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Calibration of Nu-Instruments Noblesse multicollector mass spectrometers for argon isotopic measurements using a newly developed reference gas

机译:使用新开发的参考气体校准用于氩同位素测量的Nu-Instruments Noblesse多收集器质谱仪

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The greatest challenge limiting ~(40)Ar/~(39)Ar multicollection measurements is the availability of appropriate standard gasses to intercalibrate detectors. In particular, use of zoom lens ion-optics to steer and focus ion beams into a fixed detector array (i.e., Nu Instruments Noblesse) makes intercalibration of multiple detectors challenging because different ion-optic tuning conditions are required for optimal peak shape and sensitivity at different mass stations. We have found that detector efficiency and mass discrimination are affected by changes in ion-optic tuning parameters. Reliance upon an atmospheric Ar standard to calibrate the Noblesse is problematic because there is no straightforward way to relate atmospheric ~(40)Ar and ~(36)Ar to measurements of ~(40)Ar and ~(39)Ar if they are measured on separate detectors. After exploring alternative calibration approaches, we have concluded that calibration of the Noblesse is best performed using exactly the same source, detector, and ion-optic tuning settings as those used in routine ~(40)Ar/~(39)Ar analysis. To accomplish this, we have developed synthetic reference gasses containing ~(40)Ar, ~(39)Ar and ~(38)Ar produced by mixing gasses derived from neutron-irradiated sanidine with an enriched ~(38)Ar spike. We present a new method for calibrating the Noblesse based on use of both atmospheric Ar and the synthetic reference gasses. By combining atmospheric Ar and synthetic reference gas in different ways, we can directly measure ~(40)Ar/~(39)Ar, ~(38)Ar/~(39)Ar, and ~(36)Ar/~(39)Ar correction factors over ratios that vary from 0.5 to 460. These correction factors are reproducible to better than ±0.5‰ (2σ standard error) over intervals spanning ~24h but can vary systematically by ~4% over 2weeks of continuous use when electron multiplier settings are held constant. Monitoring this variation requires daily calibration of the instrument. Application of the calibration method to ~(40)Ar/~(39)Ar multicollection measurements of widely used sanidine reference materials ACs-2, FCs-2, and TCs-2 demonstrate that calculated ~(40)Ar*/~(39)Ar_K can be accurately corrected to yield model ~(40)Ar/~(39)Ar ages consistent with those reported by Earthtime ~(40)Ar/~(39)Ar laboratories. Replicate analyses of 8-12 single-crystal sanidine ages are reproduced to within 1-2‰ (2σ standard error) under optimal analytical conditions. This calibration technique is applicable over a wide range of isotopic ratios and signal sizes. Finally, the reference gas has the added advantage of facilitating straightforward characterization of electron multiplier dead time over a wide dynamic range.
机译:限制〜(40)Ar /〜(39)Ar多次收集测量的最大挑战是如何使用合适的标准气体对检测器进行内部校准。特别是,使用变焦透镜离子光学器件将离子束转向和聚焦到固定的检测器阵列(即Nu Instruments Noblesse)中,使多个检测器的相互校准具有挑战性,因为需要不同的离子光学调谐条件才能获得最佳的峰形和灵敏度。不同的大众车站。我们发现,检测器效率和质量区分受离子光学调谐参数变化的影响。依靠大气Ar标准来校准Noblesse是有问题的,因为如果测量到〜(40)Ar和〜(39)Ar,没有直接的方法将大气〜(40)Ar和〜(36)Ar与〜(40)Ar和〜(39)Ar相关联在单独的探测器上。在探索了替代校准方法之后,我们得出结论,最好使用与常规〜(40)Ar /〜(39)Ar分析中使用的源,检测器和离子光学调谐设置完全相同的方式对Noblesse进行校准。为此,我们开发了含有〜(40)Ar,〜(39)Ar和〜(38)Ar的合成参考气体,这些参考气体是通过将中子辐照的尿苷衍生的气体与富集的〜(38)Ar尖峰混合而产生的。我们提出了一种基于大气Ar和合成参考气体的校准Noblesse的新方法。通过以不同方式组合大气Ar和合成参考气体,我们可以直接测量〜(40)Ar /〜(39)Ar,〜(38)Ar /〜(39)Ar和〜(36)Ar /〜(39 )Ar校正系数,范围从0.5到460不等。这些校正系数在〜24h的间隔内可重现优于±0.5‰(2σ标准误差),但是当电子倍增器连续使用2周后,可以系统地变化约4%设置保持不变。监视此变化需要每天校准仪器。校准方法在广泛使用的Sanidine参考物质ACs-2,FCs-2和TCs-2的〜(40)Ar /〜(39)Ar多次收集测量中的应用证明了计算出的〜(40)Ar * /〜(39可以准确地校正)Ar_K以产生与Earthtime〜(40)Ar /〜(39)Ar实验室报告的模型一致的〜(40)Ar /〜(39)Ar年龄模型。在最佳分析条件下,对8-12个单晶Sanidine年龄的重复分析可再现到1-2‰(2σ标准误差)之内。该校准技术适用于各种同位素比率和信号大小。最后,参比气体具有在宽动态范围内促进电子倍增器死区时间的简单表征的附加优势。

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