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N3W3B1R5.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)
N3W4B2R8.BPPeq
(bppA)
N3W2B1R4.BPPgq
(bppB)
N3W3B2R2.BPPeq
(bppA)
a20200_1-min
(gapD)
e20200_1-max
(gapC)
gapc_6-max
(gapA)
gapd_6-max
(gapA)
gapb_6-max
(gapA)
d15900_1-max
(gapC)
c201600_1-min
(gapD)
e201600_1-max
(gapC)
e30900_1-min
(gapD)
d30900_1-min
(gapD)
N120B100.0t120_04.BPPeq
(bppC)
N120B100.0t120_09.BPPeq
(bppC)
N120B100.0t120_06.BPPgq
(bppD)
N2W1B1R3.BPPgq
(bppB)
sa5_30-junqueira
(clpD)
sa5_35-junqueira
(clpD)
gapc_5-min
(gapB)
gapb_5-min
(gapB)
c20100_1-min
(gapD)
c10400_1-max
(gapC)
d10400_1-min
(gapD)
sa15_95-tsai
(clpF)
TEST0084-wae-eq
(cutG)
N60B100.0t60_13.BPPeq
(bppC)
N60B100.0t60_06.BPPeq
(bppC)
N60B100.0t60_07.BPPeq
(bppC)
N60B100.0t60_09.BPPgq
(bppD)
BR6_23-tsai
(clpF)
sa5_10-junqueira
(clpD)
sa35_15-tsai
(clpF)
BR1_90-tsai
(clpF)
BR7_93-tsai
(clpF)
BR3_46-tsai
(clpF)
BR2_43-tsai
(clpF)
TEST0054-wae-eq
(cutG)
TEST0005-wae-eq
(cutG)
TEST0005-wae-gq
(cutH)
TEST0055-wae-gq
(cutH)
c10200_1-max
(gapC)
a10200_1-min
(gapD)
c10200_1-min
(gapD)
p4
(cpmE)
p2050-2.eq
(cpmC)
p7
(cpmE)
p2050-1.eq
(cpmC)
p23-6.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 / 1.181
2 / 1.181
3 / 2.363
4 / 2.363
5 / 2.578
6 / 2.578
7 / 2.578
8 / 2.578
9 / 2.578
10 / 2.847
11 / 3.132
12 / 3.132
13 / 3.343
14 / 3.343
15 / 3.431
16 / 3.431
17 / 3.431
18 / 3.581
19 / 3.637
20 / 3.775
21 / 4.068
22 / 4.068
23 / 4.068
24 / 4.377
25 / 4.377
26 / 4.576
27 / 4.651
28 / 4.656
29 / 4.656
30 / 4.656
31 / 4.656
32 / 4.728
33 / 4.747
34 / 4.810
35 / 4.817
36 / 4.869
37 / 4.870
38 / 4.900
39 / 4.923
40 / 5.118
41 / 5.124
42 / 5.145
43 / 5.157
44 / 5.157
45 / 5.157
46 / 5.214
47 / 5.214
48 / 5.214
49 / 5.214
50 / 5.214