Dynamic contrast-enhanced MR imaging of rectal cancer using a golden-angle radial stack-of-stars VIBE sequence: comparison with conventional contrast-enhanced 3D VIBE sequence
Purpose To compare conventional 3D volumetric-interpolated breath-hold examination (C-VIBE) sequence image quality to that of golden-angle radial stack-of stars acquisition scheme (R-VIBE) in rectal cancer patients. Methods Seventy-eight patients had undergone pre-contrast C-VIBE, followed by DCE-MR...
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Veröffentlicht in: | Abdominal imaging 2020-02, Vol.45 (2), p.322-331 |
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Sprache: | eng |
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Zusammenfassung: | Purpose
To compare conventional 3D volumetric-interpolated breath-hold examination (C-VIBE) sequence image quality to that of golden-angle radial stack-of stars acquisition scheme (R-VIBE) in rectal cancer patients.
Methods
Seventy-eight patients had undergone pre-contrast C-VIBE, followed by DCE-MRI with R-VIBE and post-contrast C-VIBE in the visualization of rectal cancer. The first phase and the last phase of R-VIBE sequence were compared with pre-contrast and post-contrast C-VIBE sequences, respectively. Signal-to-noise ratios (SNRs) and contrast-to-noise ratios (CNRs) of rectal neoplasms, gluteus maximus, and subcutaneous fat were compared between the two different sequences. A further qualitative score system (graded 1–5) was used to evaluate the overall image. Quantitative and qualitative parameters from the two sequences were compared.
Results
In all patients, R-VIBE achieved the same SNR and CNR ratings in pre- and post-contrast (all
P
> 0.05), with the exception of a higher SNR of fat in pre-contrast images (
P
= 0.037). In addition, there were no significant differences in scores of overall image quality, lesion conspicuity, and rectal wall boundary (all
P
> 0.05). There was an improved score in artifacts of post-contrast R-VIBE sequence (
P
= 0.005).
Conclusion
R-VIBE sequence can provide comparable image quality and less motion artifacts to that of C-VIBE sequence and is feasible for imaging of rectal cancer. |
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ISSN: | 2366-004X 2366-0058 |
DOI: | 10.1007/s00261-019-02225-7 |