In a paper published in Nature, Rakib Hassan with fellow EarthByters Dietmar Müller, Simon E. Williams & Nicolas Flament, and Caltech’s Michael Gurnis, proposed a solution to a long standing geological mystery – how the distinct bend in the Hawaiian-Emperor Seamount Chain came to be. Using NCI’s Raijin supercomputer, the research team simulated flow patterns in the Earth’s mantle over the past 100 million years. The convection model suggests that the history of subduction has a profound effect on the time-dependent deformation of the edges of the Large Low-Shear Velocity Province (LLSVP) under the Pacific. The Hawaiian plume originates from the edge of this province and the southward migration of the plume during the formation of the Emperor chain reflects the migration of the northern edge of the LLSVP before ~47 million years ago.
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Tectonic evolution of Western Tethys from Jurassic to present day: coupling geological and geophysical data with seismic tomography models
Author List: Maral Hosseinpour, Simon Williams, Maria Seton, Nicholas Barnett-Moore and Dietmar Müller Citation: Hosseinpour, M., Williams, S., Seton, M., Barnett-Moore, N., and Müller, R.D. (2016). Tectonic evolution of Western Tethys from Jurassic to present day: coupling geological and geophysical data with seismic tomography models. International Geology Review 58 (13): 1616–1645. doi:10.1080/00206814.2016.1183146 Abstract: The geodynamic evolution of the … Read more…