EGU24-20543, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-20543
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Do gas fluxes from numerical modeling and from field data match ?

Marielle Collombet1, Alain Burgisser2, Didier Bresch3, and Gladys Narbona Reina4
Marielle Collombet et al.
  • 1ISTerre, Université Savoie Mont Blanc, Le Bourget du Lac, France (marielle.collombet@univ-smb.fr)
  • 2ISTerre, CNRS, Université Savoie Mont Blanc, Le Bourget du Lac, France (alain.burgisser@univ-smb.fr)
  • 3LAMA, CNRS, Université Savoie Mont Blanc, Le Bourget du Lac, France (didier.bresch@univ-smb.fr)
  • 4E.T.S Arquitectura, Universidad de Sevilla, Sevilla, Spain (gnarbona@us.es)

Modeling magma ascent within volcanic conduits is not an easy task since it involves complex physical interactions between melt, crystals and gas. Since the evolution of gas content mainly controls the eruptive dynamics, we have to do our best to understand and quantify how and when this gas phase exsolves from the melt, expands and finds its way toward the surface, possibly independently from the melt. In order to follow these phenomena with time, we developed a new 1.5D two-phase system which takes, among others, effects of pressure, temperature, volatile exchanges (including diffusion and viscous relaxation) between the melt and gas phases into account. First tests with this numerical model have then been conduced in order to see if we manage to reproduce gas content and gas fluxes prior to the July 2013 vulcanian eruption at Tungurahua volcano in Ecuador.

How to cite: Collombet, M., Burgisser, A., Bresch, D., and Narbona Reina, G.: Do gas fluxes from numerical modeling and from field data match ?, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-20543, https://doi.org/10.5194/egusphere-egu24-20543, 2024.