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Effect of pressure and temperature on Raman shifts of methane in CH_4-H_2O vapor phase

机译:压力和温度对CH_4-H_2O气相中甲烷拉曼偏移的影响

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Raman spectroscopy is an extremely useful tool in fluid inclusion studies; however, it is important to recognize that the characteristics of Raman-active species spectra are associated to their environments, therefore, the pressure and temperature dependence of characteristic Raman spectra of geologic fluids is the key for the correct interpretations of the physico-chemical properties of fluid inclusions. Previous studies of methane-containing gases have shown that methane peak positions shifted to lower wavenumbers with increasing pressure, and such relationship had been used to calculate the pressure of CH_4 vapor in the inclusion near room temperature (Chou et al., 2006). However, little is known about the temperature effect on this Raman shift-pressure relationship. In this study, Raman spectra of methane in the vapor phase for methane-water system were studied at pressures up to 36.82 MPa from room temperature up to 200°C.
机译:拉曼光谱是流体包裹性研究中非常有用的工具;然而,重要的是要认识到拉曼活性物种光谱的特性与其环境相关,因此,地质流体的特征拉曼光谱的压力和温度依赖性是正确解释物理化学性质的关键流体夹杂物。先前的含甲烷气体的研究表明,甲烷峰值位置随着压力的增加而转移到下波数,并且这种关系已经用于计算夹杂物附近的CH_4蒸汽的压力(Chou等,2006)。然而,关于这种拉曼移位压力关系的温度效应很少。在该研究中,在高达200℃的压力下,在高达36.82MPa的压力下研究了甲烷 - 水系统的气相中的甲烷的拉曼光谱。

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