Title of article :
Radiation dose to patients and image quality evaluation from coronary 256-slice computed tomographic angiography
Author/Authors :
Chen، نويسنده , , Liang-Kuang and Wu، نويسنده , , Tung-Hsin and Yang، نويسنده , , Ching-Ching and Tsai، نويسنده , , Chia-Jung and Lee، نويسنده , , Jason J.S. and Yonas، نويسنده ,
Abstract :
The aim of this study is to assess radiation dose and the corresponding image quality from suggested CT protocols which depends on different mean heart rate and high heart rate variability by using 256-slice CT. Fifty consecutive patients referred for a cardiac CT examination were included in this study. All coronary computed tomographic angiography (CCTA) examinations were performed on a 256-slice CT scanner with one of five different protocols: retrospective ECG-gating (RGH) with full dose exposure in all R–R intervals (protocol A), RGH of 30–80% pulsing window with tube current modulation (B), RGH of 78±5% pulsing window with tube current modulation (C), prospective ECG-triggering (PGT) of 78% R–R interval with 5% padding window (D) and PGT of 78% R–R interval without padding window (E). Radiation dose parameters and image quality scoring were determined and compared. In this study, no significant differences were found in comparison on image quality of the five different protocols. Protocol A obtained the highest radiation dose comparing with those of protocols B, C, D and E by a factor of 1.6, 2.4, 2.5 and 4.3, respectively (p<0.001), which were ranged between 2.7 and 11.8 mSv. The PGT could significantly reduce radiation dose delivered to patients, as compared to the RGH. However, the use of PGT has limitations and is only good in assessing cases with lower mean heart rate and stable heart rate variability. With higher mean heart rate and high heart rate variability circumstances, the RGH within 30–80% of R–R interval pulsing window is suggested as a feasible technique for assessing diagnostic performance.
Keywords :
CT angiography , 256-slice CT , radiation dose , image quality
Journal title :
Astroparticle Physics