[This post is participating at the 2015 Student Presentation Awards at ICTJA]
Fig. 1 Geological cross section of the frontal part of the South Pyrenean fold and thrust belt.

The comparison of the obtained
results with those obtained in previous works by other authors in nearby areas will
allow us to perform the fluid flow model of the frontal part of the South
Pyrenean fold and thrust belt.
Fig. 2 Schemes of the
structural and fluid flow evolution of the Puig-reig anticline. Red and blue
arrows indicate fluid movement. No vertical exaggeration. A) Fluid flow during
the early folding. Hot evolved meteoric fluids migrated along the main faults
and more permeable sedimentary units. B) Fluid flow during the main stage of
folding. During this event, local meteoric fluids circulated downwards the
normal faults formed by outer arc extension and mixed with the evolved meteoric
fluids.
This work is supervised by Dr. Jaume Vergés (Group of Dynamics of The Litosphere - GDL, ICTJA - CSIC) and by Dr. Anna Travé (Grup de Geologia Sedimentària, Department of Geochemistry, Petrology and Geological Prospecting - UB).
This work is supervised by Dr. Jaume Vergés (Group of Dynamics of The Litosphere - GDL, ICTJA - CSIC) and by Dr. Anna Travé (Grup de Geologia Sedimentària, Department of Geochemistry, Petrology and Geological Prospecting - UB).
No comments:
Post a Comment