Multi-contrast image acquisitions are valuable for diagnostics but the scan time scales with the number of contrast images. Accelerated acquisitions are necessary for practical scan times and require the use of constrained reconstructions. Subspace-constraints, which constrain the multi-contrast data to lie in a low-dimensional subspace, are popularly used to reconstruct these datasets. Despite yielding good quality images at most imaging contrasts, these constraints create poor image quality at certain contrasts. We demonstrate that this is due to poor recovery of higher order subspace coefficients and present a model to enable high quality recovery of these coefficients and consequently the echo-images.
The measured data can be related to $$$\mathbf{X}_{n}$$$ as follows: $$$\mathbf{Y=E(X)}$$$ where $$$\mathbf{X}_{M \times N}$$$ ($$$M$$$ spatial pixels) is a matrix with $$$\mathbf{(X}_{n})^{N}_{n=1}$$$ as its columns. A subspace-constraint for $$$\mathbf{X}$$$ takes the following form: $$$\mathbf{X} \approx \mathbf{\alpha}_{M \times K} \mathbf{\phi}_{K \times N}$$$ where $$$\mathbf{\phi}$$$ maps the $$$K$$$-dimensional subspace coefficients $$$\mathbf{\alpha}$$$ back to the $$$N$$$-dimensional contrast space. Subspace-constrained reconstruction takes the following general form: $$\min_\alpha\frac{1}{2}||\mathbf{Y}-\mathbf{E(\alpha\phi)}||_2^2+\lambda\mathbf{R(\alpha)}$$
When no additional regularization is used, this reconstruction is the same as k-t PCA3,4. Joint-sparsity (JS) constraints were used in4 while locally low rank (LLR) regularization was used in6 to augment subspace constraints. The regularizer in the JS model is $$$\mathbf{R(\alpha)}=||D_{x}\mathbf{\alpha}||_{2,1}+||D_{y}\mathbf{\alpha}||_{2,1}$$$ where $$$D_{x}$$$ are $$$D_{y}$$$ are the horizontal and vertical finite difference operators that operate on all the subspace images and $$$||.||_{2,1}$$$ is the mixed $$$\ell_2/\ell_1$$$ norm. The LLR model uses the nuclear norm, $$$||.||_{*}$$$, as a surrogate for rank and is defined as: $$$\mathbf{R(\alpha)}=\sum_{j}||T_{j}{\alpha}||_{*}$$$ where $$$T_{j}$$$ is an operator that extracts the relaxation (subspace) signals from a small spatial patch about the spatial pixel $$$j$$$ and orders the contrast signals from the patch into a matrix.
We propose a regularization operator built on 3D block matching (BM). For a reference 3D block (3DB), the BM algorithm identifies the L-nearest 3DBs in a local neighborhood. For the ensemble of patches, the regularization operator is defined as: $$\mathbf{R(\alpha)}=\sum_{j}\sum_{k}||\Psi_{k}(\Phi(R_{j}{\alpha}))||_{*}$$
The operator $$$R_{j}({\alpha})$$$ extracts the L-nearest (in $$$\ell_2$$$ sense) 3DBs for a reference 3DB indexed by $$$j$$$ using the BM algorithm. $$$\Phi(R_{j}({\alpha}))$$$ applies a temporal transform across the extracted 3DBs. We use the SVD algorithm to allow this transform to be data driven. $$$\Psi_{k}(.)$$$ extracts the spatial patches from the $$$k^{th}$$$ coefficient dimension and orders these as columns in a matrix which are then constrained with the nuclear norm. Note that the ensemble of 3DBs and the coefficient dimension are indexed by $$$j$$$ and $$$k$$$, respectively. The BM step makes this approach a form of non-local rank (NLR) constraint on transform domain data. Therefore, the method is named NLR3D. A cartoon illustrating subspace-constraint and the working of the proposed model is presented in Figure 1.
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