Three-dimensional radial trajectories have shown important benefits for multidimensional MR imaging of the heart. However, the performance of radial scanning approaches is sensitive even to small trajectory imperfections, which can induce significant artifacts in the reconstructed images. Here, we implemented a simple and flexible post-processing technique for trajectory inaccuracy artifact compensation that does not require any pre-scan calibration or pulse sequence modification. The technique proved effective when applied to in silico and in vitro phantom datasets, and preliminarily results suggest good feasibility in vivo for fully self-gated and motion-resolved 5D cardiac imaging.
The mismatch between nominal and acquired trajectories is schematically illustrated in Fig.1a. The deviation of a generic radial readout $$$S\left(k\right)$$$ from the theoretical path can be defined by 3 independent shifts. Here, the correction method will consider only shifts in the parallel direction, which in general can vary according to the readout direction ($$${\Delta{k}}_{R}\left(\theta,\phi\right)$$$ in 3D polar coordinates, where $$$\theta$$$ and $$$\phi$$$ are azimuthal and polar angles, Fig.1b). In the proposed method, magnitudes of all k-space readouts are individually interpolated (by cubic spline) and the peak position indices (PPI) are determined. After a weighted average over all the coil elements (where weights are proportional to the readout’s peak amplitude), each PPI is then plotted in 3D according to the angular direction of the corresponding readout, where angles $$$\theta$$$ and $$$\phi$$$ are the x- and y-axis, respectively. A locally weighted linear regression algorithm estimates the surface that best fits the obtained data cloud. Finally, the estimated parallel shifts $$$\hat{{\Delta{k}}}_{R}\left(\theta,\phi\right)$$$ are extracted from the fitted surface and applied to correct the corresponding readouts according to the equation $$$S_{\theta,\phi}^{corr}\left(k\right)=F\left\{F^{-1}\left\{S_{\theta,\phi}\left(k\right)\right\}e^{-2\pi{i}{x}\hat{\Delta{k}}_{R}\left(\theta,\phi\right)}\right\}$$$ (Fig.1c).
k-Space data for a uniform spherical object were analytically simulated according to equations in10, and artificially sampled using the same prototype golden-angle Phyllotaxis trajectory used in the subsequent scanner acquisitions (Fig.1d).11 Corrupted trajectories were simulated by shifting readouts individually in the range of values observed in the following in vitro test, i.e. $$${\Delta{k}}_{R}\left(\theta,\phi\right)=\left[0,1.5\Delta{k}\right]$$$. A reference dataset was first reconstructed using “perfect” non-shifted trajectory conditions, while the corrupted trajectory was reconstructed both with and without our proposed correction. Difference images and root-mean-square errors (RMSE) were calculated between the two reconstructions and the ground-truth image.
The in vitro experimental setup consisted of a spherical phantom positioned close to the scanner isocenter, and the acquisition was performed with the same non-triggered 3D bSSFP sequence protocol as used for in vivo 5D cardiac imaging. Images reconstructed with and without the described method were compared using the distribution of the background noise magnitude, the signal phase inside the sphere, and the air-phantom interface sharpness.
N=10 volunteers provided written informed consent, and 5D images of the heart were acquired in a free-running mode on a 1.5T clinical MRI scanner (MAGNETOM Aera, Siemens Healthcare).12 Physiological signals for binning were extracted from the k-space data, and fully self-gated 5D motion-resolved reconstruction was performed.9,13 Images with and without the proposed correction were then visually compared.
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