Oliver C. Kiersnowski1, Anita Karsa1, John S. Thornton2, and Karin Shmueli1
1Department of Medical Physics and Biomedical Engineering, University College London, London, United Kingdom, 2UCL Queens Square Institute of Neurology, London, United Kingdom
Synopsis
Quantitative susceptibility
mapping (QSM) using the MRI phase to calculate tissue magnetic susceptibility
is finding increasing clinical applications. Oblique image slices are often
acquired to facilitate radiological viewing and reduce artifacts. Here, we show
that artifacts and errors arise in susceptibility maps if oblique acquisition
is not properly taken into account in QSM. We performed a comprehensive
analysis of the effects of oblique acquisition on brain susceptibility maps and
compared tilt correction schemes for three susceptibility calculation methods, using
a numerical phantom and human in-vivo images. We demonstrate a robust tilt
correction method for accurate QSM with oblique acquisition.
Introduction
Quantitative susceptibility
mapping (QSM) is finding increasing clinical applications.
Acquisition of oblique image slices is common clinical practice to facilitate
radiological viewing but pilot studies suggest this gives incorrect
susceptibility ($$$\chi$$$) estimates when unaccounted
for1. Using a numerical brain phantom2, we performed a
comprehensive analysis of the effects of oblique acquisition and compared
proposed tilt correction methods for the final $$$\chi$$$ calculation step in the QSM pipeline. We
confirmed these results in vivo, and demonstrate a robust tilt correction method for accurate $$$\chi$$$ calculation.Methods
Numerical Phantom:
Local field maps were
obtained from a non-linear fit
3 over echo times of complex data, created from magnitude and phase images of a numerical brain phantom
2, with no
background fields. These background-field-free maps were used to independently
analyse the $$$\chi$$$ calculation step in the QSM pipeline without
confounds from phase unwrapping or background field removal. To simulate oblique slice acquisition, the untilted
reference local field map (at 0°) was tilted
by -45° to +45° in 5° steps. All rotations were carried out about
the
x-axis (
u-axis, Figure 1) using FSL
FLIRT
4 with trilinear interpolation.
We tested four proposed tilt
correction schemes (Figure 1):
- RotPrior: image
rotated into scanner frame prior to $$$\chi$$$ calculation (with a k-space
dipole defined in the scanner frame)
- DipK: image
left unaligned (k-space dipole defined in the tilted image frame)
- DipIm: image
left unaligned (image-space dipole defined in the tilted image frame)
- NoRot: image
left unaligned (simulating mistaken definition of the k-space
dipole in the scanner frame misaligned to the tilted image)
To facilitate comparisons,
all susceptibility maps left in the image-frame after correction (
DipK,
DipIm
and
NoRot) were rotated back into alignment with the scanner axes. These
schemes were compared for three $$$\chi$$$ calculation methods:
thresholded
k-space division (TKD)
5 (threshold = 2/3), iterative
fitting with Tikhonov regularisation
6,7 (α =
0.003), both corrected for $$$\chi$$$ underestimation
8, and weighted linear
total variation (wlTV) regularisation (FANSI toolbox
9,10, α =2x10
-4 ). Mean $$$\chi$$$ values were calculated in five deep grey
matter regions of interest (ROIs) provided with the phantom. Susceptibility
maps were compared using the root mean squared error (RMSE) relative to the
ground truth susceptibility map and the QSM-tuned structural similarity index (XSIM)
11.
In Vivo:
3D gradient-echo brain images
of a healthy volunteer were acquired on a 3T Siemens Prisma MR system (National
Hospital for Neurology and Neurosurgery, London, UK) using a 64-channel head
coil. The image volume was tilted about the
x-axis from -20° to +20° in 5°
increments and acquired in 3 min 23 s (per volume) with TE1/ΔTE/TE5 = 4.92/4.92/24.60ms; TR=30ms; 1.23 mm isotropic voxels; 6/8 partial Fourier; and GRAPPA
PE
acceleration = 3.
For all angles/volumes, a
total field map and noise map were obtained using a non-linear fit of the
complex data
3. A brain mask was created using BET
12,13,
eroded by 6 voxels, and multiplied with a mask created by thresholding the
inverse noise map at its mean to remove noisy voxels. Residual phase wraps were
removed using Laplacian unwrapping
13,14 and background fields were
removed using the Laplacian boundary value (LBV)
13,15 technique as
it is independent of tilt angle. The four tilt correction schemes were compared
using the same three $$$\chi$$$ calculation methods as for the numerical
phantom.
For each angle, the magnitude
image (RMS across echoes) was rigidly registered to the reference (0°) using NiftyReg
16 and the transformation matrix was used to transform
the $$$\chi$$$ maps into the reference space for comparison. ROIs
were obtained by registering the EVE
17 magnitude image with the same reference image and applying the resulting transformation to the EVE
ROIs. Mean $$$\chi$$$ values were calculated in these ROIs for all angles. RMSE and XSIM were also used to compare tilt-corrected maps with
the 0° reference susceptibility map.
Results
Numerical Phantom:
All QSM methods are most
accurate with RotPrior, and least accurate with NoRot when the
dipole is misaligned to the main magnetic field (Figure 2). wlTV is relatively
robust to oblique acquisition, with RotPrior and DipK performing similarly.
However, DipK shows variability in $$$\chi$$$ across angles in different ROIs. $$$\chi$$$ maps (Figure 3) make clearly apparent the
errors resulting from NoRot.
In Vivo:
Figure 4 confirms that
NoRot results in large susceptibility errors and that RotPrior is
comparable to DipK between $$$\pm$$$20°, both performing better
than DipIm, in agreement with the
phantom results. Difference images also
confirm the phantom results (Figure 5). Subtle effects found
in the phantom ROIs (Figure 2) were not apparent in vivo (not shown) due
to noise, motion, rotation/registration interpolation effects and the expected
variability in QSMs over repeated acquisitions18. Conclusions
We have shown that, for any susceptibility calculation method (TKD,
iterative Tikhonov and wlTV) applied to an oblique acquisition, leaving the
dipole kernel misaligned with the main magnetic field ($$$\mathbf{\hat{B}}_0$$$) direction, which is often the default mode of QSM
toolboxes, leads to substantial $$$\chi$$$ errors. The
most accurate susceptibilities can be obtained when local field maps are rotated
into alignment with the scanner axes prior to $$$\chi$$$ calculation (RotPrior). For wlTV, accurate susceptibility calculation can be
carried out in the tilted image frame without any rotations provided the
correct ($$$\mathbf{\hat{B}}_0$$$) direction is
used in defining the k-space dipole (DipK). Acknowledgements
Oliver Kiersnowski is supported by the EPSRC-funded UCL Centre for Doctoral Training in
Intelligent, Integrated Imaging in Healthcare (i4health) (EP/S021930/1). Karin
Shmueli is supported by ERC Consolidator Grant DiSCo MRI SFN 770939. We thank Dr Carlos Milovic for his assistance with FANSI.References
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