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Computational Models of Music Similarity and their ... - OFAI

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30 2 Audio-based <strong>Similarity</strong> Measures<br />

Blue Rondo ...<br />

Kathy’s Waltz<br />

Bad Med.<br />

Bring Me To ...<br />

Someday<br />

Bolero<br />

20<br />

0<br />

−20<br />

20<br />

0<br />

−20<br />

20<br />

0<br />

−20<br />

20<br />

0<br />

−20<br />

20<br />

0<br />

−20<br />

20<br />

0<br />

−20<br />

10 20 30<br />

10 20 30<br />

10 20 30<br />

10 20 30<br />

10 20 30<br />

10 20 30<br />

Figure 2.10: Illustration <strong>of</strong> the cluster model for G30. Each column shows different<br />

representations <strong>of</strong> one piece <strong>of</strong> music. The pieces are the same as the ones used in<br />

Figure 2.2. Each plot has the dimensions Mel frequency b<strong>and</strong> on the x-axis <strong>and</strong><br />

dB on the y-axis. That is, all MFCCs are reconstructed <strong>and</strong> visualized in the Mel<br />

space. The first row is a 2-dimensional histogram <strong>of</strong> all spectra (MFCCs). The<br />

second row are the 30 GMM centers. The gray shading corresponds to the prior <strong>of</strong><br />

each component (black being the highest prior). The third row shows a flattened<br />

probability density <strong>of</strong> the GMM. In particular, the variance <strong>of</strong> the components<br />

are visible. The fourth row shows the probability <strong>of</strong> the original MFCC frames.<br />

The frame with the highest probability is plotted in black. The fifth row shows<br />

the probabilities <strong>of</strong> the 2000 sample frames that are drawn from the GMM. Most<br />

<strong>of</strong> them are not visible because <strong>their</strong> probability is very small compared to the<br />

highest one. The last row shows the histogram <strong>of</strong> the sample drawn.

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