| Literature DB >> 36172590 |
Lu Lin1, Peijun Liu1, Gan Sun2, Jian Wang1, Dong Liang3, Hairong Zheng3, Zhengyu Jin1, Yining Wang1.
Abstract
Background: Cardiovascular magnetic resonance (CMR) imaging at ultra-high fields (UHF) such as 7T has encountered many challenges such as faster T 2 * relaxation, stronger B0 and B1+ field inhomogeneities and additional safety concerns due to increased specific absorption rate (SAR) and peripheral nervous stimulation (PNS). Recently, a new line of 5T whole body MRI system has become available, and this study aims at evaluating the performance and benefits of this new UHF system for CMR imaging.Entities:
Keywords: 5T; UHF; cardiac MR; cine; ventricular function
Year: 2022 PMID: 36172590 PMCID: PMC9510665 DOI: 10.3389/fcvm.2022.913707
Source DB: PubMed Journal: Front Cardiovasc Med ISSN: 2297-055X
Figure 1Typical ECG wave forms from one volunteer, recorded during CMR CINE scans at 3 and 5T respectively.
CMR scanning parameters in this study.
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| Short axis | Field of view (mm) | 360 × 280~320 | *360 × 280~320 | 360 × 280~320 | 360 × 280~320 |
| Spatial resolution (mm) | 1.6 × 1.6 | 1.6 × 1.6 | 1.6 × 1.6 | 1.0 × 1.0 | |
| Matrix | 224 × 174~199 | 224 × 174~199 | 224 × 174~199 | 352 × 274~313 | |
| Number of slices | 10 | 10 | 10 | 12 | |
| Slice thickness (mm) | 8 | 8 | 8 | 6 | |
| Slice gap (mm) | 1.6 | 1.6 | 1.6 | 1.2 | |
| TE/TR (ms) | 1.37/2.98 | 2.65~2.69/5.42~5.45 | 2.84/5.55 | 3.06/5.95 | |
| Flip angle (°) | 60° | 15° | 10° | 10° | |
| Bandwidth (Hz/pixel) | 1,000 | 300 | 300 | 300 | |
| 2 Chamber | Field of view (mm) | 360 × 280~320 | 360 × 280~320 | 360 × 280~320 | 360 × 280~320 |
| Spatial resolution (mm) | 1.6 × 1.6 | 1.6 × 1.6 | 1.6 × 1.6 | 1.0 × 1.0 | |
| Matrix | 224 × 174~199 | 224 × 174~199 | 224 × 174~199 | 352 × 274~313 | |
| Number of slices | 1 | 1 | 1 | 1 | |
| Slice thickness (mm) | 8 | 8 | 8 | 6 | |
| TE/TR (ms) | 1.37/2.98 | 2.65~2.69/5.42~5.45 | 2.42/4.48 | 3.06/5.95 | |
| Flip angle (°) | 60° | 15° | 10° | 10° | |
| Bandwidth (Hz/pixel) | 1,000 | 300 | 500 | 300 | |
| 4 Chamber | Field of view (mm) | 360 × 260~320 | 360 × 260~320 | 360 × 260~300 | 360 × 260~300 |
| Spatial resolution (mm) | 1.6 × 1.6 | 1.6 × 1.6 | 1.6 × 1.6 | 1.0 × 1.0 | |
| Matrix | 224 × 162~187 | 224 × 162~187 | 224 × 162~187 | 352 × 254~293 | |
| Number of slices | 1 | 1 | 1 | 1 | |
| Slice thickness (mm) | 8 | 8 | 8 | 6 | |
| TE/TR (ms) | 1.37/2.98 | 2.65/5.42 | 2.42/4.48 | 3.06/5.95 | |
| Flip angle (°) | 60° | 15° | 10° | 10° | |
| Bandwidth (Hz/pixel) | 1,000 | 300 | 500 | 300 |
Figure 2Typical CMR cine images of one subject. All images are free of major artifacts and show good image quality.
Figure 3Multi-slice short-axis GRE images at 5T of one volunteer, comparing between routine resolution (top row) and high resolution (bottom row).
Rating of overall image quality and presence of artifacts, using 3T GRE as reference.
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| SAX | 3T GRE | 1.6 × 1.6 × 8 | 2.0 ± 0.5 | 1.2 ± 0.4 |
| 3T bSSFP | 1.6 ×1.6 ×8 | 2.5 ± 0.6 ( | 0.6 ± 0.6 ( | |
| 5T GRE | 1.6 ×1.6 ×8 | 2.2 ± 0.5 ( | 1.2 ± 0.4 ( | |
| 5T GRE HR | 1.0 ×1.0 ×6 | 2.1 ± 0.8 ( | 1.4 ± 0.5 ( | |
| Long axis | 3T GRE | 1.6 ×1.6 ×8 | 1.5 ± 0.5 | 1.4 ± 0.6 |
| 3T bSSFP | 1.6 ×1.6 ×8 | 2.6 ± 0.5 ( | 0.4 ± 0.5 ( | |
| 5T GRE | 1.6 ×1.6 ×8 | 1.9 ± 0.5 ( | 1.1 ± 0.5 ( | |
| 5T GRE HR | 1.0 ×1.0 ×6 | 2.3 ± 0.7 ( | 1.1 ± 0.4 ( |
Both rating scores ranged from 0 to 3, and a higher rating denotes better image quality, but worse artifact control.
Asteroids indicate significant differences, i.e., p < 0.05, when compared to 3T GRE.
Comparison on SNR and CNR of SAX images, using 3T GRE as reference.
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| 3T GRE | 1.6 ×1.6 ×8 | 91.8 ± 10.0 | 1.00 | 52.1 ± 13.7 | 1.00 |
| 3T bSSFP | 1.6 ×1.6 ×8 | 130.9 ± 23.2 ( | 1.43 | 94.0 ± 21.5 ( | 1.80 |
| 5T GRE | 1.6 ×1.6 ×8 | 143.8 ± 26.3 ( | 1.57 | 92.5 ± 22.7 ( | 1.78 |
| 5T GRE HR | 1.0 ×1.0 ×6 | 62.5 ± 9.9 ( | 0.68 | 37.4 ± 10.2 ( | 0.72 |
Asteroids indicate significant differences, i.e., p < 0.05, when compared to 3T GRE.
Comparison of CMR CINE functional quantities, using 3T bSSFP as reference.
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| 3T bSSFP | 129.8 ± 18.5 | 45.1 ± 9.1 | 98.1 ± 21.2 | 65.3 ± 4.1 | 142.2 ± 20.5 | 63.0 ± 13.4 | 56.1 ± 4.7 |
| 3T GRE | 128.1 ± 20.2 | 43.3 ± 9.2 | 105.7 ± 20.7 | 66.4 ± 5.0 | 148.7 ± 21.4* | 62.3 ± 13.1 | 58.4 ± 4.9* |
| 5T GRE | 130.1 ± 19.2 | 44.0 ± 11.6 | 104.0 ± 20.2* | 66.8 ± 6.0 | 152.1 ± 21.3* | 66.5 ± 12.7 | 57.4 ± 4.7 |
| 5T GRE HR | 129.6 ± 18.0 | 45.2 ± 10.8 | 101.5 ± 19.5 | 65.4 ± 5.2 | 151.5 ± 20.2* | 65.8 ± 13.8 | 56.8 ± 6.5 |
Asteroids indicate significant differences, i.e., p < 0.05, when compared to 3T bSSFP.
Figure 4Bland-Altman analyses for LV. LV EDV (ml), ESV (ml), mass (g) and EF (%) are shown in rows. Comparisons of 3T GRE, 5T GRE, and 5T GRE HR to 3T bSSFP are shown in columns.
Figure 5Bland-Altman analyses for RV. RV EDV (ml), ESV (ml) and EF (%) are shown in rows. Comparisons of 3T GRE, 5T GRE, and 5T GRE HR to 3T bSSFP are shown in columns.