EGU26-14092, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-14092
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Thursday, 07 May, 16:30–16:40 (CEST)
 
Room 0.96/97
The IMPULSE experiment: New oceanic crustal record of thermal plume pulsing of Earth’s strongest mantle plume
Stephen M Jones1, Nirmit Dhabaria2, Tim Henstock3, and Nicky White3
Stephen M Jones et al.
  • 1School of Geography, Earth & Environmental Science, University of Birmingham, UK (s.jones.4@bham.ac.uk)
  • 2School of Ocean & Earth Science, University of Southampton, UK (n.dhabaria@soton.ac.uk; t.j.henstock@soton.ac.uk)
  • 3Department of Earth Science, University of Cambridge, UK (njw10@cam.ac.uk)

Thermal pulsing is thought to be a characteristic process of major mantle convection cells.  Seafloor features near Iceland, known as the "V-Shaped Ridges" (VSRs), may comprise the best record of thermal plume pulsing.  However, a satisfactory test of this thermal plume pulsing model has been compromised by the lack of suitable geophysical and geochemical datasets from the VSRs.  Here, we present the first full crustal seismic image of multiple complete VSR cycles.  In 2024, the IMPULSE experiment acquired an approximately 400 km long profile that straddles the Reykjanes Ridge spreading axis and several V-Shaped Ridge/Trough cycles spanning over 18 million years.  Traveltime picks for crustal and upper mantle refractions and PmP wide-angle Moho reflections were inverted using the TOMO2D software package to obtain crustal thickness as well as crustal and upper mantle seismic velocity.  The results show crustal thickness variations that correlate with VSR geometry.  They also reveal seismic velocity variations which indicate fluctuations in mineralogy of the lower crustal cumulates that correlate with the VSRs.  Mid-ocean ridge basalts sampled by International Ocean Drilling Program Expedition 395 at five sites along the seismic profile show trace element variations that correlate with the VSRs.  Significantly, we have imaged both conjugate flanks of the spreading axis along a plate spreading flowline.  Comparison of conjugate crustal thickness and structure permits us to disentangle primary melt supply processes from asymmetric crustal accretion processes.  The combined geophysical and geochemical dataset supports a model in which the VSRs form when thermal plume pulsing causes fluctuations in the volume and composition of magma supplied to the mid-oceanic ridge, and crustal accretion processes related to oblique spreading at variable rate then modify VSR morphology in different locations.

How to cite: Jones, S. M., Dhabaria, N., Henstock, T., and White, N.: The IMPULSE experiment: New oceanic crustal record of thermal plume pulsing of Earth’s strongest mantle plume, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-14092, https://doi.org/10.5194/egusphere-egu26-14092, 2026.