EGU25-16667, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-16667
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Friday, 02 May, 11:00–11:10 (CEST)
 
Room -2.43
In a Spin: Raman spectroscopy on organic-carbon in fault zones
Clare Bond1, Alexander O'Donnell1, Rebecca Robertson2, David Muirhead1, and Catriona Menzies2
Clare Bond et al.
  • 1Aberdeen, Geology and Geophysics, Aberdeen, United Kingdom of Great Britain – England, Scotland, Wales (clare.bond@abdn.ac.uk)
  • 2Durham University, Durham, United Kingdom of Great Britain – England, Scotland, Wales

Over the past decade raman spectroscopy has been used to investigate an increasing range of geological challenges. It’s application in fault zones to track strain is an emerging area. Difficulties in the applications of raman spectroscopy to fault zones stem from deciphering the effects of the multitude of processes occurring in a fault zone on carbon structure and hence raman spectroscopy. Here we consider a range of raman data acquired from fault zones, the processes occurring in the fault zones and how these could influence the raman spectroscopy signal. Our samples include carbonaceous material from natural brittle and ductile fault zones as well as synthetic fault gouge and show that if we are to successfully use raman spectroscopy to determine strain in fault zones we need to better understand fault zone processes and their interaction with carbonaceous material.   

How to cite: Bond, C., O'Donnell, A., Robertson, R., Muirhead, D., and Menzies, C.: In a Spin: Raman spectroscopy on organic-carbon in fault zones, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-16667, https://doi.org/10.5194/egusphere-egu25-16667, 2025.