Power spectrum analysis of ionospheric fluctuations with the Murchison Widefield Array

Low‐frequency, wide field‐of‐view (FOV) radio telescopes such as the Murchison Widefield Array (MWA) enable the ionosphere to be sampled at high spatial completeness. We present the results of the first power spectrum analysis of ionospheric fluctuations in MWA data, where we examined the position o...

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Veröffentlicht in:	Radio science 2015-07, Vol.50 (7), p.574-597
Hauptverfasser:	Loi, Shyeh Tjing, Trott, Cathryn M., Murphy, Tara, Cairns, Iver H., Bell, Martin, Hurley-Walker, Natasha, Morgan, John, Lenc, Emil, Offringa, A. R., Feng, L., Hancock, P. J., Kaplan, D. L., Kudryavtseva, N., Bernardi, G., Bowman, J. D., Briggs, F., Cappallo, R. J., Corey, B. E., Deshpande, A. A., Emrich, D., Gaensler, B. M., Goeke, R., Greenhill, L. J., Hazelton, B. J., Johnston-Hollitt, M., Kasper, J. C., Kratzenberg, E., Lonsdale, C. J., Lynch, M. J., McWhirter, S. R., Mitchell, D. A., Morales, M. F., Morgan, E., Oberoi, D., Ord, S. M., Prabu, T., Rogers, A. E. E., Roshi, A., Shankar, N. Udaya, Srivani, K. S., Subrahmanyan, R., Tingay, S. J., Waterson, M., Wayth, R. B., Webster, R. L., Whitney, A. R., Williams, A., Williams, C. L.
Format:	Artikel
Sprache:	eng
Schlagworte:	Arrays Completeness Density Earth science Fluctuation Ionosphere Ionospherics Magnetic fields Murchison Widefield Array power spectrum Radio Radio telescopes Spectrum analysis
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