3F4M Noblesse-HR惰性气体质谱仪用于多收集Ne-Ar-N2分析的性能

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
L. Zimmermann, E. Füri, J. Boulliung, J. M. Saxton
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引用次数: 0

摘要

Noblesse-HR惰性气体质谱仪设计用于固定探测器阵列在静态条件下对不同组的惰性气体同位素进行多采集分析。在法国科学与技术研究中心(CRPG, Nancy, France),我们开发了一种新的方法来测量氮(N2)丰度和同位素比率(28N2/29N2),使用3法拉第4倍增器(3F4M)系统。该过程同时获取14N14N+ (Fa2)、15N14N+ (Fa1)和15N15N+ (IC0)离子信号。内置净化系统确保超低空白水平(≤1 × 10−12 mol N2),而空气标准测量监测检测器灵敏度和仪器质量分离。在这里,我们评估了光源和变焦光学设置对质量分辨率(MR)、质量分辨率(MRP)和峰对准的影响,并确定了干扰物种的潜在贡献。Noblesse-HR用于多次收集Ne-Ar-N2分析的性能经过了几个月的评估,并在引入质谱仪的不同气体量中进行了评估。在1σ相对散射下,20Ne的平均灵敏度为5.05 × 10−5 A/Torr±1.02%,36Ar的平均灵敏度为2.86 × 10−4 A/Torr±1.37%,N2的平均灵敏度为1.18 × 10−4 A/Torr±1.90%。相应的同位素比例20 ne / 22 = 9.80±0.34%,21 ne / 22 ne = 2.90×10−2±1.53%,40 ar / 36 ar(20天)= 296.19±0.10%,38 ar / 36 ar = 0.1876±0.28%,和28 n2/29n2 = 135.92±0.05%。这些结果表明,3F4M Noblesse-HR提供了精确、准确和可重复的数据,适用于研究行星物质。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Performance of the 3F4M Noblesse–HR Noble Gas Mass Spectrometer for Multicollection Ne-Ar-N2 Analyses

Performance of the 3F4M Noblesse–HR Noble Gas Mass Spectrometer for Multicollection Ne-Ar-N2 Analyses

The Noblesse–HR noble gas mass spectrometer was designed for multicollection analyses of different sets of noble gas isotopes with a fixed detector array under static conditions. At the Centre de Recherches Pétrographiques et Géochimiques (CRPG, Nancy, France), we developed a novel procedure to measure nitrogen (N2) abundance and isotope ratio (28N2/29N2) using the 3 Faraday–4 Multiplier (3F4M) system. This procedure simultaneously acquires ion signals for 14N14N+ (Fa2), 15N14N+ (Fa1), and 15N15N+ (IC0). An in-house-built purification system ensures ultra-low blank levels (≤1 × 10−12 mol N2), while air standard measurements monitor detector sensitivity and instrumental mass fractionation. Here, we assess the effects of the source and zoom optics settings on mass resolution (MR), mass resolving power (MRP), and peak alignment, and identify potential contributions from interfering species. The performance of the Noblesse–HR for multicollection Ne-Ar-N2 analyses was evaluated over several months and across varying gas quantities introduced into the mass spectrometer. Average sensitivities, with 1σ relative scatter, were 5.05 × 10−5 A/Torr ±1.02% for 20Ne, 2.86 × 10−4 A/Torr ±1.37% for 36Ar, and 1.18 × 10−4 A/Torr ±1.90% for N2. Corresponding isotopic ratios were 20Ne/22Ne = 9.80 ± 0.34%, 21Ne/22Ne = 2.90 × 10−2 ± 1.53%, 40Ar/36Ar = 296.19 ± 0.10% (over 20 days), 38Ar/36Ar = 0.1876 ± 0.28%, and 28N2/29N2 = 135.92 ± 0.05%. These results demonstrate that the 3F4M Noblesse–HR provides precise, accurate, and reproducible data, adapted for studying planetary materials.

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来源期刊
Geochemistry Geophysics Geosystems
Geochemistry Geophysics Geosystems 地学-地球化学与地球物理
CiteScore
5.90
自引率
11.40%
发文量
252
审稿时长
1 months
期刊介绍: Geochemistry, Geophysics, Geosystems (G3) publishes research papers on Earth and planetary processes with a focus on understanding the Earth as a system. Observational, experimental, and theoretical investigations of the solid Earth, hydrosphere, atmosphere, biosphere, and solar system at all spatial and temporal scales are welcome. Articles should be of broad interest, and interdisciplinary approaches are encouraged. Areas of interest for this peer-reviewed journal include, but are not limited to: The physics and chemistry of the Earth, including its structure, composition, physical properties, dynamics, and evolution Principles and applications of geochemical proxies to studies of Earth history The physical properties, composition, and temporal evolution of the Earth''s major reservoirs and the coupling between them The dynamics of geochemical and biogeochemical cycles at all spatial and temporal scales Physical and cosmochemical constraints on the composition, origin, and evolution of the Earth and other terrestrial planets The chemistry and physics of solar system materials that are relevant to the formation, evolution, and current state of the Earth and the planets Advances in modeling, observation, and experimentation that are of widespread interest in the geosciences.
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