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2-FullIns_4.col.disa
Source: colD
Source Composite Image
All sources below were be compared against this source composite image.  |
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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.
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| Name (Source) | nsf_p0.3_s5 (pcp) | nsf_p0.4_s4 (pcp) | nsf_p0.3_s3 (pcp) | 1-Insertions_5.col.bigM (colC) | nsf_p0.4_s2 (pcp) | nsf_p0.3_s1 (pcp) | jean.col.bigM (colC) | ring_n10p0.7s5 (pcp) | n90p2t2s2 (pcp) | n90p2t2s4 (pcp) | n90p2t2s1 (pcp) | R75_5gb.col.bigM (colG) | R75_5g.col.bigM (colG) | queen7_7.col.bigM (colC) | nsf_p0.5_s5 (pcp) | 2-Insertions_4.col.disa (colD) | gcol12.disa (colF) | n100p5t2s5 (pcp) | gcol10.disa (colF) | n90p1t2s2 (pcp) | n100p5t2s2 (pcp) | nsf_p0.5_s1 (pcp) | gcol17.disa (colF) | n100p5t2s4 (pcp) | ring_n10p0.6s3 (pcp) | n100p5t2s3 (pcp) | gcol3.disa (colF) | n90p1t2s3 (pcp) | gcol15.disa (colF) | ring_n10p0.6s2 (pcp) | nsf_p0.2_s5 (pcp) | gcol13.disa (colF) | gcol20.disa (colF) | queen10_10.col.bigM (colC) | gcol12.bigM (colE) | ring_n10p0.5s2 (pcp) | myciel6.col.disa (colD) | gcol10.bigM (colE) | gcol7.bigM (colE) | gcol6.bigM (colE) | gcol19.bigM (colE) | gcol20.bigM (colE) | gcol3.bigM (colE) | R100_5g.col.bigM (colG) | n90p4t2s3 (pcp) | n90p8t2s4 (pcp) | n90p9t2s4 (pcp) | n90p6t2s3 (pcp) | n90p9t2s3 (pcp) | n90p5t2s1 (pcp) | |
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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.
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1 / 0.487 | 2 / 0.512 | 3 / 0.534 | 4 / 0.541 | 5 / 0.541 | 6 / 0.561 | 7 / 0.596 | 8 / 0.625 | 9 / 0.640 | 10 / 0.672 | 11 / 0.676 | 12 / 0.679 | 13 / 0.679 | 14 / 0.684 | 15 / 0.700 | 16 / 0.703 | 17 / 0.711 | 18 / 0.714 | 19 / 0.714 | 20 / 0.716 | 21 / 0.717 | 22 / 0.717 | 23 / 0.719 | 24 / 0.720 | 25 / 0.722 | 26 / 0.723 | 27 / 0.724 | 28 / 0.726 | 29 / 0.728 | 30 / 0.732 | 31 / 0.735 | 32 / 0.737 | 33 / 0.740 | 34 / 0.742 | 35 / 0.745 | 36 / 0.749 | 37 / 0.751 | 38 / 0.752 | 39 / 0.757 | 40 / 0.761 | 41 / 0.775 | 42 / 0.775 | 43 / 0.776 | 44 / 0.778 | 45 / 0.779 | 46 / 0.785 | 47 / 0.786 | 48 / 0.787 | 49 / 0.787 | 50 / 0.788 |
