Pupil configuration optimality criterion in synthetic aperture optics

Details Pupil configuration optimality criterion in synthetic aperture optics Pupil configuration optimality criterion in synthetic aperture optics

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995spie.2477..124m&link_type=abstract

Proc. SPIE Vol. 2477, p. 124-131, Spaceborne Interferometry II, Robert D. Reasenberg; Ed.

Physics

1

Scientific paper

This paper addresses the optimization of the relative arrangement (pupil configuration) of a phased array of optical telescopes, coherently combined to form images of extended objects in a common focal plane. A new optimality criterion, which is directly linked to the restoration error of the original object from the recorded image, is derived. The optimal configuration is a function of the maximum frequency of interest (or sought resolution), and takes into account the diameter of the elementary telescopes. Simulations illustrate the usefulness of this criterion for designing a synthetic aperture optical instrument.

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