Feature visibility limits in the non-linear enhancement of turbid images

被引:4
|
作者
Jobson, DJ [1 ]
Rahman, ZU [1 ]
Woodell, GA [1 ]
机构
[1] NASA, Langley Res Ctr, Hampton, VA 23681 USA
来源
关键词
D O I
10.1117/12.488842
中图分类号
TP31 [计算机软件];
学科分类号
081202 ; 0835 ;
摘要
The advancement of non-linear processing methods for generic automatic clarification of turbid imagery has led us from extensions of entirely passive multiscale Retinex processing to a new framework of active measurement and control of the enhancement process called the Visual Servo. In the process of testing this new non-linear computational scheme, we have identified that feature visibility limits in the post-enhancement image now simplify to a single signal-to-noise figure of merit: a feature is visible if the feature-background signal difference is greater than the RMS noise level. In other words, a signal-to-noise limit of approximately unity constitutes a lower limit on feature visibility.
引用
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页码:24 / 30
页数:7
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