Abstract
Crustal-derived rocks can be subducted to mantle depth and metamorphosed at ultra-high pressure conditions (>2.6 GPa and 600 \(^{\circ }\)C), which are defined by the presence of coesite . Findings of diamond in metamorphic rocks further extended the upper pressure limit for crustal rocks (>4.0 GPa and 900–1000 \(^{\circ }\)C). Almost all ultra-high pressure mineral-indicators occur as small relics and Raman spectroscopy is a very powerful tool for the identification of these relics. Despite the significant progress in Raman imaging, this technique remains underestimated in ultra-high pressure research. In this chapter several examples of Raman imaging applied in ultra-high pressure petrology are summarised and discussed.
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Notes
- 1.
The measured depth in this image is about 5 \( \upmu \mathrm{m}\) and this needs to be multiplied with the refractive index of Garnet to obtain the approximate correct value.
- 2.
Mg#: The magnesium number (Mg/(Mg+Fe)) is commonly used in petrology for the calculation of the temperature. The calculation itself can be quite complicated, while Mg# can be considered as “raw” data.
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Acknowledgements
This study was supported by a grant from the Russian Science Foundation (RSF 15-17-30012).
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Korsakov, A.V. (2018). Application of Raman Imaging in UHPM Research. In: Toporski, J., Dieing, T., Hollricher, O. (eds) Confocal Raman Microscopy. Springer Series in Surface Sciences, vol 66. Springer, Cham. https://doi.org/10.1007/978-3-319-75380-5_11
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