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Developing a CCD camera with high spatial resolution for RIXS in the soft X-ray range

机译:为软X射线范围内的RIXS开发具有高空间分辨率的CCD相机

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摘要

The Super Advanced X-ray Emission Spectrometer (SAXES) at the Swiss Light Source contains a high resolution Charge-Coupled Device (CCD) camera used for Resonant Inelastic X-ray Scattering (RIXS). Using the current CCD-based camera system, the energy-dispersive spectrometer has an energy resolution (E/ΔE) of approximately 12,000 at 930 eV. A recent study predicted that through an upgrade to the grating and camera system, the energy resolution could be improved by a factor of 2. In order to achieve this goal in the spectral domain, the spatial resolution of the CCD must be improved to better than 5 μm from the current 24 μm spatial resolution (FWHM). The 400 eV-1600 eV energy X-rays detected by this spectrometer primarily interact within the field free region of the CCD, producing electron clouds which will diffuse isotropically until they reach the depleted region and buried channel. This diffusion of the charge leads to events which are split across several pixels. Through the analysis of the charge distribution across the pixels, various centroiding techniques can be used to pinpoint the spatial location of the X-ray interaction to the sub-pixel level, greatly improving the spatial resolution achieved. Using the PolLux soft X-ray microspectroscopy endstation at the Swiss Light Source, a beam of X-rays of energies from 200 eV to 1400 eV can be focused down to a spot size of approximately 20 ran. Scanning this spot across the 16 μm square pixels allows the sub-pixel response to be investigated. Previous work has demonstrated the potential improvement in spatial resolution achievable by centroiding events in a standard CCD. An Electron-Multiplying CCD (EM-CCD) has been used to improve the signal to effective readout noise ratio achieved resulting in a worst-case spatial resolution measurement of 4.5 ± 0.2 μm and 3.9 + 0.1 μm at 530 eV and 680 eV respectively. A method is described that allows the contribution of the X-ray spot size to be deconvolved from these worst-case resolution measurements, estimating the spatial resolution to be approximately 3.5 μm and 3.0 μm at 530 eV and 680 eV, well below the resolution limit of 5 μm required to improve the spectral resolution by a factor of 2.
机译:瑞士光源处的超高级X射线发射光谱仪(SAXES)包含用于共振非弹性X射线散射(RIXS)的高分辨率电荷耦合器件(CCD)相机。使用当前的基于CCD的摄像头系统,能量色散光谱仪在930 eV时的能量分辨率(E /ΔE)约为12,000。最近的一项研究预测,通过升级光栅和摄像系统,可以将能量分辨率提高2倍。为了在光谱域中实现这一目标,必须将CCD的空间分辨率提高到优于从当前的24μm空间分辨率(FWHM)减小5μm。该光谱仪检测到的400 eV-1600 eV能量X射线主要在CCD的无场区内相互作用,产生电子云,这些云将各向同性扩散,直到到达耗尽区和掩埋通道。电荷的这种扩散导致事件分成多个像素。通过分析整个像素上的电荷分布,可以使用各种质心技术将X射线交互的空间位置精确定位到子像素级别,从而大大提高了实现的空间分辨率。使用瑞士光源的PolLux软X射线显微光谱终端站,可以将200 eV至1400 eV的X射线能量束聚焦到大约20纳米的光斑。在16μm正方形像素上扫描此点可以研究子像素响应。先前的工作表明,通过标准CCD的质心事件可以实现空间分辨率的潜在提高。已使用电子倍增CCD(EM-CCD)来提高信号与有效读数的噪声比,从而在530 eV和680 eV的最坏情况下分别进行4.5±0.2μm和3.9 + 0.1μm的空间分辨率测量。描述了一种方法,该方法可以从这些最坏情况的分辨率测量结果中消除X射线光斑大小的贡献,从而在530 eV和680 eV时估计空间分辨率分别约为3.5μm和3.0μm,远低于分辨率极限将光谱分辨率提高2倍需要5μm。

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