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非晶硒X射线成像:雪崩增益波动的脉冲高度测量

X-ray imaging with amorphous selenium: pulse height measurements of avalanche gain fluctuations.

作者信息

Lui Brian J M, Hunt D C, Reznik A, Tanioka K, Rowlands J A

机构信息

Sunnybrook Health Sciences Centre, Imaging Research, University of Toronto, 2075 Bayview Avenue, Toronto, Ontario M4N 3M5, Canada.

出版信息

Med Phys. 2006 Sep;33(9):3183-92. doi: 10.1118/1.2335491.

Abstract

Avalanche multiplication in amorphous selenium (a-Se) can provide a large, adjustable gain for active matrix flat panel imagers (AMFPI), enabling quantum noise limited x-ray imaging during both radiography and fluoroscopy. In the case of direct conversion AMFPI, the multiplication factor for each x ray is a function of its depth of interaction, and the resulting variations in gain can reduce the detective quantum efficiency (DQE) of the system. An experimental method was developed to measure gain fluctuations by analyzing images of individual x rays that were obtained using a video camera with an a-Se target operated in avalanche mode. Pulse height spectra (PHS) of the charge produced per x ray were recorded for monoenergetic 30.9, 49.4, and 73.8 keV x-ray sources. The rapid initial decay and long tail of each PHS can be explained by a model in which positive charge dominates the initiation of avalanche. The Swank information factor quantifies the effect of gain fluctuation on DQE and was calculated from the PHS. The information factor was found to be 0.5 for a 25 microm a-Se layer with a maximum gain of approximately 300. Changing the energy of the incident x ray influenced the range of the primary photoelectron and noticeably affected the tail of the experimental PHS, but did not significantly change the avalanche Swank factor.

摘要

非晶硒(a-Se)中的雪崩倍增可为有源矩阵平板成像器(AMFPI)提供大的、可调节的增益,从而在放射摄影和荧光透视过程中实现量子噪声受限的X射线成像。对于直接转换AMFPI,每个X射线的倍增因子是其相互作用深度的函数,增益的变化会降低系统的探测量子效率(DQE)。通过分析使用在雪崩模式下运行的带有a-Se靶的摄像机获得的单个X射线图像,开发了一种实验方法来测量增益波动。记录了单能30.9、49.4和73.8 keV X射线源每X射线产生的电荷的脉冲高度谱(PHS)。每个PHS的快速初始衰减和长尾可以用一个模型来解释,在该模型中,正电荷主导雪崩的起始。斯旺克信息因子量化了增益波动对DQE的影响,并从PHS中计算得出。对于厚度为25微米、最大增益约为300的a-Se层,发现信息因子为0.5。改变入射X射线的能量会影响初级光电子的射程,并显著影响实验PHS的尾部,但不会显著改变雪崩斯旺克因子。

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