Partially redundant apertures for infrared stellar imaging
JOSA, Vol. 71, Issue 6, pp. 759-763 (1981)
http://dx.doi.org/10.1364/JOSA.71.000759
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Abstract
Spectral-bandwidth constraints to ensure controlled amounts of redundancy are established for a class of two-dimensional partially redundant arrays (PRA’s). In the IR, where speckle statistics are poor, the telescope-atmosphere modulation transfer function is determined solely by the PRA geometry. Signal-to-noise-ratio estimates, an optimum aperture criterion, and a six-element PRA example are presented.
© 1981 Optical Society of America
Citation
G. J. M. Aitken, J. P. Corteggiani, and J. Gay, "Partially redundant apertures for infrared stellar imaging," J. Opt. Soc. Am. 71, 759-763 (1981)
http://www.opticsinfobase.org/josa/abstract.cfm?URI=josa-71-6-759
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