Paper
25 October 1996 Signal-to-noise and convergence properties of a modified Richardson-Lucy algorithm with Knox-Thompson start point
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Abstract
The utility of a blind deconvolution algorithm used in conjunction with the Knox-Thompson algorithm is demonstrated with day time observations of the MIR space station. We also investigate the convergence properties of the Richardson- Lucy Blind deconvolution algorithm when used in conjunction with the Knox-Thompson algorithm.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David Charles Dayton, Steven C. Sandven, and John D. Gonglewski "Signal-to-noise and convergence properties of a modified Richardson-Lucy algorithm with Knox-Thompson start point", Proc. SPIE 2827, Digital Image Recovery and Synthesis III, (25 October 1996); https://doi.org/10.1117/12.255079
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CITATIONS
Cited by 3 scholarly publications.
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KEYWORDS
Reconstruction algorithms

Deconvolution

Signal to noise ratio

Speckle

Point spread functions

Space telescopes

Fourier transforms

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