Research in
Algorithms for Geometric Pattern Matching
MIT2001-06
Progress Report:
January 1, 2002 Ð June 30, 2002
Piotr Indyk
Project Overview
Geometric pattern matching is pervasive in many
areas of computer science, e.g., in computer vision, computational drug design
and computational biology. The
goal of this project is to develop efficient algorithms for key geometric
pattern matching problems.
During
the period of January-June 2002, the main focus of this project was
implementing and evaluating algorithms for embedding Earth-Mover Distance into
the Euclidean space. Earth-mover distance (EMD) is a recently proposed metric
for computing distance between features of images (see [EMD] and references
therein). It was experimentally verified to capture well the perceptual notion
of a difference between images, in fact much better than other well-known
metrics (e.g., Euclidean distance between the feature vectors). The basic idea
behind EMD is as follows. Assume that the features of an image are represented
by a set of points in low-dimensional space Rd.
For example, an image could be represented by a set of pixels, where each pixel
is a point in 3-dimensional color space or texture space. The distance between
two sets of points (representing two different images) is defined as the
minimum amount of work needed to transform one set into another. Formally, this
corresponds to the minimum weight matching between the two sets of points.
Since EMD has been shown to outperform other
measures for comparing color or texture similarity between images, it is of
great interest to design efficient algorithms for pattern matching under this
metric. In particular, the most interesting case occurs when one is given a
ÒqueryÓ image, and wants to scan a large database of images, in order to find
the image most similar to the query. The approach used so far is to compute the
distances between the query image and each image stored in the database. This is highly inefficient, since the
time needed to answer a query could be very large for large databases.
During the earlier stages of this project we
designed a method which drastically reduces the time needed to solve this
problem [ITÕ01]. The main
idea of our approach is to embed the Earth Mover Distance into the
Euclidean space and use very efficient nearest neighbor data structure for the
latter (well-studied) space. In other words, we show that one can represent
each pixel set by a feature vector, in such a way that the EMD between two
pixel sets is approximately proportional to the Euclidean distance between the
feature vectors. The distortion induced by the embedding algorithm is provably
bounded.
Since very fast nearest neighbor algorithms for
the Euclidean space are known (e.g., see [IMÕ98, GIMÕ98]), our embedding method
yields dramatic improvement in the running of nearest neighbor algorithms for
EMD. However, as we mentioned above, the embedding is not exact Ð it introduces
a small error which could in
principle affect the quality of the retrieved images. Thus, for this approach
to work in practice, it is crucial to verify that the actual error occurring in practice is low. This could
require additional adjustments and fine-tuning of the algorithm, to minimize
the embedding error.
In the next section we describe our progress on
implementing and evaluating our method in the context of image retrieval in
large image databases.
Progress through June 2002
We have implemented a system, which given a large
collection of images, extracts color features of the images, embeds them into
the Euclidean space and then enables to search for similar images. Due to efficient implementation of the
algorithm, the embedding procedures take very little time compared to the time
needed to extract color
information from images, and thus time overhead of our method is essentially
negligible.
Having the system ready, we performed preliminary
experiments comparing similarities of images under the embedded EMD with the
actual EMD. The experiments were performed on images taken from the CorelDraw
image database, with varied number of images. The experiments revealed that the
actual embedding error, as well as the error resulting from computing nearest
neighbor under the Òembedded EMDÓ as opposed to original EMD, was very small.
In many cases, it was smaller than 10%. This discovery is quite significant,
since it means that the actual error is much smaller than it would follow from
our current theoretical bound [ITÕ01]. In addition, anecdotal user experiments indicate that this small error is
negligible in the context of searching for perceptually similar images. Thus, our algorithm replaces the
need of dealing with a fairly intractable metric (the well-studied Euclidean
space is used instead), while essentially preserving the quality of the
retrieval of the original EMD metric.
Research Plan for the Next Six Months
Our
main goals for the nearest future are:
á
Perform further
experiments on additional data sets, to evaluate the embedding error, as a
function of various embedding parameters. This will allow us to fine-tune the
parameters to achieve the optimal retrieval performance
á
Implement fast
nearest neighbor algorithms for searching in the space of embedded color
histograms; perform extensive timing experiments
á
Build an
easy-to-navigate user interface
á
Perform rigorous
user experiments to measure the influence of the embedding error on the
perceptual retrieval error
á
Write a report
In addition (time permitting) we plan to
investigate the (quite fortunate!) discrepancy between the theoretical error
bounds and the error we achieve in practice. This could entail developing a
model for color histogram data sets which are closer to reality than the
current worst-case approach.
References
[EMD] Scott Cohen, ÒComputing Earth-Mover distance under
transformationsÓ,
http://robotics.stanford.edu/~scohen/research/emdg/emdg.html
[GIMÕ99] Aris Gionis, Piotr Indyk and Rajeev
Motwani, ÒSimilarity Search in High Dimensions via HashingÓ, IEEE Symposium on
Very Large Databases, 1999.
[IMÕ98] Piotr Indyk and Rajeev Motwani,
ÒApproximate Nearest Neighbor Ð Towards Removing the Curse of DimensionalityÓ,
ACM Symposium on Theory of Computing, 1998.
[ITÕ01] Piotr Indyk and Nitin Thaper, ÒEmbedding Earth-Mover Distance into
the Euclidean spaceÓ, manuscript, 2001.