| Facilities |
raman spectrometers of Laboratoire de Sciences de la Terre are national instruments
supported by Institut des Sciences de L Univers and therefore to work with one of this machine :
- consult the [facilities]
booking system
- send us an email [raman@geologie-lyon.fr]
Pressure calculation
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[wavelength in cm-1]
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[wavelength in nm]
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| To send spectrum |
| to help us to increase this data base, fill
[this form]
and send new spectrum file |
| Links |
The Rruff Project website containing an integrated database of Raman spectra, X-ray diffraction and chemistry
data for minerals
[link]
Raman Mineral Spectroscopy Server (Caltech)
[link]
Raman Spectra Minerals (University of Parma)
[link]
Raman data base of minerals (SFMC)
[link]
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Laser spot on a Pyrite sample
Raman spectroscopy can be used
to identify, with a minimum of preparation, minerals, glasses and fluids
in geological samples
[LST].
We therefore present a selection of Raman spectra of minerals representative
of some major mineral groups
[use search engine]. The spectra provide the main vibrational
fingerprints of each main mineral group and related minerals. We report
here more recent references and references for Raman studies carried out
at high-pressures and high-temperatures are also mentionned. Most of the spectra
were recorded on a XY ©DILOR Raman microspectrometer equipped with
a CCD detector [Picture].
The spectrometer was used in backscattering geometry. The laser
beam (488 or 514.5
nm exciting lines of a Spectra Physics® Ar+ laser) was
focussed through microscope objectives (x50) down to a 2 micrometer
spot on sample and the backscattered light was collected through the
same objective.
Even though polarization effects are minimized, the intensity of the
Raman modes can be sensitive to crystal orientation.
| Instruments |
| spectrometer |
laser source |
Labram HR800 vis Jobin Yvon Horiba
semi-confocal microscope - mapping stage |
Spectra Physics® 2018
Ar+/Kr+ 647.1 nm 514.5nm 457.9nm
HeNe 632.8nm |
Labram HR800 vis Jobin Yvon Horiba
confocal microscope and fiber entrance |
Spectra Physics® 2017
Ar+ 514.5nm
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| Labram HR800 UV Jobin Yvon Horiba |
Spectra Physics®
WaveTrain 244nm |
| XY Dilor |
Spectra Physics® 177G
Ar+ 514.5nm 488nm 457.9nm |
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