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Interferometric imaging II:

Two-dimensional non-redundant arrays

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Abstract

Non-redundant arrays offer a promising technique for producing diffraction-limited solar images. Pairs of two-dimensional non-redundant arrays yield sufficient information to recover the phases of all the spatial frequencies to which they respond. The algorithms to select and test such pairs are given and applied to a particular example.

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Authors and Affiliations

  1. National Optical Astronomy Observatories, National Solar Observatory/SP, 88349, Sunspot, NM, U.S.A.

    J. B. Zirker

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  1. J. B. Zirker
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Operated by the Association of Universities for Research in Astronomy, Inc., under contract with the National Science Foundation.

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Zirker, J.B. Interferometric imaging II:. Sol Phys 120, 253–259 (1989). https://doi.org/10.1007/BF00159879

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  • DOI: https://doi.org/10.1007/BF00159879

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