Barber H Bradford, Fastje David, Lemieux Daniel, Grim Gary P, Furenlid Lars R, Miller Brian W, Parkhurst Philip, Nagarkar Vivek V
Center for Gamma-Ray Imaging, University of Arizona, Tucson, AZ.
Center for Gamma-Ray Imaging, University of Arizona, Tucson, AZ ; Los Alamos National Laboratories, Los Alamos, NM.
Proc SPIE Int Soc Opt Eng. 2014 Aug 17;9215. doi: 10.1117/12.2066172.
We have investigated the light-transport properties of scintillator arrays with long, thin pixels (deep pixels) for use in high-energy gamma-ray imaging. We compared 10×10 pixel arrays of YSO:Ce, LYSO:Ce and BGO (1mm × 1mm × 20 mm pixels) made by Proteus, Inc. with similar 10×10 arrays of LSO:Ce and BGO (1mm × 1mm × 15mm pixels) loaned to us by Saint-Gobain. The imaging and spectroscopic behaviors of these scintillator arrays are strongly affected by the choice of a reflector used as an inter-pixel spacer (3M ESR in the case of the Proteus arrays and white, diffuse-reflector for the Saint-Gobain arrays). We have constructed a 3700-pixel LYSO:Ce Prototype NIF Gamma-Ray Imager for use in diagnosing target compression in inertial confinement fusion. This system was tested at the OMEGA Laser and exhibited significant optical, inter-pixel cross-talk that was traced to the use of a single-layer of ESR film as an inter-pixel spacer. We show how the optical cross-talk can be mapped, and discuss correction procedures. We demonstrate a 10×10 YSO:Ce array as part of an iQID (formerly BazookaSPECT) imager and discuss issues related to the internal activity of Lu in LSO:Ce and LYSO:Ce detectors.
我们研究了用于高能伽马射线成像的具有长而细像素(深像素)的闪烁体阵列的光传输特性。我们将Proteus公司制造的YSO:Ce、LYSO:Ce和BGO的10×10像素阵列(1毫米×1毫米×20毫米像素)与圣戈班借给我们的类似的LSO:Ce和BGO的10×10阵列(1毫米×1毫米×15毫米像素)进行了比较。这些闪烁体阵列的成像和光谱行为受到用作像素间隔物的反射器选择的强烈影响(Proteus阵列使用3M ESR,圣戈班阵列使用白色漫反射器)。我们构建了一个3700像素的LYSO:Ce原型国家点火装置伽马射线成像仪,用于诊断惯性约束聚变中的靶压缩。该系统在OMEGA激光装置上进行了测试,表现出显著的光学像素间串扰,这可追溯到使用单层ESR膜作为像素间隔物。我们展示了如何绘制光学串扰图,并讨论了校正程序。我们展示了一个10×10的YSO:Ce阵列作为iQID(原BazookaSPECT)成像仪的一部分,并讨论了与LSO:Ce和LYSO:Ce探测器中Lu的内部活性相关的问题。