Purpose: Accurate quantification of proton density fat fraction (PDFF) and in the supracalvicular (SCV) fossa is critical for studying brown adipose tissue (BAT), but is challenged by respiratory motion-induced fluctuations. This study compares conventional Cartesian imaging to a radial stack-of-stars (SoS) trajectory, with and without retrospective temporal correction, in terms of PDFF and mapping precision.
Methods: Motion-induced fluctuations and tissue displacement were modeled using a digital anatomical phantom. Both Cartesian and radial SoS trajectories were simulated, with temporal correction, relying on oversampling of the k-space center, applied to the radial SoS data. Additionally, repeated in vivo scans were performed in four volunteers using both trajectories. PDFF and were quantified across repetitions.
Results: Simulations demonstrated smaller PDFF and errors in radial SoS compared to Cartesian imaging under the influence of simulated motion effects. In the simulations, the mean absolute PDFF error decreased from with Cartesian to with radial SoS, and the error decreased from 7.50 ms to 3.37 ms. In vivo, radial SoS provided higher repeatability for both parameters compared to Cartesian acquisitions, as measured by the inter-scan coefficient of variation. Retrospective temporal correction further improved the repeatability of quantification.
Conclusions: Radial SoS imaging improves motion robustness and repeatability of PDFF and quantification in the SCV fossa compared to Cartesian acquisitions. Incorporating retrospective temporal correction further enhances reliability and may strengthen the precision of BAT activation studies.
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