Department of Radiological Science, College of Health Science, Yonsei University, Wonju 220-710, Korea.
Phys Med Biol. 2012 Aug 7;57(15):4931-49. doi: 10.1088/0031-9155/57/15/4931. Epub 2012 Jul 17.
The energy-resolved photon counting detector provides the spectral information that can be used to generate images. The novel imaging methods, including the K-edge imaging, projection-based energy weighting imaging and image-based energy weighting imaging, are based on the energy-resolved photon counting detector and can be realized by using various energy windows or energy bins. The location and width of the energy windows or energy bins are important because these techniques generate an image using the spectral information defined by the energy windows or energy bins. In this study, the reconstructed images acquired with K-edge imaging, projection-based energy weighting imaging and image-based energy weighting imaging were simulated using the Monte Carlo simulation. The effect of energy windows or energy bins was investigated with respect to the contrast, coefficient-of-variation (COV) and contrast-to-noise ratio (CNR). The three images were compared with respect to the CNR. We modeled the x-ray computed tomography system based on the CdTe energy-resolved photon counting detector and polymethylmethacrylate phantom, which have iodine, gadolinium and blood. To acquire K-edge images, the lower energy thresholds were fixed at K-edge absorption energy of iodine and gadolinium and the energy window widths were increased from 1 to 25 bins. The energy weighting factors optimized for iodine, gadolinium and blood were calculated from 5, 10, 15, 19 and 33 energy bins. We assigned the calculated energy weighting factors to the images acquired at each energy bin. In K-edge images, the contrast and COV decreased, when the energy window width was increased. The CNR increased as a function of the energy window width and decreased above the specific energy window width. When the number of energy bins was increased from 5 to 15, the contrast increased in the projection-based energy weighting images. There is a little difference in the contrast, when the number of energy bin is increased from 15 to 33. The COV of the background in the projection-based energy weighting images is only slightly changed as a function of the number of energy bins. In the image-based energy weighting images, when the number of energy bins were increased, the contrast and COV increased and decreased, respectively. The CNR increased as a function of the number of energy bins. It was concluded that the image quality is dependent on the energy window, and an appropriate choice of the energy window is important to improve the image quality.
能谱解析型光子计数探测器可提供光谱信息,用于生成图像。新型成像方法包括 K 边成像、基于投影的能量加权成像和基于图像的能量加权成像,这些方法都是基于能谱解析型光子计数探测器实现的,可通过各种能量窗或能量bins 来实现。能量窗或能量 bins 的位置和宽度非常重要,因为这些技术使用能量窗或能量 bins 定义的光谱信息生成图像。在这项研究中,使用蒙特卡罗模拟对 K 边成像、基于投影的能量加权成像和基于图像的能量加权成像所获得的重建图像进行了模拟。研究了能量窗或能量 bins 对对比度、变异系数(COV)和对比噪声比(CNR)的影响。比较了这三种图像的 CNR。我们基于 CdTe 能谱解析型光子计数探测器和包含碘、钆和血液的聚甲基丙烯酸甲酯体模构建了 X 射线计算机断层扫描系统模型。为了获取 K 边图像,将较低的能量阈值固定在碘和钆的 K 边吸收能量上,并将能量窗的宽度从 1 增加到 25 个 bins。从 5、10、15、19 和 33 个能量 bins 计算了碘、钆和血液的优化能量加权因子。我们将计算出的能量加权因子分配到每个能量 bin 采集的图像中。在 K 边图像中,随着能量窗宽度的增加,对比度和 COV 降低。CNR 随能量窗宽度的增加而增加,并在特定能量窗宽度以上降低。当能量 bins 的数量从 5 增加到 15 时,基于投影的能量加权图像中的对比度增加。当能量 bin 的数量从 15 增加到 33 时,对比度几乎没有差异。基于投影的能量加权图像中背景的 COV 随能量 bin 的数量仅略有变化。在基于图像的能量加权图像中,随着能量 bins 的数量增加,对比度和 COV 分别增加和降低。CNR 随能量 bins 的数量增加而增加。结论是,图像质量取决于能量窗,选择合适的能量窗对于提高图像质量非常重要。