sa25_80-hifi

Source: clpC

Source Composite Image

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

Instance: sa25_80-hifi

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: BR1_20-hifi Model group: BR6_40-hifi Model group: sa10_60-hifi Model group: BR1_3-hifi Model group: BR6_19-hifi Model group: BR6_5-hifi Model group: d30900_1-min Model group: e30900_1-min Model group: c201600_1-min Model group: e201600_1-max Model group: sa5_35-junqueira Model group: e60900_1-max Model group: d60900_1-max Model group: c60900_1-max Model group: d15900_1-max Model group: sa5_30-junqueira Model group: sa45_25-hifi Model group: N3W2B1R4.BPPgq Model group: N3W3B2R2.BPPeq Model group: N3W3B1R5.BPPeq Model group: N3W4B2R7.BPPgq Model group: N3W4B2R8.BPPeq Model group: e20200_1-max Model group: a20200_1-min Model group: gapc_6-max Model group: gapb_6-max Model group: gapd_6-max Model group: sa5_95-junqueira Model group: sa5_100-junqueira Model group: 5-club_partitioning_chesapeake Model group: 5-club_covering_chesapeake Model group: d10400_1-min Model group: c10400_1-max Model group: 4-club_covering_chesapeake Model group: N120B100.0t120_04.BPPeq Model group: N120B100.0t120_09.BPPeq Model group: N120B100.0t120_06.BPPgq Model group: 3-club_covering_karate Model group: 3-club_covering_chesapeake Model group: N2W1B1R3.BPPgq Model group: 4-club_covering_lesmis Model group: 5-club_partitioning_lesmis Model group: BR1_90-tsai Model group: sa5_10-junqueira Model group: sa35_15-tsai Model group: BR7_93-tsai Model group: BR2_43-tsai Model group: sa15_95-tsai Model group: gapc_5-min Model group: c20100_1-min
Name (Source) BR1_20-hifi (clpC) BR6_40-hifi (clpC) sa10_60-hifi (clpC) BR1_3-hifi (clpC) BR6_19-hifi (clpC) BR6_5-hifi (clpC) d30900_1-min (gapD) e30900_1-min (gapD) c201600_1-min (gapD) e201600_1-max (gapC) sa5_35-junqueira (clpD) e60900_1-max (gapC) d60900_1-max (gapC) c60900_1-max (gapC) d15900_1-max (gapC) sa5_30-junqueira (clpD) sa45_25-hifi (clpC) N3W2B1R4.BPPgq (bppB) N3W3B2R2.BPPeq (bppA) N3W3B1R5.BPPeq (bppA) N3W4B2R7.BPPgq (bppB) N3W4B2R8.BPPeq (bppA) e20200_1-max (gapC) a20200_1-min (gapD) gapc_6-max (gapA) gapb_6-max (gapA) gapd_6-max (gapA) sa5_95-junqueira (clpD) sa5_100-junqueira (clpD) 5-club_partitioning_chesapeake (relE) 5-club_covering_chesapeake (relD) d10400_1-min (gapD) c10400_1-max (gapC) 4-club_covering_chesapeake (relD) N120B100.0t120_04.BPPeq (bppC) N120B100.0t120_09.BPPeq (bppC) N120B100.0t120_06.BPPgq (bppD) 3-club_covering_karate (relD) 3-club_covering_chesapeake (relD) N2W1B1R3.BPPgq (bppB) 4-club_covering_lesmis (relD) 5-club_partitioning_lesmis (relE) BR1_90-tsai (clpF) sa5_10-junqueira (clpD) sa35_15-tsai (clpF) BR7_93-tsai (clpF) BR2_43-tsai (clpF) sa15_95-tsai (clpF) gapc_5-min (gapB) c20100_1-min (gapD)
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 / 1.329 2 / 2.263 3 / 2.515 4 / 3.341 5 / 3.598 6 / 4.212 7 / 5.757 8 / 5.757 9 / 6.173 10 / 6.173 11 / 6.256 12 / 6.334 13 / 6.334 14 / 6.334 15 / 6.815 16 / 6.843 17 / 6.861 18 / 6.927 19 / 6.927 20 / 6.937 21 / 6.984 22 / 6.984 23 / 7.351 24 / 7.351 25 / 7.351 26 / 7.351 27 / 7.351 28 / 7.528 29 / 7.717 30 / 7.978 31 / 7.978 32 / 8.114 33 / 8.114 34 / 8.120 35 / 8.200 36 / 8.200 37 / 8.200 38 / 8.357 39 / 8.454 40 / 8.552 41 / 8.557 42 / 8.688 43 / 8.815 44 / 8.819 45 / 8.822 46 / 8.853 47 / 8.864 48 / 8.902 49 / 8.914 50 / 8.914
Updated August 16, 2019