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X 射线 PCD 成像中光谱退降和空间能量相关性的影响。

Effect of Spectral Degradation and Spatio-Energy Correlation in X-Ray PCD for Imaging.

出版信息

IEEE Trans Med Imaging. 2018 Aug;37(8):1910-1919. doi: 10.1109/TMI.2018.2834369. Epub 2018 May 8.

DOI:10.1109/TMI.2018.2834369
PMID:29993882
Abstract

Charge sharing, scatter, and fluorescence events in a photon counting detector can result in counting of a single incident photon in multiple neighboring pixels, each at a fraction of the true energy. This causes energy distortion and correlation of data across energy bins in neighboring pixels (spatio-energy correlation), with the severity depending on the detector pixel size and detector material. If a "macro-pixel" is formed by combining the counts from multiple adjacent small pixels, it will exhibit correlations across its energy bins. Understanding these effects can be crucial for detector design and for model-based imaging applications. This paper investigates the impact of these effects in basis material and effective monoenergetic estimates using the Cramér-Rao Lower Bound. To do so, we derive a correlation model for the multi-counting events. CdTe detectors with grids of pixels with side length of $250\mu \text{m}$ , $500\mu \text{m}$ , and 1 mm were compared, with binning of $4\times4$ , $2\times2$ , and $1\times1$ pixels, respectively, to keep the same net 1 mm2 aperture constant. The same flux was applied to each. The mean and covariance matrix of measured photon counts were derived analytically using spatio-energy response functions precomputed from Monte Carlo simulations. Our results show that a 1 mm2 macro-pixel with $250\times 250,,\mu \text{m}^{\textsf {2}}$ sub-pixels shows 35% higher standard deviation than a single 1 mm2 pixel for material-specific imaging, while the penalty for effective monoenergetic imaging is <10% compared with a single 1 mm $^{\textsf {2}}$ pixel. Potential benefits of sub-pixels (higher spatial resolution and lower pulse pile-up effects) are important but were not investigated here.

摘要

在光子计数探测器中,电荷共享、散射和荧光事件可能导致单个入射光子在多个相邻像素中被计数,每个像素的能量都只有真实能量的一部分。这会导致能量失真和相邻像素之间的数据相关性(空间-能量相关性),其严重程度取决于探测器像素尺寸和探测器材料。如果通过组合多个相邻小像素的计数来形成一个“宏像素”,则它将在其能量-bin 之间表现出相关性。了解这些影响对于探测器设计和基于模型的成像应用至关重要。本文使用克拉美-罗下界研究了这些效应在基础材料和有效单能估计中的影响。为此,我们为多计数事件推导了一个相关模型。比较了具有边长为$250\mu \text{m}$、$500\mu \text{m}$和 1 毫米的网格像素的 CdTe 探测器,分别采用$4\times4$、$2\times2$和$1\times1$像素的 binning,以保持相同的净 1 毫米$^2$孔径不变。相同的通量应用于每个探测器。使用从蒙特卡罗模拟预先计算的空间-能量响应函数,从分析上推导出测量光子计数的均值和协方差矩阵。我们的结果表明,对于特定材料的成像,具有$250\times 250\mu \text{m}^{\textsf {2}}$子像素的 1 毫米$^2$宏像素的标准偏差比单个 1 毫米$^2$像素高 35%,而与单个 1 毫米$^2$像素相比,有效单能成像的代价小于 10%。子像素的潜在优势(更高的空间分辨率和更低的脉冲堆积效应)很重要,但这里没有进行研究。

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