The purpose of this study was to investigate the effects of spatial resolution on the performance of quantitative susceptibility mapping (QSM). The combination of magnitude contrast in spoiled gradient echo images and the voxel sensitivity function can create significant errors in the estimated B0 field map. This work evaluated the use of proton density weighted imaging and joint R2* and field map estimation to reduce the impact of imaging resolution on QSM. Our results indicate that reducing magnitude contrast in the complex-valued echo images will reduce errors in the field map estimates and, thus, the susceptibility estimates in QSM.
The effect of magnitude contrast and resolution can be demonstrated with a signal model for a voxel of a given size, based on the spoiled gradient echo (SGRE) signal at a given position ($$$r_0$$$) and echo time ($$$t$$$) as:$$s(\vec{r}_0,t)=\int{\rho(\vec{r})S_0\bigl(T_1(\vec{r}\bigr),\alpha)e^{-R_2^*(\vec{r})t}}e^{i2\pi\psi(\vec{r})t}VSF(\vec{r}-r_0)d\vec{r}\quad[1]$$where$$$\space\rho\space$$$is the proton density,$$$\space{}S_0\space$$$is the SGRE signal equation4 that varies with$$$\space{}T_1\space$$$ and flip angle$$$\space\alpha\space$$$, $$$\psi\space$$$is the field map, and$$$\space{}VSF\space$$$is the voxel sensitivity function (VSF) corresponding to the size of the voxel4. The leading magnitude terms in this expression$$$\space\bigl(\rho(\vec{r})S_0\bigl(T_1(\vec{r}\bigr),\alpha)e^{-R_2^*(\vec{r})t}\bigr)\space$$$enable spatially distant points with high magnitude to have a larger impact on the resulting complex-valued signal, than with the VSF alone. Increasing the magnitude contrast has been shown to increase QSM underestimation3. Therefore, we propose a technique to reduce the effect of magnitude contrast.
We can minimize the amplitude term in Eq. [1] by performing proton density weighted imaging instead of T1 weighted imaging, eg: utilizing small flip angles to eliminate$$$\space{}S_0\space$$$in Eq [1]. Assuming that the proton density is homogeneous in the object then we can rewrite the signal model as:
$$s(\vec{r}_0,t)\approx\int{\rho e^{i2\pi\psi^\prime(\vec{r})t}VSF(\vec{r}-r_0)d\vec{r}}\quad[2]$$
where
$$\psi^\prime(\vec{r})=\psi(\vec{r})+i\frac{R_2^*(\vec{r})}{2\pi},\quad[3]$$
and the proton density is approximated by a scalar. Estimating this complex-valued field map ($$$\psi^\prime$$$) is equivalent to joint estimation of R2* and the field map, which has the potential to reduce the effects of R2* on field map estimation. In Eq. [2] there is no magnitude weighting as a function of position, which will limit the dominant terms to those in the VSF. This produces a field map more similar to an averaged version of the original field map.
3T simulations were conducted to compare the effects of resolution on B0 field map estimation. The field map for a sphere with radius 7.5mm and homogeneous 4ppm susceptibility was created on an isotropic 0.6mm grid, with no noise and served as our high-resolution B0 field map. No R2* effects are present in this simulation, so its impact on the field map has not been included. Two sets of complex-valued echoes were generated with this field map with two homogeneous regions (object and background), and with a magnitude contrast of 10/1 (sphere/background) and 1/1.
Complex echoes were down-sampled in only the slice direction to simulate different coronal slice thicknesses (1.0mm, 1.4mm, and 1.8mm) to simulate measurement of the high-resolution B0 field map at a lower resolution. Down-sampling was performed using k-space truncation to emulate the ideal 3D VSF5. The estimated field maps were then used with the Morphology Enabled Diopole Inversion (MEDI) algorithm6 to estimate susceptibility at each slice thickness.
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