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A re-examination of the fundamental parameters approach to calibration of the Curiosity rover alpha particle X-ray spectrometer

机译:对校准校准的好奇松罗波α粒子X射线光谱仪的基本参数方法的重新检查

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摘要

In terrestrial instruments for X-ray emission analysis (e.g. X-ray fluorescence, electron microprobe) the angle of excitation and the angle of characteristic X-ray emission by samples are typically well-defined. This is not the case for the Mars rovers' alpha particle X-ray spectrometers, necessitating use of "effective" angles in any fundamental parameters approach to spectrum fitting and derivation of element concentrations. A new Monte Carlo computation of expected characteristic X-ray yields has enabled us to examine the choice of effective angles in detail and to compare with our previous estimates; the mean angles taken over all detected events appear to be the most satisfactory approximation. These were used in our GUAPX code to process APXS spectra from ten mono-mineralic geochemical reference materials. Agreement between our concentration values and those determined by the specialist company ActLabs was excellent.
机译:在X射线发射分析(例如X射线荧光,电子微探针)的陆生仪器中,通常定义了X射线发射分析的激发角和特征X射线发射的角度。这不是火星群α粒子X射线光谱仪的情况,需要在任何基本参数方法中使用“有效”角度来频谱拟合和元素浓度的推导。新的蒙特卡罗计算预期特征X射线产量使我们能够详细检查有效角度的选择,并与我们以前的估计进行比较;所有检测到的事件所采取的平均角度似乎是最令人满意的近似。这些用于我们的GUAPX代码,以从10个单一矿物地球化学参考材料处理APXS光谱。我们的集中价值与专家公司Actlabs确定的人之间的协议非常出色。

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