- 1Energy Research Unit, CSIRO, Australia (peng.guo@csiro.au)
- 2Institut de Physique du Globe de Paris, Université Paris Cité, CNRS, Paris, France
Oceanic transform faults (TFs) are fundamental elements of plate tectonics and have traditionally been viewed as conservative strike-slip boundaries. Seafloor observations and numerical modeling suggest the existence of extensional stress, however how it manifest at depth remains unknown. Moreover, slow-slipping TFs are often associated with thin crust and possible exposures of serpentinised peridotite near the seafloor. Here we apply full waveform inversion (FWI) to a 12-km offset seismic dataset across the Romanche TF, the largest TF on the Earth. The TF along our profile contains 20-km-wide 6 km deep valley with inward steeply dipping bounding faults. Given the steep seafloor topography, we first enhance the refracted waves by applying source-receiver reciprocity and downward continuation to the surface streamer data to mimic an ocean bottom cable survey geometry. We then perform trace-normalized FWI to derive a high-resolution crustal model. Our results reveal low P-wave velocity in the upper 3 km, suggestive of basaltic origin, and no evidence for high velocities characteristic of serpentinised peridotite beneath the valley floor. Moreover, we image inward dipping normal faults extending down to ~4 km depth below the seafloor, forming a flower-like structure. Regional earthquake data reveal both strike-slip and normal-faulting, with strike-slip hypocenters aligning with interpreted faults. These features suggest that the Romanche TF resembles a trans-tensional regime with a deep-rooted strike-slip fault in the middle, and complex faulting in the transform valley, accommodating both plate-scale and local strain deformation.
How to cite: Guo, P. and Singh, S.: Seismic Evidence for Trans-Tensional-Regime at the Romanche Oceanic Transform Fault in the Equatorial Atlantic Ocean, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-21531, https://doi.org/10.5194/egusphere-egu26-21531, 2026.