sa45_40-fasano

Source: clpB

Source Composite Image

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

Instance: sa45_40-fasano

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: sa20_50-fasano Model group: sa45_85-fasano Model group: sa15_85-fasano Model group: sa20_100-fasano Model group: sa35_75-fasano Model group: 3-club_covering_karate Model group: sa45_25-hifi Model group: sa5_30-junqueira Model group: sa5_35-junqueira Model group: gapb_6-max Model group: gapd_6-max Model group: gapc_6-max Model group: e20200_1-max Model group: a20200_1-min Model group: N3W4B2R8.BPPeq Model group: N3W4B2R7.BPPgq Model group: c20100_1-min Model group: gapc_5-min Model group: gapb_5-min Model group: d15900_1-max Model group: a10200_1-min Model group: c10200_1-max Model group: c10200_1-min Model group: c10400_1-max Model group: d10400_1-min Model group: BR1_90-tsai Model group: N3W3B1R5.BPPeq Model group: 3-club_covering_chesapeake Model group: BR7_93-tsai Model group: BR2_43-tsai Model group: N60B100.0t60_06.BPPeq Model group: N60B100.0t60_07.BPPeq Model group: N60B100.0t60_09.BPPgq Model group: N60B100.0t60_13.BPPeq Model group: sa15_95-tsai Model group: BR6_23-tsai Model group: BR3_46-tsai Model group: N2W1B1R3.BPPgq Model group: TEST0054-wae-eq Model group: sa35_15-tsai Model group: sa40_10-fasano Model group: N1W2B3R5.BPPeq Model group: e10100_1-max Model group: gapb_3-min Model group: a10100_1-min Model group: BPP58-s2-eq Model group: BPP83-s1-eq Model group: BPP93-s1-eq Model group: sa10_60-hifi Model group: TEST0084-wae-eq
Name (Source) sa20_50-fasano (clpB) sa45_85-fasano (clpB) sa15_85-fasano (clpB) sa20_100-fasano (clpB) sa35_75-fasano (clpB) 3-club_covering_karate (relD) sa45_25-hifi (clpC) sa5_30-junqueira (clpD) sa5_35-junqueira (clpD) gapb_6-max (gapA) gapd_6-max (gapA) gapc_6-max (gapA) e20200_1-max (gapC) a20200_1-min (gapD) N3W4B2R8.BPPeq (bppA) N3W4B2R7.BPPgq (bppB) c20100_1-min (gapD) gapc_5-min (gapB) gapb_5-min (gapB) d15900_1-max (gapC) a10200_1-min (gapD) c10200_1-max (gapC) c10200_1-min (gapD) c10400_1-max (gapC) d10400_1-min (gapD) BR1_90-tsai (clpF) N3W3B1R5.BPPeq (bppA) 3-club_covering_chesapeake (relD) BR7_93-tsai (clpF) BR2_43-tsai (clpF) N60B100.0t60_06.BPPeq (bppC) N60B100.0t60_07.BPPeq (bppC) N60B100.0t60_09.BPPgq (bppD) N60B100.0t60_13.BPPeq (bppC) sa15_95-tsai (clpF) BR6_23-tsai (clpF) BR3_46-tsai (clpF) N2W1B1R3.BPPgq (bppB) TEST0054-wae-eq (cutG) sa35_15-tsai (clpF) sa40_10-fasano (clpB) N1W2B3R5.BPPeq (bppA) e10100_1-max (gapC) gapb_3-min (gapB) a10100_1-min (gapD) BPP58-s2-eq (cutE) BPP83-s1-eq (cutE) BPP93-s1-eq (cutE) sa10_60-hifi (clpC) TEST0084-wae-eq (cutG)
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 / 2.189 2 / 4.827 3 / 7.398 4 / 7.642 5 / 7.705 6 / 8.246 7 / 8.295 8 / 8.341 9 / 8.502 10 / 8.560 11 / 8.560 12 / 8.560 13 / 8.560 14 / 8.560 15 / 8.725 16 / 8.725 17 / 8.737 18 / 8.737 19 / 8.737 20 / 8.827 21 / 8.874 22 / 8.874 23 / 8.874 24 / 8.890 25 / 8.890 26 / 8.913 27 / 8.914 28 / 8.969 29 / 9.007 30 / 9.020 31 / 9.041 32 / 9.041 33 / 9.041 34 / 9.041 35 / 9.079 36 / 9.084 37 / 9.097 38 / 9.125 39 / 9.156 40 / 9.164 41 / 9.164 42 / 9.172 43 / 9.173 44 / 9.173 45 / 9.173 46 / 9.209 47 / 9.209 48 / 9.212 49 / 9.221 50 / 9.234
Updated August 16, 2019