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Table 1 Performance of various algorithms at different noise densities for PSNR on Lena image corrupted by SPN

From: An adaptive decision based interpolation scheme for the removal of high density salt and pepper noise in images

Noise in %

PSNR in DB

SMF [30]

AMF [6]

PSMF [10]

αTMF

α = 4 [30]

CWF [7]

DBA [13]

MDBMF [16]

CUDBMPF [15]

MDBUTMF [17]

MDBUMF-GM [18]

ACBSA [20]

AWMF [23]

DBIDWIF [PA]

10

34.9

39.3

38.8

27.6

35.2

39

45.2

32.3

43.1

45.3

41.9

39.37

43.01

20

30.3

36.9

33.4

24.6

28.1

36.8

41.5

32.1

41.2

41.6

38.8

38.16

40.26

30

23.9

34.6

29.4

21

22.2

35.8

38.8

31.8

37.9

38.8

37.1

36.94

38.5

40

19

32.2

25.4

17.9

17.8

33.2

36.5

31.4

36.4

36.5

35.5

35.88

37.15

50

15.9

27.3

25.3

15.7

14.3

31.4

34.4

31.1

34.3

34.53

33.8

34.57

35.68

60

12.3

21.6

21.2

13.8

11.7

29.6

32.1

30.3

32.1

32.1

30.3

33.14

34.31

70

10

16.6

9.9

12.3

9.6

27.8

29.6

30.2

29.6

29.73

29.8

31.38

32.44

80

8.1

12.7

8.1

11.1

7.9

25.5

26.5

29.3

26.8

28.78

27.2

29.4

30.34

90

6.6

9.86

6.6

10.1

6.5

21.8

22.1

27.4

22.4

22.36

26.6

25.97

28.45