MWA is located at the extraordinarily radio quiet Murchison Radioastronomy Observatory in the mid-west of Western Australia, the selected home for the Phase 1 and Phase 2 SKA low frequency arrays. The MWA science goals include: 1) detection of fluctuations in the brightness temperature of the diffuse redshifted 21 cm line of neutral hydrogen from the epoch of reionisation; 2) studies of Galactic and extragalactic processes based on deep, confusion-limited surveys of the full sky visible to the array; 3) time domain astrophysics through exploration of the variable radio sky; and 4) solar imaging and characterisation of the heliosphere and ionosphere via propagation effects on background radio source emission. This paper concentrates on the capabilities of the MWA for solar science and summarises some of the solar science results to date, in advance of the initial operation of the final instrument in 2013.

AB - The Murchison Widefield Array is a low frequency (80-300 MHz) SKA Precursor, comprising 128 aperture array elements (known as tiles) distributed over an area of 3 km diameter. The MWA is located at the extraordinarily radio quiet Murchison Radioastronomy Observatory in the mid-west of Western Australia, the selected home for the Phase 1 and Phase 2 SKA low frequency arrays. The MWA science goals include: 1) detection of fluctuations in the brightness temperature of the diffuse redshifted 21 cm line of neutral hydrogen from the epoch of reionisation; 2) studies of Galactic and extragalactic processes based on deep, confusion-limited surveys of the full sky visible to the array; 3) time domain astrophysics through exploration of the variable radio sky; and 4) solar imaging and characterisation of the heliosphere and ionosphere via propagation effects on background radio source emission. This paper concentrates on the capabilities of the MWA for solar science and summarises some of the solar science results to date, in advance of the initial operation of the final instrument in 2013.

UR - http://www.scopus.com/inward/record.url?scp=84880282392&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/440/1/012033

DO - 10.1088/1742-6596/440/1/012033

M3 - Conference article

AN - SCOPUS:84880282392

SN - 1742-6588

VL - 440

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

IS - 1

M1 - 012033

Y2 - 12 November 2012 through 16 November 2012

ER -

The murchison widefield array: Solar science with the low frequency SKA precursor

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