d100_18

Source: mapB

Source Composite Image

All sources below were be compared against this source composite image.

Instance: d100_18

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.
Model group: d100_03 Model group: d100_03_alternative Model group: d100_04 Model group: prob4_030_000500_04 Model group: prob4_020_000500_05 Model group: d100_02_alternative Model group: ring_n10p0.1s2 Model group: prob4_005_000500_02 Model group: prob4_020_001000_02 Model group: prob4_030_001000_07 Model group: prob4_010_000500_03 Model group: d100_14 Model group: tr12-15 Model group: prob4_010_000500_07 Model group: d100_20_alternative Model group: prob4_010_001000_02 Model group: tr24-15 Model group: d100_10_alternative Model group: prob4_005_001000_09 Model group: vpm2a Model group: d100_11 Model group: prob2_050_040_060_015_025_10 Model group: d100_20 Model group: prob2_050_040_060_025_035_05 Model group: prob3_050_040_060_015_025_06 Model group: prob2_050_040_060_035_045_01 Model group: prob3_050_040_060_035_045_01 Model group: prob1_050_040_060_025_035_08 Model group: n20p5t2s4 Model group: prob1_050_040_060_035_045_03 Model group: tr24-30 Model group: prob2_050_040_060_035_045_04 Model group: prob2_050_090_110_015_025_06 Model group: prob1_100_040_060_025_035_04 Model group: prob4_020_002500_06 Model group: prob1_050_040_060_015_025_06 Model group: prob2_100_040_060_035_045_10 Model group: prob1_050_040_060_015_025_05 Model group: prob1_100_040_060_015_025_08 Model group: prob1_100_040_060_035_045_09 Model group: prob3_050_090_110_025_035_04 Model group: pp08a Model group: prob1_100_040_060_005_015_04 Model group: prob3_050_090_110_015_025_08 Model group: prob3_050_090_110_005_015_06 Model group: prob2_100_040_060_035_045_06 Model group: prob2_050_090_110_025_035_08 Model group: prob1_100_040_060_035_045_06 Model group: prob1_100_090_110_015_025_04 Model group: prob2_050_090_110_035_045_07
Name (Source) d100_03 (mapB) d100_03_alternative (mapA) d100_04 (mapB) prob4_030_000500_04 (kps) prob4_020_000500_05 (kps) d100_02_alternative (mapA) ring_n10p0.1s2 (pcp) prob4_005_000500_02 (kps) prob4_020_001000_02 (kps) prob4_030_001000_07 (kps) prob4_010_000500_03 (kps) d100_14 (mapB) tr12-15 (lotC) prob4_010_000500_07 (kps) d100_20_alternative (mapA) prob4_010_001000_02 (kps) tr24-15 (lotC) d100_10_alternative (mapA) prob4_005_001000_09 (kps) vpm2a (lotC) d100_11 (mapB) prob2_050_040_060_015_025_10 (kps) d100_20 (mapB) prob2_050_040_060_025_035_05 (kps) prob3_050_040_060_015_025_06 (kps) prob2_050_040_060_035_045_01 (kps) prob3_050_040_060_035_045_01 (kps) prob1_050_040_060_025_035_08 (kps) n20p5t2s4 (pcp) prob1_050_040_060_035_045_03 (kps) tr24-30 (lotC) prob2_050_040_060_035_045_04 (kps) prob2_050_090_110_015_025_06 (kps) prob1_100_040_060_025_035_04 (kps) prob4_020_002500_06 (kps) prob1_050_040_060_015_025_06 (kps) prob2_100_040_060_035_045_10 (kps) prob1_050_040_060_015_025_05 (kps) prob1_100_040_060_015_025_08 (kps) prob1_100_040_060_035_045_09 (kps) prob3_050_090_110_025_035_04 (kps) pp08a (lotC) prob1_100_040_060_005_015_04 (kps) prob3_050_090_110_015_025_08 (kps) prob3_050_090_110_005_015_06 (kps) prob2_100_040_060_035_045_06 (kps) prob2_050_090_110_025_035_08 (kps) prob1_100_040_060_035_045_06 (kps) prob1_100_090_110_015_025_04 (kps) prob2_050_090_110_035_045_07 (kps)
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 / 1.345 2 / 1.360 3 / 1.536 4 / 1.587 5 / 1.641 6 / 1.657 7 / 1.675 8 / 1.867 9 / 1.869 10 / 1.874 11 / 1.882 12 / 1.889 13 / 1.906 14 / 1.922 15 / 1.959 16 / 1.966 17 / 1.993 18 / 2.008 19 / 2.010 20 / 2.038 21 / 2.040 22 / 2.076 23 / 2.076 24 / 2.088 25 / 2.100 26 / 2.100 27 / 2.105 28 / 2.124 29 / 2.125 30 / 2.127 31 / 2.129 32 / 2.137 33 / 2.148 34 / 2.151 35 / 2.152 36 / 2.163 37 / 2.165 38 / 2.165 39 / 2.185 40 / 2.187 41 / 2.188 42 / 2.190 43 / 2.193 44 / 2.196 45 / 2.201 46 / 2.207 47 / 2.219 48 / 2.222 49 / 2.223 50 / 2.234