Expand this Topic clickable element to expand a topic
Skip to content
Optica Publishing Group

Multiframe iterative blind deconvolution using only a positivity constraint

Not Accessible

Your library or personal account may give you access

Abstract

The problem of blind deconvolution, extracting both the original image and point spread function (PSF) from only the measurement of their convolution, may at first seem a futile task. However Lane and Bates [1] have shown via separation of zero sheets that blind deconvolution is theoretically possible for dimensions of two or greater when very little noise is present. In practice noise is a significant problem that limits the ability to perform successful deconvolution. Many researchers have also found that the only way of achieving blind deconvolution is to impose spatial and spectral constraints on the solution, derived from a priori information about the imaging system, and to eliminate the trivial solution of the image or PSF being a delta function. This becomes less useful in situations where very little else is known except the measured data.

© 1998 Optical Society of America

PDF Article
More Like This
Regularized blind deconvolution

R.G. Lane, R. A. Johnston, R. Irwan, and T.J. Connolly
STuA.2 Signal Recovery and Synthesis (SRS) 1998

Astronomical Results using Physically-Constrained Iterative Deconvolution

E. K. Hege, M. Cheselka, M. Lloyd-Hart, P. Hinz, W.F. Hoffmann, J.C. Christou, and S.M. Jefferies
STuB.3 Signal Recovery and Synthesis (SRS) 1998

Multiframe Blind Deconvolution for Object and PSF Recovery for Astronomical Imaging

Julian C. Christou, E. Keith Hege, and Stuart M. Jefferies
RWA2 Signal Recovery and Synthesis (SRS) 1995

Select as filters


Select Topics Cancel
© Copyright 2024 | Optica Publishing Group. All rights reserved, including rights for text and data mining and training of artificial technologies or similar technologies.