User:JohnMeier/Sandbox

Determining the number of clusters in a data set
Determining the number of clusters in a data set, a quantity often labeled k, is fundamental to the problem of data clustering, and is a distinct issue from the process of actually solving the clustering problem. In most cases, k must be chosen somehow and specified as an input parameter to clustering algorithms, with the exception of methods such as correlation clustering, which are able to determine the optimal number of clusters during the course of the algorithm. The correct choice of k is often ambiguous, with interpretations depending on the shape and scale of the distribution of points in a data set and the desired clustering resolution of the user. In addition, increasing k without penalty will always reduce the amount of error in the resulting clustering, to the extreme case of zero error if each data point is considered its own cluster (i.e., when k equals the number of data points, n). Intuitively then, the optimal choice of k will strike a balance between maximum compression of the data using a single cluster, and maximum accuracy by assigning each data point to its own cluster. If an appropriate value of k is not apparent from prior knowledge of the properties of the data set, it must be chosen somehow. There are several categories of methods for making this decision.

The Elbow Method
One rule of thumb looks at the percentage of variance explained as a function of the number of clusters: You should choose a number of clusters so that adding another cluster doesn't give much better modeling of the data. More precisely, if you graph the percentage of variance explained by the clusters against the number of clusters, the first clusters will add much information (explain a lot of variance), but at some point the marginal gain will drop, giving an angle in the graph. The number of clusters are chosen at this point, hence the "elbow criterion". This "elbow" cannot always be unambiguously identified. Percentage of variance explained is the ratio of the between-group variance to the total variance. A slight variation of this method plots the curvature of the within group variance. The method can be traced to speculation by Robert L. Thorndike in 1953.

Information Criterion Approach
Another set of methods for determining the number of clusters are information criteria, such as the Akaike information criterion (AIC), Bayesian information criterion (BIC), or the Deviance information criterion (DIC) &mdash; if it is possible to make a likelihood function for the clustering model. For example: The k-means model is "almost" a Gaussian mixture model and one can construct a likelihood for the Gaussian mixture model and thus also determine information criterion values.

=== An Information Theoretic Approach ===

Ideas from a sub-field of electrical engineering known as rate distortion theory have been applied to formulate an algorithm for choosing k called the "jump" method, which determines the number of clusters that maximizes efficiency while minimizing error by information theoretic standards. The strategy of the algorithm is to generate a distortion curve for the input data by running a standard clustering algorithm such as k-means for all values of k between 1 and n, and computing the distortion (described below) of the resulting clustering. The distortion curve is then transformed by a negative power chosen based on the dimensionality of the data. Jumps in the resulting values then signify reasonable choices for k, with the largest jump representing the best choice.

The distortion of a clustering of some input data is formally defined as follows: Let the data set be modeled as a p-dimensional random variable, X, consisting of a mixture distribution of G components with common covariance, $$ \Gamma $$. If we let $$ c_1 ... c_K $$ be a set of K cluster centers, with $$ c_x $$ the closest center to a given sample of X, then the minimum average distortion per dimension when fitting the K centers to the data is:

$$ d_K = \frac{1}{p} \min_{c_1 ... c_K}{E[(X - c_x)^T\Gamma^{-1}(X - c_x)]} $$

This is also the average Mahalanobis distance per dimension between X and the set of cluster centers C. Because the minimization over all possible sets of cluster centers is prohibitively complex, the distortion is computed in practice by generating a set of cluster centers using a standard clustering algorithm and computing the distortion using the result.

The pseudo-code for the jump method with an input set of p-dimensional data points X is:

The choice of the transform power $$ Y = (p/2) $$ is motivated by asymptotic reasoning using results from rate distortion theory. Let the data X have a single, arbitrarily p-dimensional Gaussian distribution, and let fixed K = floor($$\alpha^p$$), for some $$\alpha$$ greater than zero. Then the distortion of a clustering of K clusters in the limit as p goes to infinity is $$ \alpha^{-2} $$. It can be seen that asymptotically, the distortion of a clustering to the power $$(-p/2)$$ is proportional to $$\alpha^p$$, which by definition is approximately the number of clusters K. In other words, for a single Gaussian distribution, increasing K beyond the true number of clusters, which should be one, causes a linear growth in distortion. This behavior is important in the general case of a mixture of multiple distribution components.

Let X be a mixture of G p-dimensional Gaussian distributions with common covariance. Then for any fixed K less than G, the distortion of a clustering as p goes to infinity is infinite. Intuitively, this means that a clustering of less than the correct number of clusters is unable to describe asymptotically high-dimensional data, causing the distortion to increase without limit. If, as described above, K is made an increasing function of p, namely, K = floor($$\alpha^p$$), the same result as above is achieved, with the value of the distortion in the limit as p goes to infinity being equal to $$\alpha^{-2}$$. Correspondingly, there is the same proportional relationship between the transformed distortion and the number of clusters, K.

Putting the results above together, it can be seen that for sufficiently high values of p, the transformed distortion $$d_K^{-p/2}$$ is approximately zero for K < G, then jumps suddenly and begins increasing linearly for K >= G. The jump algorithm for choosing K makes use of these behaviors to identify the most likely value for the true number of clusters.

Although the mathematical support for the method is given in terms of asymptotic results, the algorithm has been empirically verified to work well in a variety of data sets with reasonable dimensionality. In addition to the localized jump method described above, there exists a second algorithm for choosing K using the same transformed distortion values known as the broken line method. The broken line method identifies the jump point in the graph of the transformed distortion by doing a simple least squares error line fit of two line segments, which in theory will fall along the x-axis for K < G, and along the linearly increasing phase of the transformed distortion plot for K >= G. The broken line method is more robust than the jump method in that its decision is global rather than local, but it also relies on the assumption of Gaussian mixture components, whereas the jump method is fully non-parametric and has been shown to be viable for general mixture distributions.

Choosing k Using the Silhouette
The average silhouette of the data is another useful criterion for assessing the natural number of clusters. The silhouette of a datum is a measure of how closely it is matched to data within its cluster and how loosely it is matched to data of the neighbouring cluster, i.e. the cluster whose average distance from the datum is lowest. A silhouette close to $$1$$ implies the datum is in an appropriate cluster, whilst a silhouette close to $$-1$$ implies the datum is in the wrong cluster. Optimization techniques such as genetic algorithms are useful in determining the number clusters that gives rise to the largest silhouette.