Paper
23 August 2005 Phase diverse wavefront estimation and image restoration with a magnification change between imaging channels
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Abstract
Ideally phase diversity determines the object and wavefront that are consistent with two images taken identically except that the wavefront of the diversity channel is perturbed by a known additive aberration. In practice other differences may occur such as image rotation, magnification, changes in detector response, and non-common image motion. This paper develops a mathematical forward model for addressing magnification changes and a corresponding maximumlikelihood implementation of phase diversity. Performance using this physically correct forward model is compared with the more simple approach of resampling the data of the diversity channel.
© (2005) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Carlos Luna, David R. Gerwe, and Brandoch Calef "Phase diverse wavefront estimation and image restoration with a magnification change between imaging channels", Proc. SPIE 5896, Unconventional Imaging, 58960H (23 August 2005); https://doi.org/10.1117/12.614465
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Cited by 1 scholarly publication.
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KEYWORDS
Staring arrays

Sensors

Wavefronts

Image processing

Point spread functions

Data modeling

Telescopes

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