2013
DOI: 10.1016/j.jvcir.2013.01.004
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A restoration algorithm for images contaminated by mixed Gaussian plus random-valued impulse noise

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Cited by 24 publications
(18 citation statements)
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“…The results are presented in Table 8, which demonstrate that PWMF is rather fast: much faster than NLMixF and even faster than TriF when the noise level is low, thanks to the simplified joint impulse factor F (k, T (k)) defined in (17). The results also show that our method is faster than Zhou [38]. which can be considered as impulse noise, to make an impartial comparison, we compute PSNR for Peppers images after removing all the four boundaries, that is with images of size 510 × 510 for Peppers512 and 254 × 254 for Peppers256 Table 3: PSNR values (dB) to remove impulse noise for TriF [18], ROLD-EPR [13], PARIGI [12], NLMixF [20] and our filter PWMF Lena p = 0.2 p = 0.3 p = 0.4 p = 0.5 Bridge p = 0.2 p = 0.3 p = 0.4 p = 0.5 Peppers256 p = 0.2 p = 0.3 p = 0.4 p = 0.5 Peppers512 p = 0.2 p = 0.3 p = 0.4 p = 0.5 Boats p = 0.2 p = 0.3 p = 0.4 p = 0.5 [18], ROLD-EPR [13], PARIGI [12] and our filter PWMF for removing impulse noise with p = 0.4 for Peppers512 Table 6: PSNR values (dB) for mixed noise removal with (Xiao) [32], (IPAMF+BM) [35], (Zhou) [38] and our filter PWMF Lena σ = 10 p = 0.1 p = 0.2 p = 0.…”
Section: Experiments and Comparisonsmentioning
confidence: 85%
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“…The results are presented in Table 8, which demonstrate that PWMF is rather fast: much faster than NLMixF and even faster than TriF when the noise level is low, thanks to the simplified joint impulse factor F (k, T (k)) defined in (17). The results also show that our method is faster than Zhou [38]. which can be considered as impulse noise, to make an impartial comparison, we compute PSNR for Peppers images after removing all the four boundaries, that is with images of size 510 × 510 for Peppers512 and 254 × 254 for Peppers256 Table 3: PSNR values (dB) to remove impulse noise for TriF [18], ROLD-EPR [13], PARIGI [12], NLMixF [20] and our filter PWMF Lena p = 0.2 p = 0.3 p = 0.4 p = 0.5 Bridge p = 0.2 p = 0.3 p = 0.4 p = 0.5 Peppers256 p = 0.2 p = 0.3 p = 0.4 p = 0.5 Peppers512 p = 0.2 p = 0.3 p = 0.4 p = 0.5 Boats p = 0.2 p = 0.3 p = 0.4 p = 0.5 [18], ROLD-EPR [13], PARIGI [12] and our filter PWMF for removing impulse noise with p = 0.4 for Peppers512 Table 6: PSNR values (dB) for mixed noise removal with (Xiao) [32], (IPAMF+BM) [35], (Zhou) [38] and our filter PWMF Lena σ = 10 p = 0.1 p = 0.2 p = 0.…”
Section: Experiments and Comparisonsmentioning
confidence: 85%
“…Different papers consider different mixtures of Gaussian noise and impulse noise. We show the performance of PWMF for removing mixed noise in Tables 4, 5, 6, and 7 by comparing it with TriF [18], NLMixF [20], PA-RIGI [12] IPAMF+BM [35], Xiao [32], MNF [22], and Zhou [38]. All these comparisons show good performance of our filter except for Barbara when comparing with PARIGI.…”
Section: Experiments and Comparisonsmentioning
confidence: 95%
“…Given the excellent performance of non-local methods [2,5], learned sparse models [8,18], and the combination of both [6,17] for random Gaussian noise, they were explored for impulse noise as well [20,22]. Non-local methods use redundant visual information within an image (i.e., self-similarity) to group similar image patches together, followed by collaborative filtering [2,5].…”
Section: Related Workmentioning
confidence: 99%
“…The final S can be easily estimated from the difference between the input P and the output L (see [22] …”
Section: Optimizationmentioning
confidence: 99%
“…Uniform impulse noise is considered by replacing a portion of some image pixel values with random values. Speckle noise is characterized by 2 Mathematical Problems in Engineering signal-dependent noise where the noise corrupts the image in the form of multiplicative noise [5][6][7][8][9][10][11][12].…”
Section: Introductionmentioning
confidence: 99%