Abstract
Large multi-aperture interferometers are expected to provide snap-shot images with milli- to nano-arcsecond resolution, directly at the combined focus. This requires a densified exit pupil and phased beams for all the wavelengths used. The wave analysis methods serving for adaptive optics in monolithic telescopes being inadequate for diluted apertures, we have developed a different phasing algorithm. It involves a hierarchy of aperture triplets and uses image sharpness criteria. Numerical simulations on unresolved and resolved objects show that a single iteration is generally sufficient. On wavelength-dependant objects, the proper position indexing of the monochromatic image components appears also efficiently achievable.
Original language | English |
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Pages (from-to) | 543-551 |
Number of pages | 9 |
Journal | Astronomy and Astrophysics Supplement Series |
Volume | 137 |
Issue number | 3 |
DOIs | |
Publication status | Published - 2 Jun 1999 |
Keywords
- INSTRUMENTATION: INTERFEROMETERS, METHODS: NUMERICAL, TECHNIQUES: IMAGE PROCESSING, TECHNIQUES: INTERFEROMETRIC, TELESCOPES