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Proceedings Paper

Fine-resolution astronomical imaging with phase-diverse speckle
Author(s): Richard G. Paxman; John H. Seldin
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Paper Abstract

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.

Paper Details

Date Published: 9 November 1993
PDF: 12 pages
Proc. SPIE 2029, Digital Image Recovery and Synthesis II, (9 November 1993); doi: 10.1117/12.162007
Show Author Affiliations
Richard G. Paxman, Environmental Research Institute of Michigan (United States)
John H. Seldin, Environmental Research Institute of Michigan (United States)


Published in SPIE Proceedings Vol. 2029:
Digital Image Recovery and Synthesis II
Paul S. Idell, Editor(s)

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