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Measuring and Interpreting X-ray Fluorescence from Planetary Surfaces

机译:测量和解释行星表面的X射线荧光

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As part of a comprehensive study of X-ray emission from planetary surfaces and in particular the planet Mercury, we have measured fluorescent radiation from a number of planetary analog rock samples using monochromatized synchrotron radiation provided by the BESSY II electron storage ring. The experiments were carried out using a purpose built X-ray fluorescence (XRF) spectrometer chamber developed by the Physikalisch-Technische Bundesanstalt, Germany's national metrology institute. The XRF instrumentation is absolutely calibrated and allows for reference-free quantitation of rock sample composition, taking into account secondary photon- and electron-induced enhancement effects. The fluorescence data, in turn, have been used to validate a planetary fluorescence simulation tool based on the GEANT4 transport code. This simulation can be used as a mission analysis tool to predict the time-dependent orbital XRF spectral distributions from planetary surfaces throughout the mapping phase.
机译:作为对行星表面(尤其是水星)的X射线发射进行全面研究的一部分,我们已经使用BESSY II电子存储环提供的单色同步加速器辐射测量了许多行星模拟岩石样品的荧光辐射。实验是使用由德国国家计量学会Physikalisch-Technische Bundesanstalt开发的专用X射线荧光(XRF)光谱仪室进行的。 XRF仪器经过绝对校准,并考虑到二次光子和电子诱导的增强效应,可对岩石样品成分进行无参考定量。荧光数据又被用于验证基于GEANT4传输代码的行星荧光模拟工具。该模拟可以用作任务分析工具,以预测整个制图阶段来自行星表面的时间相关的轨道XRF光谱分布。

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