Fine-resolution astronomical imaging with phase-diverse speckle

Details Fine-resolution astronomical imaging with phase-diverse speckle Fine-resolution astronomical imaging with phase-diverse speckle

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993spie.2029..287p&link_type=abstract

Proc. SPIE Vol. 2029, p. 287-298, Digital Image Recovery and Synthesis II, Paul S. Idell; Ed.

Physics

Optics

2

Scientific paper

Phase-diverse speckle imaging is a novel post-detection correction technique for use in imaging through atmospheric turbulence. When the wavelength dependence is introduced, the data-collection model and problem statement are seen to accommodate a variety of existing and proposed data-collection schemes, including speckle imaging, multi-frame blind deconvolution, deconvolution with wavefront sensing, and hybrid adaptive optics.

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