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ID 61839
フルテキストURL
著者
Hagiwara, Yuuki Graduate School of Science, Hokkaido University
Yoshida, Kenta Research Institute for Marine Geodynamics, Japan Agency for Marine-Earth Science and Technology (JAMSTEC)
Yoneda, Akira Institute for Planetary Materials, Okayama University
Torimoto, Junji Ore Genesis Research Unit, Project Team for Development of New-Generation Research Protocol for Submarine Resources, Japan Agency for Marine-Earth Science and Technology (JAMSTEC)
Yamamoto, Junji The Hokkaido University Museum
抄録
Raman spectroscopy for fluid, melt, and mineral inclusions provides direct insight into the physicochemical conditions of the environment surrounding the host mineral at the time of trapping. However, the obtained Raman spectral characteristics such as peak position are modified because of local temperature enhancement of the inclusions by the excitation laser, which might engender systematic errors and incorrect conclusions if the effect is not corrected. Despite the potentially non-negligible effects of laser heating, the laser heating coefficient (B) (°C/mW) of inclusions has remained unsolved. For this study, we found B from experiments and heat transport simulation to evaluate how various parameters such as experimental conditions, mineral properties, and inclusion geometry affect B of inclusions. To assess the parameters influencing laser heating, we measured B of a total of 19 CO2-rich fluid inclusions hosted in olivine, orthopyroxene, clinopyroxene, spinel, and quartz. Our results revealed that the measured B of fluid inclusions in spinel is highest (approx. 6 °C/mW) and that of quartz is lowest (approx. 1 × 10−2 °C/mW), consistent with earlier inferences. Our simulation results show that the absorption coefficient of the host mineral is correlated linearly with B. It is the most influential parameter when the absorption coefficient of the host mineral (αh) is larger than that of an inclusion (αinc). Furthermore, although our results indicate that both the inclusion size and depth have little effect on B if αh > αinc, the thickness and radius of the host mineral slightly influence B. These results suggest that the choice of inclusion size and depth to be analyzed in a given sample do not cause any systematic error in the Raman data because of laser heating, but the host radius and thickness, which can be adjusted to some degree at the time of sample preparation, can cause systematic errors between samples.Our results demonstrate that, even with laser power of 10 mW, which is typical for inclusion analysis, the inclusion temperature rises to tens or hundreds of degrees during the analysis, depending especially on the host mineral geometry and optical properties. Therefore, correction of the heating effects will be necessary to obtain reliable data from Raman spectroscopic analysis of inclusions. This paper presents some correction methods for non-negligible effects of laser heating.
キーワード
Finite element method
Inclusions
Laser heating
Raman spectroscopy
発行日
2021-01-05
出版物タイトル
Chemical Geology
559巻
出版者
Elsevier
開始ページ
119928
ISSN
00092541
NCID
AA0060201X
資料タイプ
学術雑誌論文
言語
英語
OAI-PMH Set
岡山大学
著作権者
© 2020 The Authors.
論文のバージョン
publisher
NAID
DOI
Web of Science KeyUT
関連URL
isVersionOf https://doi.org/10.1016/j.chemgeo.2020.119928
ライセンス
http://creativecommons.org/licenses/by/4.0/
Citation
Yuuki Hagiwara, Kenta Yoshida, Akira Yoneda, Junji Torimoto, Junji Yamamoto, Experimental variable effects on laser heating of inclusions during Raman spectroscopic analysis, Chemical Geology, Volume 559, 2021, 119928, ISSN 0009-2541, https://doi.org/10.1016/j.chemgeo.2020.119928.
助成機関名
日本学術振興会
助成番号
17K18794
17H02994
16H04079
P19J21537
オープンアクセス(出版社)
OA
オープンアーカイブ(出版社)
非OpenArchive