sa10_60-hifi

Source: clpC

Source Composite Image

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

Instance: sa10_60-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: sa25_80-hifi Model group: BR1_20-hifi Model group: BR6_40-hifi Model group: sa5_35-junqueira Model group: d30900_1-min Model group: e30900_1-min Model group: BR1_3-hifi Model group: e201600_1-max Model group: c201600_1-min Model group: BR6_19-hifi Model group: sa45_25-hifi Model group: d15900_1-max Model group: sa5_30-junqueira Model group: N3W4B2R7.BPPgq Model group: N3W4B2R8.BPPeq Model group: N3W3B1R5.BPPeq Model group: gapc_6-max Model group: a20200_1-min Model group: gapb_6-max Model group: gapd_6-max Model group: e20200_1-max Model group: BR6_5-hifi Model group: N3W3B2R2.BPPeq Model group: N3W2B1R4.BPPgq Model group: c60900_1-max Model group: d60900_1-max Model group: e60900_1-max Model group: d10400_1-min Model group: c10400_1-max Model group: N120B100.0t120_06.BPPgq Model group: N120B100.0t120_04.BPPeq Model group: N120B100.0t120_09.BPPeq Model group: sa5_95-junqueira Model group: 5-club_covering_chesapeake Model group: 5-club_partitioning_chesapeake Model group: N2W1B1R3.BPPgq Model group: 3-club_covering_karate Model group: sa5_100-junqueira Model group: 4-club_covering_chesapeake Model group: 3-club_covering_chesapeake Model group: c20100_1-min Model group: gapb_5-min Model group: gapc_5-min Model group: sa5_10-junqueira Model group: sa35_15-tsai Model group: 4-club_covering_lesmis Model group: a10200_1-min Model group: c10200_1-min Model group: c10200_1-max Model group: BR1_90-tsai
Name (Source) sa25_80-hifi (clpC) BR1_20-hifi (clpC) BR6_40-hifi (clpC) sa5_35-junqueira (clpD) d30900_1-min (gapD) e30900_1-min (gapD) BR1_3-hifi (clpC) e201600_1-max (gapC) c201600_1-min (gapD) BR6_19-hifi (clpC) sa45_25-hifi (clpC) d15900_1-max (gapC) sa5_30-junqueira (clpD) N3W4B2R7.BPPgq (bppB) N3W4B2R8.BPPeq (bppA) N3W3B1R5.BPPeq (bppA) gapc_6-max (gapA) a20200_1-min (gapD) gapb_6-max (gapA) gapd_6-max (gapA) e20200_1-max (gapC) BR6_5-hifi (clpC) N3W3B2R2.BPPeq (bppA) N3W2B1R4.BPPgq (bppB) c60900_1-max (gapC) d60900_1-max (gapC) e60900_1-max (gapC) d10400_1-min (gapD) c10400_1-max (gapC) N120B100.0t120_06.BPPgq (bppD) N120B100.0t120_04.BPPeq (bppC) N120B100.0t120_09.BPPeq (bppC) sa5_95-junqueira (clpD) 5-club_covering_chesapeake (relD) 5-club_partitioning_chesapeake (relE) N2W1B1R3.BPPgq (bppB) 3-club_covering_karate (relD) sa5_100-junqueira (clpD) 4-club_covering_chesapeake (relD) 3-club_covering_chesapeake (relD) c20100_1-min (gapD) gapb_5-min (gapB) gapc_5-min (gapB) sa5_10-junqueira (clpD) sa35_15-tsai (clpF) 4-club_covering_lesmis (relD) a10200_1-min (gapD) c10200_1-min (gapD) c10200_1-max (gapC) BR1_90-tsai (clpF)
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 / 2.515 2 / 3.306 3 / 4.219 4 / 5.117 5 / 5.164 6 / 5.164 7 / 5.236 8 / 5.292 9 / 5.292 10 / 5.493 11 / 5.518 12 / 5.549 13 / 5.592 14 / 5.692 15 / 5.692 16 / 5.736 17 / 5.959 18 / 5.959 19 / 5.959 20 / 5.959 21 / 5.959 22 / 6.011 23 / 6.039 24 / 6.039 25 / 6.425 26 / 6.425 27 / 6.425 28 / 6.756 29 / 6.756 30 / 6.929 31 / 6.929 32 / 6.929 33 / 6.971 34 / 7.069 35 / 7.069 36 / 7.085 37 / 7.099 38 / 7.130 39 / 7.140 40 / 7.336 41 / 7.360 42 / 7.360 43 / 7.360 44 / 7.458 45 / 7.524 46 / 7.547 47 / 7.554 48 / 7.554 49 / 7.554 50 / 7.591
Updated August 16, 2019