Cunningham I A, Westmore M S, Fenster A
Imaging Research Laboratories, John P. Robarts Research Institute, London Ontario, Canada.
Med Phys. 1994 Mar;21(3):417-27. doi: 10.1118/1.597401.
The detective quantum efficiency (DQE) is a system parameter that can be used to accurately describe image noise transfer characteristics through many imaging systems. A simpler approach used by some investigators, particularly when evaluating new ideas and system designs, is to describe the system as a series of cascaded stages. Each stage may correspond to either an increase in the number of quanta (e.g., conversion from x-ray to optical quanta in a radiographic screen), or a loss (a detection or coupling probability). The number of secondary quanta at each stage per incident primary quantum is given by the product of all preceding gains, and can be displayed graphically for convenient interpretation. The stage with the fewest quanta is called the "quantum sink," limiting the pixel signal-to-noise ratio to less than the square root of the number of quanta per pixel. This conventional zero-spatial-frequency "quantum accounting diagram" (QAD), however, neglects the spatial spreading of secondary quanta and can seriously underestimate image noise. It is shown that this problem is avoided with the introduction of a spatial-frequency dependent QAD, expressed as the product of the gains and squared modulation-transfer functions (MTF) of each stage. A generalized expression is developed for the DQE of a cascaded imaging system that is dependent only on the gain, gain Poisson excess (related to the variance), and MTF, of each stage. A direct relationship is then shown to exist between the DQE and values in the QAD. The QAD of a hypothetical system consisting of a charge-coupled device camera and a scintillating screen is evaluated as an illustrative example. The conventional zero-frequency analysis suggests two quantum sinks occur with approximately equal importance: one in the number of x rays, and one in the number of optical quanta. The spatial-frequency dependent analysis, however, shows the optical quantum sink becomes severe and dominates at nonzero frequencies. The necessary increase in gain or optical numerical aperture required to prevent the optical quantum sink for spatial frequencies of interest is determined from the QAD analysis. The visual impact of this nonzero spatial-frequency quantum sink is shown in images generated using a Monte Carlo simulation of the cascading process.
探测量子效率(DQE)是一个系统参数,可用于精确描述图像噪声通过许多成像系统的传递特性。一些研究人员采用的一种更简单的方法,特别是在评估新想法和系统设计时,是将系统描述为一系列级联阶段。每个阶段可能对应于量子数量的增加(例如,在射线照相屏中从X射线转换为光量子),或者损失(检测或耦合概率)。每个入射初级量子在每个阶段的次级量子数量由所有先前增益的乘积给出,并且可以以图形方式显示以便于解释。量子数量最少的阶段称为“量子阱”,将像素信噪比限制为小于每个像素量子数量的平方根。然而,这种传统的零空间频率“量子核算图”(QAD)忽略了次级量子的空间扩展,并且可能严重低估图像噪声。结果表明,通过引入与空间频率相关的QAD可以避免这个问题,该QAD表示为每个阶段的增益和平方调制传递函数(MTF)的乘积。针对级联成像系统的DQE开发了一个广义表达式,该表达式仅取决于每个阶段的增益、增益泊松过量(与方差相关)和MTF。然后表明DQE与QAD中的值之间存在直接关系。作为一个说明性示例,评估了由电荷耦合器件相机和闪烁屏组成的假设系统的QAD。传统的零频率分析表明存在两个重要性大致相等的量子阱:一个在X射线数量中,另一个在光量子数量中。然而,与空间频率相关的分析表明,光量子阱在非零频率下变得严重并占主导地位。根据QAD分析确定了为防止感兴趣空间频率处的光量子阱所需的增益或光学数值孔径的必要增加。在使用级联过程的蒙特卡罗模拟生成的图像中显示了这种非零空间频率量子阱的视觉影响。