期刊
ULTRAMICROSCOPY
卷 159, 期 -, 页码 248-254出版社
ELSEVIER
DOI: 10.1016/j.ultramic.2015.05.021
关键词
Atom-probe tomography; Meteoritic nanodiamond; Presolar grains; Nucleosynthesis; FIB liftout
类别
资金
- NASA [NNX13AF53G]
- NSF-MRI program [DMR0420532]
- NRL-DURIP [N00014-0400798, N00014-0610539, N00014-0910781]
- MRSEC program at the Materials Research Center [NSF DMR-1121262]
- Nanoscale Science and Engineering Center at the International Institute for Nanotechnology [NSF EEC0647560]
- State of Illinois, through the International Institute for Nanotechnology
- Initiative for Sustainability and Energy at Northwestern
- NASA [NNX13AF53G, 474493] Funding Source: Federal RePORTER
The astrophysical origins of similar to 3 nm-diameter meteoritic nanodiamonds can be inferred from the ratio of C-12/C-13. It is essential to achieve high spatial and mass resolving power and minimize all sources of signal loss in order to obtain statistically significant measurements. We conducted atom-probe tomography on meteoritic nanodiamonds embedded between layers of Pt. We describe sample preparation, atom-probe tomography analysis, 3D reconstruction, and bias correction. We present new data from meteoritic nanodiamonds and terrestrial standards and discuss methods to correct isotopic measurements made with the atom-probe tomograph. (C) 2015 Elsevier B.V. All rights reserved.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据