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A Proposed Correlator Back-End ror the Culgoora Radioheliograph

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Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 76))

Abstract

The original design of the Culgoora radioheliograph (Wild, 1967; Sheridan et al., 1973) incorporated a number of features, such as high time resolution and limited declination coverage, which were particularly suited to its primary function of observing the Sun. Although some of these features are disadvantageous for cosmic work, the instrument has nevertheless proved useful for a variety of non-solar studies as well.

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© 1979 D. Reidel Publishing Company

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McLean, D.J. (1979). A Proposed Correlator Back-End ror the Culgoora Radioheliograph. In: Van Schooneveld, C. (eds) Image Formation from Coherence Functions in Astronomy. Astrophysics and Space Science Library, vol 76. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-9449-2_18

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  • DOI: https://doi.org/10.1007/978-94-009-9449-2_18

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-9451-5

  • Online ISBN: 978-94-009-9449-2

  • eBook Packages: Springer Book Archive

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