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N3W4B2R8.BPPeq
Source:
bppA
Source Composite Image
All sources below were be compared against this source composite image.
Top 49 Most Similar strIPlib Instances
These are the 49 CCM images (for individual instances) that are most similar to the CCM image for this instance, according to the ISS metric.
These are the 49 most similar strIPlib instance CCM images.
Name (Source)
N3W4B2R7.BPPgq
(bppB)
N3W3B1R5.BPPeq
(bppA)
gapc_6-max
(gapA)
gapd_6-max
(gapA)
gapb_6-max
(gapA)
a20200_1-min
(gapD)
e20200_1-max
(gapC)
d15900_1-max
(gapC)
N3W2B1R4.BPPgq
(bppB)
N3W3B2R2.BPPeq
(bppA)
c201600_1-min
(gapD)
e201600_1-max
(gapC)
sa5_30-junqueira
(clpD)
N2W1B1R3.BPPgq
(bppB)
N120B100.0t120_09.BPPeq
(bppC)
N120B100.0t120_06.BPPgq
(bppD)
N120B100.0t120_04.BPPeq
(bppC)
sa5_35-junqueira
(clpD)
d30900_1-min
(gapD)
e30900_1-min
(gapD)
gapb_5-min
(gapB)
gapc_5-min
(gapB)
c20100_1-min
(gapD)
c10400_1-max
(gapC)
d10400_1-min
(gapD)
N60B100.0t60_07.BPPeq
(bppC)
N60B100.0t60_06.BPPeq
(bppC)
N60B100.0t60_09.BPPgq
(bppD)
N60B100.0t60_13.BPPeq
(bppC)
TEST0084-wae-eq
(cutG)
sa5_10-junqueira
(clpD)
TEST0054-wae-eq
(cutG)
c10200_1-max
(gapC)
a10200_1-min
(gapD)
c10200_1-min
(gapD)
sa35_15-tsai
(clpF)
sa15_95-tsai
(clpF)
N1W2B3R5.BPPeq
(bppA)
TEST0005-wae-eq
(cutG)
BR6_23-tsai
(clpF)
TEST0005-wae-gq
(cutH)
TEST0055-wae-gq
(cutH)
p4
(cpmE)
p7
(cpmE)
p1
(cpmE)
p5
(cpmE)
p2050-2.eq
(cpmC)
p10
(cpmE)
p550-1.eq
(cpmC)
p1250-5.eq
(cpmC)
Rank / ISS
The image-based structural similarity (ISS) metric measures the Euclidean distance between two image-based feature vectors. A smaller ISS value indicates greater similarity.
1 / 0.000
2 / 1.181
3 / 2.038
4 / 2.038
5 / 2.038
6 / 2.038
7 / 2.038
8 / 2.421
9 / 2.739
10 / 2.739
11 / 3.128
12 / 3.128
13 / 3.196
14 / 3.214
15 / 3.300
16 / 3.300
17 / 3.300
18 / 3.390
19 / 3.453
20 / 3.453
21 / 3.528
22 / 3.528
23 / 3.528
24 / 3.851
25 / 3.851
26 / 4.141
27 / 4.141
28 / 4.141
29 / 4.141
30 / 4.251
31 / 4.265
32 / 4.440
33 / 4.533
34 / 4.533
35 / 4.533
36 / 4.595
37 / 4.644
38 / 4.702
39 / 4.710
40 / 4.718
41 / 4.721
42 / 4.764
43 / 4.771
44 / 4.771
45 / 4.771
46 / 4.771
47 / 4.771
48 / 4.771
49 / 4.771
50 / 4.771