摘要
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.
| 源语言 | English |
|---|---|
| 页(从-至) | 543-551 |
| 期刊 | Astronomy & Astrophysics Supplement |
| 卷 | 137 |
| 出版状态 | Published - 1 6月 1999 |
学术指纹
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