Estimating Solar Flux Density at Low Radio Frequencies Using a Sky Brightness Model
Estimating Solar Flux Density at Low Radio Frequencies Using a Sky Brightness Model
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Dordrecht: Springer Netherlands
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English
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Dordrecht: Springer Netherlands
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Sky models have been used in the past to calibrate individual low radio frequency telescopes. In this article we generalize this approach from a single antenna to a two element interferometer, and formulate the problem in a way that allows us to estimate the flux density of the Sun using the normalized cross-correlations (visibilities) measured on...
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Full title
Estimating Solar Flux Density at Low Radio Frequencies Using a Sky Brightness Model
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TN_cdi_proquest_journals_1903799891
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_1903799891
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ISSN
0038-0938
E-ISSN
1573-093X
DOI
10.1007/s11207-017-1096-1
