Interferometric imaging. II - Two-dimensional non-redundant arrays

Details Interferometric imaging. II - Two-dimensional non-redundant arrays Interferometric imaging. II - Two-dimensional non-redundant arrays

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..120..253z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 120, no. 2, 1989, p. 253-259.

Physics

1

Interferometry, Solar Instruments, Telescopes, Algorithms, Image Resolution, Masks

Scientific paper

Non-redundant arrays offer a promising technique for producing
diffraction-limited solar images. Pairs of two-dimensional nonredundant
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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