d100_02_alternative

Source: mapA

Source Composite Image

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

Instance: d100_02_alternative

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_alternative Model group: d100_18 Model group: d100_03 Model group: d100_14 Model group: d100_20_alternative Model group: ring_n10p0.1s2 Model group: d100_11 Model group: d100_04 Model group: d100_10_alternative Model group: d250_08_alternative Model group: d100_20 Model group: d250_10 Model group: tr24-15 Model group: d250_21 Model group: d250_23_alternative Model group: d250_14 Model group: d250_13 Model group: n20p5t2s4 Model group: tr24-30 Model group: prob4_030_001000_07 Model group: prob4_020_001000_02 Model group: prob2_050_040_060_015_025_10 Model group: prob1_050_040_060_035_045_03 Model group: prob3_050_040_060_015_025_06 Model group: prob2_050_040_060_025_035_05 Model group: d250_17_alternative Model group: prob2_050_040_060_035_045_01 Model group: prob3_050_040_060_035_045_01 Model group: prob4_030_000500_04 Model group: d250_17 Model group: prob1_050_040_060_025_035_08 Model group: prob2_100_040_060_035_045_10 Model group: prob2_050_090_110_015_025_06 Model group: prob1_050_040_060_015_025_05 Model group: prob1_050_040_060_015_025_06 Model group: prob1_100_040_060_025_035_04 Model group: prob2_050_040_060_035_045_04 Model group: prob1_100_040_060_035_045_09 Model group: prob3_050_090_110_015_025_08 Model group: prob1_100_040_060_015_025_08 Model group: prob3_050_090_110_005_015_06 Model group: prob2_100_040_060_035_045_06 Model group: tr12-15 Model group: prob3_050_090_110_025_035_04 Model group: qwhopt.order5.holes10.1.col.bigM Model group: qwhdec.order5.holes10.1.col.bigM Model group: prob1_100_040_060_005_015_04 Model group: prob2_050_090_110_025_035_08 Model group: prob1_100_090_110_015_025_04 Model group: prob1_100_090_110_025_035_08
Name (Source) d100_03_alternative (mapA) d100_18 (mapB) d100_03 (mapB) d100_14 (mapB) d100_20_alternative (mapA) ring_n10p0.1s2 (pcp) d100_11 (mapB) d100_04 (mapB) d100_10_alternative (mapA) d250_08_alternative (mapA) d100_20 (mapB) d250_10 (mapB) tr24-15 (lotC) d250_21 (mapB) d250_23_alternative (mapA) d250_14 (mapB) d250_13 (mapB) n20p5t2s4 (pcp) tr24-30 (lotC) prob4_030_001000_07 (kps) prob4_020_001000_02 (kps) prob2_050_040_060_015_025_10 (kps) prob1_050_040_060_035_045_03 (kps) prob3_050_040_060_015_025_06 (kps) prob2_050_040_060_025_035_05 (kps) d250_17_alternative (mapA) prob2_050_040_060_035_045_01 (kps) prob3_050_040_060_035_045_01 (kps) prob4_030_000500_04 (kps) d250_17 (mapB) prob1_050_040_060_025_035_08 (kps) prob2_100_040_060_035_045_10 (kps) prob2_050_090_110_015_025_06 (kps) prob1_050_040_060_015_025_05 (kps) prob1_050_040_060_015_025_06 (kps) prob1_100_040_060_025_035_04 (kps) prob2_050_040_060_035_045_04 (kps) prob1_100_040_060_035_045_09 (kps) prob3_050_090_110_015_025_08 (kps) prob1_100_040_060_015_025_08 (kps) prob3_050_090_110_005_015_06 (kps) prob2_100_040_060_035_045_06 (kps) tr12-15 (lotC) prob3_050_090_110_025_035_04 (kps) qwhopt.order5.holes10.1.col.bigM (colA) qwhdec.order5.holes10.1.col.bigM (colA) prob1_100_040_060_005_015_04 (kps) prob2_050_090_110_025_035_08 (kps) prob1_100_090_110_015_025_04 (kps) prob1_100_090_110_025_035_08 (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 / 1.561 2 / 1.657 3 / 1.771 4 / 1.798 5 / 1.826 6 / 1.926 7 / 1.960 8 / 2.002 9 / 2.014 10 / 2.039 11 / 2.068 12 / 2.078 13 / 2.175 14 / 2.179 15 / 2.182 16 / 2.185 17 / 2.194 18 / 2.195 19 / 2.226 20 / 2.232 21 / 2.254 22 / 2.269 23 / 2.272 24 / 2.276 25 / 2.287 26 / 2.291 27 / 2.300 28 / 2.302 29 / 2.303 30 / 2.303 31 / 2.312 32 / 2.324 33 / 2.327 34 / 2.328 35 / 2.329 36 / 2.333 37 / 2.338 38 / 2.339 39 / 2.344 40 / 2.345 41 / 2.347 42 / 2.347 43 / 2.351 44 / 2.352 45 / 2.354 46 / 2.354 47 / 2.357 48 / 2.359 49 / 2.360 50 / 2.367