Raman spectroscopic measurements of CO2 density: Experimental calibration with high-pressure optical cell (HPOC) and fused silica capillary capsule (FSCC) with application to fluid inclusion observations

被引:146
|
作者
Wang, Xiaolin [1 ]
Chou, I. -Ming [2 ]
Hu, Wenxuan [1 ]
Burruss, Robert C. [3 ]
Sun, Qiang [4 ]
Song, Yucai [5 ]
机构
[1] Nanjing Univ, State Key Lab Mineral Deposits Res, Sch Earth Sci & Engn, Nanjing 210093, Peoples R China
[2] US Geol Survey, Natl Ctr 954, Reston, VA 20192 USA
[3] US Geol Survey, Natl Ctr 955, Reston, VA 20192 USA
[4] Peking Univ, Sch Earth & Space Sci, Beijing 100871, Peoples R China
[5] China Acad Geol Sci, Inst Geol, Beijing 100037, Peoples R China
基金
中国国家自然科学基金;
关键词
PHASE-EQUILIBRIA; MANTLE XENOLITHS; GOLD DEPOSIT; MIXTURES; GEOBAROMETRY; DENSIMETER; PREDICTION; CLATHRATE; QUARTZ; BELT;
D O I
10.1016/j.gca.2011.04.028
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Raman spectroscopy is a powerful method for the determination of CO2 densities in fluid inclusions, especially for those with small size and/or low fluid density. The relationship between CO2 Fermi diad split (Delta, cm(-1)) and CO2 density (rho, g/cm(3)) has been documented by several previous studies. However, significant discrepancies exist among these studies mainly because of inconsistent calibration procedures and lack of measurements for CO2 fluids having densities between 0.21 and 0.75 g/cm3, where liquid and vapor phases coexist near room temperature. In this study, a high-pressure optical cell and fused silica capillary capsules were used to prepare pure CO2 samples with densities between 0.0472 and 1.0060 g/cm(3). The measured CO2 Fermi diad splits were calibrated with two well established Raman bands of benzonitrile at 1192.6 and 1598.9 cm(-1). The relationship between the CO2 Fermi diad split and density can be represented by: rho = 47513.64243 - 1374.824414 x Delta + 13.25586152 x Delta(2) - 0.04258891551 x Delta(3) (r(2) = 0.99835, r = 0.0253 g/cm(3)), and this relationship was tested by synthetic fluid inclusions and natural CO2-rich fluid inclusions. The effects of temperature and the presence of H2O and CH4 on this relationship were also examined. (C) 2011 Elsevier Ltd. All rights reserved.
引用
收藏
页码:4080 / 4093
页数:14
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