Principal components analysis

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Principal components analysis (PCA) is a technique used to reduce multidimensional data sets to lower dimensions for analysis. Depending on the field of application, it is also named the discrete Karhunen-Loève transform, the Hotelling transform or proper orthogonal decomposition (POD).

PCA is mostly used as a tool in exploratory data analysis and for making predictive models. PCA involves the calculation of the eigenvalue decomposition or Singular value decomposition of a data set, usually after mean centering the data for each attribute. The results of a PCA are usually discussed in terms of component scores and loadings.

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PCA is mathematically defined as an orthogonal linear transformation that transforms the data to a new coordinate system such that the greatest variance by any projection of the data comes to lie on the first coordinate (called the first principal component), the second greatest variance on the second coordinate, and so on. PCA is theoretically the optimum transform for a given data in least square terms.

PCA can be used for dimensionality reduction in a data set by retaining those characteristics of the data set that contribute most to its variance, by keeping lower-order principal components and ignoring higher-order ones. Such low-order components often contain the "most important" aspects of the data. However, depending on the application this may not always be the case.

For a data matrix, XT, with zero empirical mean (the empirical mean of the distribution has been subtracted from the data set), where each row represents a different repetition of the experiment, and each column gives the results from a particular probe, the PCA transformation is given by:

\mathbf{Y^T}=\mathbf{X^T}\mathbf{W}
 = \mathbf{V}\mathbf{\Sigma}

where V Σ WT is the singular value decomposition (svd) of XT.

In this article we shall adopt the other convention, so that each column is made up of results for a different subject, and each row the results from a different probe. This will mean that the PCA for our data matrix X will be given by:

\mathbf{Y}=\mathbf{W}^T\mathbf{X}
 = \mathbf{\Sigma}\mathbf{V^T}

where W Σ VT is the svd of X.

PCA has the distinction of being the optimal linear transformation for keeping the subspace that has largest variance. This advantage, however, comes at the price of greater computational requirement if compared, for example, to the discrete cosine transform. Unlike other linear transforms, PCA does not have a fixed set of basis vectors. Its basis vectors depend on the data set.

Assuming zero empirical mean (the empirical mean of the distribution has been subtracted from the data set), the principal component w1 of a data set x can be defined as:

\mathbf{w}_1
 = \arg\max_{\Vert \mathbf{w} \Vert = 1} \operatorname{var}\{ \mathbf{w}^T \mathbf{x} \}
 = \arg\max_{\Vert \mathbf{w} \Vert = 1} E\left\{ \left( \mathbf{w}^T \mathbf{x}\right)^2 \right\}

(See arg max for the notation.) With the first k − 1 components, the k-th component can be found by subtracting the first k − 1 principal components from x:

\mathbf{\hat{x}}_{k - 1}
 = \mathbf{x} -
 \sum_{i = 1}^{k - 1}
 \mathbf{w}_i \mathbf{w}_i^T \mathbf{x}

and by substituting this as the new data set to find a principal component in

\mathbf{w}_k
 = \arg\max_{\Vert \mathbf{w} \Vert = 1} E\left\{
 \left( \mathbf{w}^T \mathbf{\hat{x}}_{k - 1}
 \right)^2 \right\}.

The Karhunen-Loève transform is therefore equivalent to finding the singular value decomposition of the data matrix X,

\mathbf{X}=\mathbf{W}\mathbf{\Sigma}\mathbf{V}^T,

and then obtaining the reduced-space data matrix Y by projecting X down into the reduced space defined by only the first L singular vectors, WL:

\mathbf{Y}=\mathbf{W_L}^T\mathbf{X} = \mathbf{\Sigma_L}\mathbf{V_L}^T

The matrix W of singular vectors of X is equivalently the matrix W of eigenvectors of the matrix of observed covariances C = X XT,

\mathbf{X}\mathbf{X}^T = \mathbf{W}\mathbf{\Sigma}\mathbf{\Sigma}^T\mathbf{W}^T

The eigenvectors with the largest eigenvalues correspond to the dimensions that have the strongest correlation in the data set (see Rayleigh quotient).

PCA is equivalent to empirical orthogonal functions (EOF).

An autoencoder neural network with a linear hidden layer is also equivalent to PCA. Upon convergence, the weight vectors of the K neurons in the hidden layer will form a basis for the space spanned by the first K principal components. Unlike PCA, this technique will not necessarily produce orthogonal vectors.

PCA is a popular technique in pattern recognition. But it is not optimized for class separability[1]. An alternative is the linear discriminant analysis, which does take this into account. PCA optimally minimizes reconstruction error under the L2 norm.

Symbol Meaning Dimensions Indices
\mathbf{X} = \{ X[m,n] \} data matrix, consisting of the set of all data vectors, one vector per column  M \times N  m = 1 \ldots M
 n = 1 \ldots N
N \, the number of column vectors in the data set 1 \times 1 scalar
M \, the number of elements in each column vector (dimension) 1 \times 1 scalar
L \, the number of dimensions in the dimensionally reduced subspace,  1 \le L \le M 1 \times 1 scalar
\mathbf{u} = \{ u[m] \} vector of empirical means, one mean for each row m of the data matrix  M \times 1  m = 1 \ldots M
\mathbf{s} = \{ s[m] \} vector of empirical standard deviations, one standard deviation for each row m of the data matrix  M \times 1  m = 1 \ldots M
\mathbf{h} = \{ h[n] \} vector of all 1's  1 \times N  n = 1 \ldots N
\mathbf{B} = \{ B[m,n] \} deviations from the mean of each row m of the data matrix  M \times N  m = 1 \ldots M
 n = 1 \ldots N
\mathbf{Z} = \{ Z[m,n] \} z-scores, computed using the mean and standard deviation for each row m of the data matrix  M \times N  m = 1 \ldots M
 n = 1 \ldots N
\mathbf{C} = \{ C[p,q] \} covariance matrix  M \times M  p = 1 \ldots M
 q = 1 \ldots M
\mathbf{R} = \{ R[p,q] \} correlation matrix  M \times M  p = 1 \ldots M
 q = 1 \ldots M
 \mathbf{V} = \{ V[p,q] \} matrix consisting of the set of all eigenvectors of C, one eigenvector per column  M \times M  p = 1 \ldots M
 q = 1 \ldots M
\mathbf{D} = \{ D[p,q] \} diagonal matrix consisting of the set of all eigenvalues of C along its principal diagonal, and 0 for all other elements  M \times M  p = 1 \ldots M
 q = 1 \ldots M
\mathbf{W} = \{ W[p,q] \} matrix of basis vectors, one vector per column, where each basis vector is one of the eigenvectors of C, and where the vectors in W are a sub-set of those in V  M \times L  p = 1 \ldots M
 q = 1 \ldots L
\mathbf{Y} = \{ Y[m,n] \} matrix consisting of N column vectors, where each vector is the projection of the corresponding data vector from matrix X onto the basis vectors contained in the columns of matrix W.  L \times N  m = 1 \ldots L
 n = 1 \ldots N

PCA is theoretically the optimal linear scheme, in terms of least mean square error, for compressing a set of high dimensional vectors into a set of lower dimensional vectors and then reconstructing the original set. It is a non-parametric analysis and the answer is unique and independent. PCA compression and decompression are easy operations to perform given the model parameters. However, the latter two properties are regarded as weakness as well as strength, in that being non-parametric, no a-priori assumptions can be incorporated and that PCA compressions often incur loss of information.

When used for clustering, the main limitation of PCA is that it does not consider class separability since it does not take into account the class label of the feature vector. PCA simply performs a coordinate rotation that aligns the transformed axes with the directions of maximum variance. There is no guarantee that the directions of maximum variance will contain good features for discrimination.

Apart from that, it must be addressed that several assumptions[2] were made in the process of reaching the result of PCA, thus limiting the application of PCA. These assumptions can be briefly listed as:

  • Assumption on Linearity

We assumed the observed data set to be linear combinations of certain basis. Non-linear methods such as kernel PCA are developed without assuming linearity.

  • Assumption that principal components are orthogonal

We assumed that principal components are orthogonal with each other. Methods such as ICA(Independent Component Analysis) are developed to address this limitation.

  • Assumption on the statistical importance of mean and covariance

PCA uses the eigenvectors of the covariance matrix and it only finds the independent axes of the data under the Gaussian assumption. For non-Gaussian or multi-modal Gaussian data, PCA simply de-correlates the axes. When used for clustering, the main limitation of PCA is that it does not consider class separability since it does not take into account the class label of the feature vector.

  • Assumption that large variances have important dynamics

PCA simply performs a coordinate rotation that aligns the transformed axes with the directions of maximum variance. It is only when we believe that the observed data has a high Signal-Noise Ratio, can we reach the result that principle components with larger variance corresponds to interesting dynamics and lower ones corresponds to noise. There is no guarantee that the directions of maximum variance will contain good features for discrimination.

Essentially, PCA evolved only rotation and scaling. The above assumptions are made rather in order to simplify the algebraic computation on the data set. Some other methods are developed without assuming one or some of them, and are briefly discussed in the following.

Following is a detailed description of PCA using the covariance method. The goal is to transform a given data set X of dimension M to an alternative data set Y of smaller dimension L. Equivalently, we are seeking to find the matrix Y, where Y is the Karhunen-Loeve transform (KLT) of matrix X:

 \mathbf{Y} = \mathbb{KLT} \{ \mathbf{X} \}

Suppose you have data comprising a set of observations of M variables, and you want to reduce the data so that each observation can be described with only L variables, L < M. Suppose further, that the data are arranged as a set of N data vectors \mathbf{x}_1 \ldots \mathbf{x}_N with each \mathbf{x}_n representing a single grouped observation of the M variables.

  • Write \mathbf{x}_1 \ldots \mathbf{x}_N as column vectors, each of which has M rows.
  • Place the column vectors into a single matrix X of dimensions M × N.

  • Find the empirical mean along each dimension m = 1...M.
  • Place the calculated mean values into an empirical mean vector u of dimensions M × 1.
u[m] = {1 \over N} \sum_{n=1}^N X[m,n]

  • Subtract the empirical mean vector u from each column of the data matrix X.
  • Store mean-subtracted data in the M × N matrix B.
\mathbf{B} = \mathbf{X} - \mathbf{u} \cdot \mathbf{h}
where h is a 1 x N row vector of all 1's:
h[n] = 1 \, \qquad \qquad \mathrm{for \ } n = 1 \ldots N

  • Find the M × M empirical covariance matrix C from the outer product of matrix B with itself:
\mathbf{C} = \mathbb{ E } \left[ \mathbf{B} \otimes \mathbf{B} \right] = \mathbb{ E } \left[ \mathbf{B} \cdot \mathbf{B}^{*} \right] = { 1 \over N } \mathbf{B} \cdot \mathbf{B}^{*}
where
\mathbb{E} is the expected value operator,
 \otimes is the outer product operator, and
 * \ is the conjugate transpose operator. Note that if B consists entirely of real numbers, which is the case in many applications, the "conjugate transpose" is the same as the regular transpose.
  • Please note that the information in this section is indeed a bit fuzzy. See the covariance matrix sections on the discussion page for more information.

\mathbf{V}^{-1} \mathbf{C} \mathbf{V} = \mathbf{D}
where D is the diagonal matrix of eigenvalues of C. This step will typically involve the use of a computer-based algorithm for computing eigenvectors and eigenvalues. These algorithms are readily available as sub-components of most matrix algebra systems, such as MATLAB, Mathematica, SciPy, or IDL(Interactive Data Language). See, for example, the eig function.
D[p,q] = \lambda_m \qquad \mathrm{for} \qquad p = q = m
is the mth eigenvalue of the covariance matrix C, and
D[p,q] = 0 \qquad \mathrm{for} \qquad p \ne q.
  • Matrix V, also of dimension M × M, contains M column vectors, each of length M, which represent the M eigenvectors of the covariance matrix C.
  • The eigenvalues and eigenvectors are ordered and paired. The mth eigenvalue corresponds to the mth eigenvector.

  • Sort the columns of the eigenvector matrix V and eigenvalue matrix D in order of decreasing eigenvalue.
  • Make sure to maintain the correct pairings between the columns in each matrix.

  • The eigenvalues represent the distribution of the source data's energy among each of the eigenvectors, where the eigenvectors form a basis for the data. The cumulative energy content g for the mth eigenvector is the sum of the energy content across all of the eigenvectors from 1 through m:
g[m] = \sum_{q=1}^m D[p,q] \qquad \mathrm{for} \qquad p = q \qquad \mathrm{and} \qquad m = 1...M

  • Save the first L columns of V as the M × L matrix W:
 W[p,q] = V[p,q] \qquad \mathrm{for} \qquad p = 1...M \qquad q = 1...L
where
1 \leq L \leq M.
  • Use the vector g as a guide in choosing an appropriate value for L. The goal is to choose as small a value of L as possible while achieving a reasonably high value of g on a percentage basis. For example, you may want to choose L so that the cumulative energy g is above a certain threshold, like 90 percent. In this case, choose the smallest value of L such that
 g[m=L] \ge 90%

  • Create an M × 1 empirical standard deviation vector s from the square root of each element along the main diagonal of the covariance matrix C:
 \mathbf{s} = \{ s[m] \} = \sqrt{C[p,q]} \qquad \mathrm{for \ } p = q = m = 1 \ldots M
  • Calculate the M × N z-score matrix:
 \mathbf{Z} = { \mathbf{B} \over \mathbf{s} \cdot \mathbf{h} } (divide element-by-element)
  • Note: While this step is useful for various applications as it normalizes the data set with respect to its variance, it is not integral part of PCA/KLT!

  • The projected vectors are the columns of the matrix
 \mathbf{Y} = \mathbf{W}^* \cdot \mathbf{Z} = \mathbb{KLT} \{ \mathbf{X} \}.
  • The columns of matrix Y represent the Karhunen-Loeve transforms (KLT) of the data vectors in the columns of matrix X.

Editor's note: This section is currently undergoing a major revision. See page history for previous revisions.

Let X be a d-dimensional random vector expressed as column vector. Without loss of generality, assume X has zero empirical mean. We want to find a d \times d orthonormal transformation matrix P such that

\mathbf{Y} = \mathbf{P}^\top \mathbf{X}

with the constraint that

\operatorname{cov}(\mathbf{Y}) is a diagonal matrix and \mathbf{P}^{-1} = \mathbf{P}^\top.

By substitution, and matrix algebra, we obtain:


\begin{matrix}
\operatorname{cov}(\mathbf{Y}) &=& \mathbb{E}[ \mathbf{Y} \mathbf{Y}^\top]\\
\ &=& \mathbb{E}[( \mathbf{P}^\top \mathbf{X} ) ( \mathbf{P}^\top \mathbf{X} )^\top]\\
\ &=& \mathbb{E}[(\mathbf{P}^\top \mathbf{X}) (\mathbf{X}^\top \mathbf{P})] \\
\ &=& \mathbf{P}^\top \mathbb{E}[\mathbf{X} \mathbf{X}^\top] \mathbf{P} \\
\ &=& \mathbf{P}^\top \operatorname{cov}(\mathbf{X}) \mathbf{P}
\end{matrix}

We now have:


\begin{matrix}
\mathbf{P}\operatorname{cov}(\mathbf{Y}) &=& \mathbf{P} \mathbf{P}^\top \operatorname{cov}(\mathbf{X}) \mathbf{P}\\
\ &=& \operatorname{cov}(\mathbf{X}) \mathbf{P}\\
\end{matrix}

Rewrite P as d d \times 1 column vectors, so

\mathbf{P} = [P_1, P_2, \ldots, P_d]

and \operatorname{cov}(\mathbf{Y}) as:


\begin{bmatrix}
\lambda_1 & \cdots & 0 \\
\vdots & \ddots & \vdots \\
0 & \cdots & \lambda_d
\end{bmatrix}.

Substituting into equation above, we obtain:

[\lambda_1 P_1, \lambda_2 P_2, \ldots, \lambda_d P_d] =
[\operatorname{cov}(X)P_1, \operatorname{cov}(X)P_2,
\ldots, \operatorname{cov}(X)P_d].

Notice that in \lambda_i P_i = \operatorname{cov}(X)P_i, Pi is an eigenvector of X′s covariance matrix. Therefore, by finding the eigenvectors of X′s covariance matrix, we find a projection matrix P that satisfies the original constraints.


It has been shown recently [3] [4] that the relaxed solution of K-means clustering, specified by the cluster indicators, are given by the PCA principal components, and the PCA subspace spanned by the principal directions is identical to the cluster centroid subspace specified by the between-class scatter matrix.

Correspondence analysis is conceptually similar to PCA, but scales the data (which must be positive) so that rows and columns are treated equivalently. It is traditionally applied to contingency tables where Pearson's chi-square test has shown a relationship between rows and columns.

  1. ^ "Introduction to Statistical Pattern Recognition." [1]
  2. ^ Jon Shlens, A Tutorial on Principal Component Analysis
  3. ^ H. Zha, C. Ding, M. Gu, X. He and H.D. Simon. "Spectral Relaxation for K-means Clustering", Neural Information Processing Systems vol.14 (NIPS 2001). pp. 1057-1064, Vancouver, Canada. Dec. 2001.
  4. ^ Chris Ding and Xiaofeng He. "K-means Clustering via Principal Component Analysis". Proc. of Int'l Conf. Machine Learning (ICML 2004), pp 225-232. July 2004.

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