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首页> 外文期刊>Journal of Analytical Atomic Spectrometry >Submicron spatial resolution Pb-Pb and U-Pb dating by using a NanoSIMS equipped with the new radio-frequency ion source
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Submicron spatial resolution Pb-Pb and U-Pb dating by using a NanoSIMS equipped with the new radio-frequency ion source

机译:亚微米空间分辨率PB-PB和U-PB通过使用配备有新的射频离子源的纳米芯片

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摘要

This paper is the first to report a Pb-Pb and U-Pb analytical method at a sub-micron scale using a NanoSIMS equipped with the new radio-frequency (RF) ion source. The RF ion source can generate a high-density primary beam to improve spatial resolution. A focused Gaussian beam of ~450 pA with a diameter of ~480 nm was utilized, significantly smaller in size than the 1.7 μm beam with the same current generated by the conventional duoplasmatron source. However, the high-density primary beam causes a more significant depth effect. Thus, a larger raster area (10 × 10 μm~2) is selected to eliminate the mass fractionation caused by the depth effect. Other settings and data processing were similar to previous methods with a Duo source. Zircon standard M257 and baddeleyite standard Phalaborwa yielded ~(207)Pb/~(206)Pb ages of 547 ± 30 Ma and 2058 ± 13.8 Ma, respectively. These results agree well with the reference age values within analytical uncertainties. Using zircon Qinghu as a standard, zircon M257 and 91500 yielded U-Pb ages of 567.7 ± 6.8 Ma and 1056 ± 15 Ma, respectively, consistent with the recommended values within the analytical uncertainties. Three 4-5 μm zirconolite grains from the lunar meteorite Northwest Africa 8127 (NWA 8127) gave Pb-Pb ages of 3201 ± 25 Ma, 3174 ± 6 Ma and 3170 ± 14 Ma. One grain shows a variation of Pb/Pb age corresponding to the sub-micron scale distribution of U and Pb, probably due to the heavy impact on the moon. This technique is the first reported submicron Pb-Pb and U-Pb dating, which can be widely applied for sub-micron Pb-Pb and U-Pb dating for the tiny Zr-rich minerals from extraterrestrial samples.
机译:本文是第一个在使用配备有新的射频(RF)离子源的纳米芯片以子微米级报告PB-PB和U-PB分析方法。 RF离子源可以产生高密度主光束以提高空间分辨率。使用直径为〜480nm的聚焦高斯光束,比具有由常规的国内单位数产生的相同电流的1.7μm光束显着较小。然而,高密度主光束导致更显着的深度效果。因此,选择较大的光栅区域(10×10μm〜2)以消除由深度效果引起的质量分级。其他设置和数据处理类似于先前的使用DUO源。锆石标准M257和Baddeleyite标准Phalaborwa分别产生〜(207)Pb /〜(206)Pb Ag,分别为547±30 mA和2058±13.8 mA。这些结果与分析不确定性内的参考年龄值吻合良好。使用ZIRCON Qinghu作为标准,锆石M257和91500分别产生567.7±6.8 mA和1056±15 mA的U-Pb Ag,与分析不确定因素内的推荐值一致。来自月球陨石西北非洲8127(NWA 8127)的三个4-5μm锆石谷物给出了3201±25 mA,3174±6 mA和3170±14 mA的PB-PB。一粒颗粒显示了与U和Pb的亚微米级分布相对应的Pb / Pb时代的变化,这可能是由于对月球的重大影响。该技术是第一个报告的亚微米PB-PB和U-PB序列,可广泛应用于来自外星样品的微米PB-PB和U-PB的富含Zr的矿物质。

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  • 来源
    《Journal of Analytical Atomic Spectrometry》 |2021年第8期|1625-1633|共9页
  • 作者单位

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences P.O. Box 9825 Beijing 10029 China;

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences P.O. Box 9825 Beijing 10029 China;

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences P.O. Box 9825 Beijing 10029 China;

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences P.O. Box 9825 Beijing 10029 China;

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences P.O. Box 9825 Beijing 10029 China;

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences P.O. Box 9825 Beijing 10029 China;

    Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences P.O. Box 9825 Beijing 10029 China;

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