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Probabilistic ICA model

Similar to the square noise-free case, the probabilistic ICA model is formulated as a generative linear latent variables model. It is characterised by assuming that the $ p$-variate vector of observations is generated from a set of $ q$ statistically independent non-Gaussian sources via a linear instantaneous mixing process corrupted by additive Gaussian noise $ \eta$$ (t)$:

$\displaystyle \mbox{\protect\boldmath$x$}$$\displaystyle _i=$$\displaystyle \mbox{\protect\boldmath$A$}$$\displaystyle \mbox{\protect\boldmath$s$}$$\displaystyle _i+$$\displaystyle \mbox{\protect\boldmath$\mu$}$$\displaystyle +$$\displaystyle \mbox{\protect\boldmath$\eta$}$$\displaystyle _i\qquad \forall i\in{\cal V}.$ (2)

Here, $ x$$ _i$ denotes the $ p$-dimensional column vector of individual measurements at voxel location $ i$, $ s$$ _i$ denotes the $ q$- dimensional column vector of non-Gaussian source signals contained in the data and $ \eta$$ _i$ denotes Gaussian noise $ \eta$$ _i \sim {\cal
N}(0,\sigma^2\mbox{\protect\boldmath $\Sigma$}_i)$. We assume that $ q<p$, i.e. that there are fewer source processes than observations in time. The covariance of the noise is allowed to be voxel dependent in order to allow for the vastly different noise covariances observed in different tissue types [Woolrich et al., 2001].

The vector $ \mu$ defines the mean of the observations $ x$$ _i$ where the index $ i$ is over the set of all voxel locations $ {\cal V}$ and the $ p\times q$ matrix $ A$ is assumed to be non-degenerate, i.e. of rank $ q$. Solving the blind separation problem requires finding a linear transformation matrix $ W$ such that

$\displaystyle \widehat{\mbox{\protect\boldmath$s$}} = \mbox{\protect\boldmath$W$}\mbox{\protect\boldmath$x$}$

is a good approximation to the true source signals $ s$.

The PICA model is similar to the standard GLM with the difference that, unlike the design matrix in the GLM, the mixing matrix $ A$ is no longer pre-specified prior to model fitting but will be estimated from the data as part of the model fitting. The spatial source signals correspond to parameter estimates in the GLM with the additional constraint of being statistically independent.

The model of equation 2 is closely related to Factor Analysis (FA) [Bartholomew, 1987]. There, the sources are assumed to have a Gaussian distribution and the noise is assumed to have a diagonal covariance matrix. In Factor Analysis, the sources are known as common factors and $ \eta$ is a vector of random variables called specific factors. In FA the assumption of independence between the individual source processes reduces to assuming that sources are mutually uncorrelated.

next up previous
Next: Uniqueness Up: tr02cb1 Previous: Introduction
Christian F. Beckmann 2003-08-05