Parallel blind deconvolution applied to solar image
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Two parallel blind deconvolution methods, each of which uses multiple frames or several images segmented from a single frame, were applied to solar images to reconstruct their fine structure. The influence of low-contrast intensity distribution on the solar images on their reconstruction was investigated with computer simulations. The methods are also applied to an observed solar image.
Key wordsblind deconvolution image reconstruction solar image atmosperic turbulence frame segmentation stellar speckle interferometry
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