Seely John F, Pereira Nino R, Weber Bruce V, Schumer Joseph W, Apruzese John P, Hudson Lawrence T, Szabo Csilla I, Boyer Craig N, Skirlo Scott
Space Science Division, Naval Research Laboratory, Washington, D.C. 20375, USA.
Appl Opt. 2010 Aug 10;49(23):4372-8. doi: 10.1364/AO.49.004372.
The spatial resolution of an x-ray CCD detector was determined from the widths of the tungsten x-ray lines in the spectrum formed by a crystal spectrometer in the 58 to 70 keV energy range. The detector had 20 microm pixel, 1700 by 1200 pixel format, and a CsI x-ray conversion scintillator. The spectral lines from a megavolt x-ray generator were focused on the spectrometer's Rowland circle by a curved transmission crystal. The line shapes were Lorentzian with an average width after removal of the natural and instrumental line widths of 95 microm (4.75 pixels). A high spatial frequency background, primarily resulting from scattered gamma rays, was removed from the spectral image by Fourier analysis. The spectral lines, having low spatial frequency in the direction perpendicular to the dispersion, were enhanced by partially removing the Lorentzian line shape and by fitting Lorentzian curves to broad unresolved spectral features. This demonstrates the ability to improve the spectral resolution of hard x-ray spectra that are recorded by a CCD detector with well-characterized intrinsic spatial resolution.
通过晶体光谱仪在58至70 keV能量范围内形成的光谱中钨X射线线的宽度,确定了X射线电荷耦合器件(CCD)探测器的空间分辨率。该探测器具有20微米像素、1700×1200像素格式,以及一个碘化铯(CsI)X射线转换闪烁体。兆伏X射线发生器产生的光谱线通过弯曲的透射晶体聚焦在光谱仪的罗兰圆上。去除自然线宽和仪器线宽后,线形状为洛伦兹分布,平均宽度为95微米(4.75像素)。通过傅里叶分析从光谱图像中去除了主要由散射伽马射线产生的高空间频率背景。通过部分去除洛伦兹线形状并将洛伦兹曲线拟合到宽的未分辨光谱特征,增强了在垂直于色散方向上具有低空间频率的光谱线。这证明了提高具有良好表征的固有空间分辨率的CCD探测器记录的硬X射线光谱的光谱分辨率的能力。