I. T. Maatman1, S. Ypma1, M. Kachelrieß2, Y. Berker2, K. T. Block3, E. Van der Bijl1, J. J. Hermans1, M. C. Maas1, and T. W. J. Scheenen1
1Radboud University Medical Centre, Nijmegen, Netherlands, 2German Cancer Research Center (DKFZ), Heidelberg, Germany, 3NYU Langone Medical Center, New York, NY, United States
Synopsis
Motion-compensated images can be created from motion-binned undersampled radial stack-of-stars data through compressed sensing and image registration. However, for long repetition times or for many partitions, the acquisition time for one radial projection with all phase-encode steps becomes too long to sample the motion via self-gating, which leads to motion artifacts. Therefore, we estimate motion from FID-navigators and perform binning on a single-readout level to gain higher spatiotemporal resolutions. Our methods are tested on a motion phantom and volunteer with gridding and motion-compensated reconstructions. Our results show accurate detection of the motion signal and reduced motion blur in reconstructions.
Introduction
MRI of the thorax is challenging, as respiratory motion can induce blurring or ghosting artifacts.1 Breath-holding limits acquisition times to approximately 15 s, precluding high spatial resolutions over large fields-of-view.
Radial sampling schemes are inherently motion robust.2 Furthermore, if golden-angle reordering is used, radial MR data can be retrospectively gated into multiple motion states according to a motion signal.3 A common method to extract the motion signal is to collect the data near the k-space center for projections of the total signal in the imaged volume at every $$$\Delta t = N_p\,T_R$$$, where $$$N_p$$$ is the number of partitions and $$$T_R$$$ is the repetition time.3-6 According to the Nyquist criterion, the detectable respiratory frequency in this case is limited to $$$f_s = 1/(2\,N_p\,T_R)$$$. For longer $$$T_R$$$, or many partitions, the acquisition time for a full stack of partitions per radial projection becomes too long to faithfully sample the motion, leading to temporal aliasing and motion blur when binning k-space data into different motion states.
We lift this restriction by acquiring a short free-induction decay (FID) navigator at every $$$T_R$$$, allowing single-readout binning (SRB) of the data into motion states, resolving motion frequencies up to $$$1/(2\,T_R)$$$. We test our method on a motion phantom and a normal breathing volunteer, reconstructing the data with a non-uniform fast Fourier transform (NUFFT) and an adapted version of the 4D motion-compensated high-dimensional total variation (MoCo-HDTV) algorithm, which is a framework for joint reconstruction and motion estimation for undersampled radial data.6Methods
We acquired data of a motion phantom (Quasar MRI 4D, Modus QA, London, Canada) and volunteer with a golden-angle radial stack-of-stars spoiled gradient echo sequence7 (Table 1) on a 3-T MR system (Prisma-Fit, Siemens Healthineers, Erlangen, Germany). The phantom contained a central oscillating gel-filled cylinder. Maximum peak-to-peak translation was set to 3 cm and the frequency of the breathing-like motion pattern was approximately 0.25 Hz. $$$T_R$$$ and $$$N_p$$$ were chosen such that spoke angle binning (SAB), which includes all phase-encode steps per spoke orientation, was expected to lead to inaccurate motion estimates. We sampled 32 FID acquisition points in 200 µs between excitation and phase-encoding gradient as a navigator. For each spoke angle, all partitions were sampled in random order before moving to the next angle to ensure a more evenly distributed number of readouts in each partition and respiratory phase (Fig. 1).
Respiratory motion signals were extracted as the first principal components of principal component analyses of the FID navigators and of the nine central points of every gradient-echo readout.6 We calculated the correlation coefficients of the FID and gradient-echo motion signals with the reference signal of the phantom. We reconstructed the data both with NUFFTs and via an adapted version of the MoCo-HDTV algorithm.6
To compare SAB and SRB independent of the method of motion detection, we created reconstructions for SAB with the means of the FID navigators across the partitions as the motion signal, since $$$Δt$$$ was too long to detect respiratory motion from the k-space center.Results and Discussion
The FID motion signal shows a clear correspondence to the motion pattern imposed on the phantom, indicating that the rigid motion during acquisition was accurately extracted from the FID navigators (Fig. 2). Meanwhile, the gradient-echo motion signal is clearly aliased (Fig. 2). Calculated correlation coefficients of the FID and gradient-echo motion signals with respect to the reference equaled 0.98 and 0.26, respectively.
SRB resulted in reduced motion blur in NUFFT reconstructions of the phantom data, and in higher through-plane incoherence of undersampling artifacts, which may be advantageous for compressed sensing reconstructions (Fig. 3).8
Figure 3 also shows comparisons of the MoCo-HDTV reconstructions for the phantom data again at end-exhalation, which greatly reduce the level of undersampling artifacts, although at the cost of slight motion blur. However, SRB, in comparison to SAB, leads to an increase of the effective spatial resolution by reducing motion blur between slices. Using SRB combined with MoCo-HDTV reconstruction on in vivo data leads to a sharp depiction of anatomical structures in the thorax and abdomen at high spatial resolution (Fig. 4).Conclusion
We showed first results for the acquisition and reconstruction of radial stack-of-stars data where the temporal resolutions for motion detection and reconstruction are increased through FID navigators and single-readout binning. Images of a moving phantom and a volunteer show reduced motion blur, and more incoherent and less prominent streaking artifacts, allowing the detection of small anatomical structures in the upper abdomen in a free-breathing acquisition.Acknowledgements
We thank C. Schneider and U. Van der Heide of the Netherlands Cancer Institute (NKI) for providing the Quasar phantom. References
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