Due to engineering limitations, the spatial encoding gradient fields produced by an MRI scanner are never perfectly linear. Gradient non-ideality is typically associated with image geometric distortion, but it also imparts spatially varying bias in the signal generated during gradient-based motion encoding. In this work, we theoretically investigate how motion encoding gradient nonlinearity affects MR elastography and develop a corrective strategy applicable to any MRE protocol.
In a standard scan, the spatial encoding field at position $$$\vec{r}=x\vec{i}+y\vec{j}+z\vec{k}$$$ is conventionally modeled as
$$B(\vec{r},t) = S_{X}(\vec{r})G_{X}(t) + S_{Y}(\vec{r})G_{Y}(t) + S_{Z}(\vec{r})G_{Z}(t) = \mathbf{G}(t)^{T}\mathbf{S}(\vec{r})~[EQ1]$$
where $$$G_{D}(t)$$$ is the (normalized) gradient waveform for direction $$$D$$$, and $$$S_{D}$$$ is the coil spatial response function, modeled as a low-order spherical harmonic expansion7. $$$S_{D}$$$ ideally varies linearly and only within its nominal dimension (e.g., $$$S_{X}(\vec{r})=x$$$); however, in practice, fields vary nonlinearly and in all directions.
Presuming [EQ1], the $$$n^{th}$$$ k-space measurement is modeled as
$$g[n]=\int_{\Omega}m_{0}(\vec{r})e^{-j\phi(\vec{r})}e^{-j\mathbf{k}[n]^{T}\mathbf{S}(\vec{r})}d\vec{r}~[EQ2]$$
where $$$m_{0}$$$ is spin density, $$$\mathbf{k}[n]$$$ is the k-space vector (i.e., time-integral of $$$\mathbf{G}(t)$$$ during readout ($$$t\geq{\Delta}$$$)), and $$$\phi(\vec{r})$$$ is motion encoded phase, the target quantity in MRE. The phase-modulated image $$$\hat{m}_{0}(\vec{r})=m_{0}(\vec{r})e^{-j\phi(\vec{r})}$$$ can be estimated by interpolating8 the inverse Fourier transform of $$$g$$$ or model-based reconstruction9, from which $$$\phi(\vec{r})$$$ can be extracted.
In MRE, spins move harmonically as $$$\vec{\mu}(\vec{r},t)=\vec{\mu}(\vec{r},0)+\mathrm{Re}\left\{\vec{\eta}_{0}(\vec{r})\exp\left(j\left(\zeta(\vec{r})-\omega{t}+\alpha\right)\right)\right\}$$$, where $$$\vec{\mu}(\vec{r},0)$$$, $$$\vec{\eta}_{0}(\vec{r})$$$, $$$\zeta(\vec{r})$$$, $$$\omega$$$, and $$$\alpha$$$ are peak displacement, instantaneous wave frequency, mechanical driving frequency, and phase delay, respectively. For moving spins, $$$S_{D}(\cdot)$$$ can be approximated (about $$$\vec{r}_{0}$$$) as $$$\mathbf{S}(\vec{\mu}(\vec{r},t))\approx\mathbf{S}(\vec{r}_{0})+\mathcal{J}_\mathbf{S}(\vec{r}_{0})\left(\vec{\mu}(\vec{r},t)-\vec{r}_{0}\right)$$$, where $$$\mathcal{J}_\mathbf{S}(\cdot)$$$ is the Jacobian of the field vector. After simplification, it follows that
$$\phi(\vec{r})\approx-\gamma\mathbf{A}^{T}\left(\mathbf{I}_{2\times{2}}\otimes\mathcal{J}_\mathbf{S}(\vec{r}_{0})\right)\left[\begin{array}{c}\vec{\eta}_{0}(\vec{r})\cos\left(\zeta(\vec{r})\right)\\\vec{\eta}_{0}(\vec{r})\sin\left(\zeta(\vec{r})\right)\end{array}\right]~[EQ3],$$
where $$$\mathcal{F}_\mathbf{G}(\cdot)$$$ is the MEG Fourier transform, $$$\otimes$$$ is Kronecker's product, and
$$\mathbf{A}_{p}=\left[\begin{array}{cc}+\mathrm{Re}\left\{\exp\left(j\alpha\right)\mathcal{F}_\mathbf{G}(\omega)\right\}\\-\mathrm{Im}\left\{\exp\left(j\alpha\right)\mathcal{F}_\mathbf{G}(\omega)\right\}\end{array}\right]~[EQ4].$$
Considering an MRE exam with $$$S$$$ scans (i.e., different MEG directions/offsets), the gradient nonlinearity-corrected first harmonic is estimated via pseudo-inversion ($$$\dagger$$$) as
$$\left[\begin{array}{c}\vec{\eta}_{0}(\vec{r})\cos\left(\zeta(\vec{r})\right)\\\vec{\eta}_{0}(\vec{r})\sin\left(\zeta(\vec{r})\right)\end{array}\right]\approx -\frac{1}{\gamma}\left(\left[\begin{array}{c}\mathbf{A}_{0}^{T} \\\mathbf{A}_{1}^{T} \\\vdots\\\mathbf{A}_{S-1}^{T} \\\end{array}\right]\left(\mathbf{I}_{2\times{2}}\otimes\mathcal{J}_\mathbf{S}(\vec{r}_{0})\right)\right)^{\dagger}\left[\begin{array}{c}\phi_{0}(\vec{r}) \\\phi_{1}(\vec{r}) \\\vdots \\\phi_{S-1}(\vec{r}) \\\end{array}\right]~[EQ5].$$
For MRE, $$$\vec{r}_{0} = \vec{r}$$$ is recommended. [EQ5] applies to any MRE sequence3,10,11,12. However, when MEGs are applied mono-directionally3 for $$$C$$$ cycles with (pseudo-)sinusoidal gradients at amplitude $$$\|\mathbf{G}_{0}\|_{2}$$$, [EQ5] simplifies to
$$\vec{\delta}(\vec{r},n) \approx -\frac{\omega}{\gamma\pi C \left\|\mathbf{G}_{0}\right\|_{2}}\mathcal{J}_\mathbf{S}(\vec{r}_{0})^{\dagger}\left[\begin{array}{c}\phi_{0}(\vec{r}) \\\phi_{1}(\vec{r}) \\\vdots \\\phi_{S-1}(\vec{r}) \\\end{array}\right]~[EQ6],$$
where $$$\vec{\delta}(\vec{r},n)=\vec{\eta}_{0}(\vec{r})\cos\left(\zeta(\vec{r})-\frac{2\pi n}{N}\right)$$$ is the displacement vector at offset $$$n\in[0,N)$$$. Hence, in most cases, MRE phase data (pre- or -post subtraction) can be corrected prior to first harmonic estimation.
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