In t his paper , we segment t he sky area by bit2plane decomposition , and fit circadian light scat tering using elliptical least squares , which could automatically determine t he cent ral brightness of the sky. Then we weight t his cent ral brightness value wit h t he average bright ness value of the segmented sky region as t he final sky region brightness. Finally , we use t he fog atmosp heric scattering model to recover degraded images.

基于位平面分解的E_自动提取去雾算法.pdf

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