Time-resolved velocity mapping at high magnetic fields: A preclinical comparison between stack‐of‐stars and cartesian 4D-Flow

dc.bibliographicCitation.firstPage963807eng
dc.bibliographicCitation.volume10eng
dc.contributor.authorNahardani, Ali
dc.contributor.authorKrämer, Martin
dc.contributor.authorEbrahimi, Mahyasadat
dc.contributor.authorHerrmann, Karl-Heinz
dc.contributor.authorLeistikow, Simon
dc.contributor.authorLinsen, Lars
dc.contributor.authorMoradi, Sara
dc.contributor.authorReichenbach, Jürgen R.
dc.contributor.authorHoerr, Verena
dc.date.accessioned2022-11-23T13:06:06Z
dc.date.available2022-11-23T13:06:06Z
dc.date.issued2022
dc.description.abstractPurpose: Prospectively-gated Cartesian 4D-flow (referred to as Cartesian-4D-flow) imaging suffers from long TE and intensified flow-related intravoxel-dephasing especially in preclinical ultra-high field MRI. The ultra-short-echo (UTE) 4D-flow technique can resolve the signal loss in higher-order blood flows; however, the long scan time of the high resolution UTE-4D-flow is considered as a disadvantage for preclinical imaging. To compensate for prolonged acquisitions, an accelerated k0-navigated golden-angle center-out stack-of-stars 4D-flow sequence (referred to as SoS-4D-flow) was implemented at 9.4T and the results were compared to conventional Cartesian-4D-flow mapping in-vitro and in-vivo. Methods: The study was conducted in three steps (A) In-vitro evaluation in a static phantom: to quantify the background velocity bias. (B) In-vitro evaluation in a flowing water phantom: to investigate the effects of polar undersampling (US) on the measured velocities and to compare the spatial velocity profiles between both sequences. (C) In-vivo evaluations: 24 C57BL/6 mice were measured by SoS-4D-flow (n = 14) and Cartesian-4D-flow (n = 10). The peak systolic velocity in the ascending aorta and the background velocity in the anterior chest wall were analyzed for both techniques and were compared to each other. Results: According to the in-vitro analysis, the background velocity bias was significantly lower in SoS-4D-flow than in Cartesian-4D-flow (p < 0.05). Polar US in SoS-4D-flow influenced neither the measured velocity values nor the spatial velocity profiles in comparison to Cartesian-4D-flow. The in-vivo analysis showed significantly higher diastolic velocities in Cartesian-4D-flow than in SoS-4D-flow (p < 0.05). A systemic background bias was observed in the Cartesian velocity maps which influenced their streamline directions and magnitudes. Conclusion: The results of our study showed that at 9.4T SoS-4D-flow provided higher accuracy in slow flow imaging than Cartesian-4D-flow, while the same measurement time could be achieved.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/10424
dc.identifier.urihttp://dx.doi.org/10.34657/9460
dc.language.isoengeng
dc.publisherLausanne : Frontiers Mediaeng
dc.relation.doihttps://doi.org/10.3389/fphy.2022.963807
dc.relation.essn2296-424X
dc.relation.ispartofseriesFrontiers in physics 10 (2022)eng
dc.rights.licenseCC BY 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/eng
dc.subject4D-floweng
dc.subjectMRIeng
dc.subjectphase-contrasteng
dc.subjectstack-of-starseng
dc.subjectUTEeng
dc.subject.ddc530eng
dc.titleTime-resolved velocity mapping at high magnetic fields: A preclinical comparison between stack‐of‐stars and cartesian 4D-Floweng
dc.typearticleeng
dc.typeTexteng
dcterms.bibliographicCitation.journalTitleFrontiers in physicseng
tib.accessRightsopenAccesseng
wgl.contributorIPHTeng
wgl.subjectPhysikeng
wgl.typeZeitschriftenartikeleng
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