Speckle Noise Removal by Energy Models with New Regularization Setting

Figure 11

Numerical result of the “peppers” image with noise standard deviation ; (a) restored image by the ROF model; (b) restored image by the ATV model; (c) restored image by the JIN’s model; (d) restored image by HYPTV model; (e) restored image by LOGTV model; (f), (g), (h), (i), and (j) about the detailed image of (a), (b), (c), (d) and (e), respectively.

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