Dynamic topography inferred from global continental hiatus surfaces as a tool for constraining global mantle circulation models

dc.contributor.author
Vilacís, Berta
dc.date.accessioned
2026-01-31T00:43:53Z
dc.date.available
2026-01-31T00:43:53Z
dc.date.issued
2024-06-27
dc.identifier
Vilacís, B. Dynamic topography inferred from global continental hiatus surfaces as a tool for constraining global mantle circulation models. A: Severo Ochoa Research Seminars at BSC. «9th Severo Ochoa Research Seminar Lectures at BSC, Barcelona, 2023-24». Barcelona: Barcelona Supercomputing Center, 2024, p. 112-113.
dc.identifier
https://hdl.handle.net/2117/452091
dc.identifier.uri
http://hdl.handle.net/2117/452091
dc.description.abstract
Mantle convection is a fundamental process governing the evolution of our planet. Buoyancies in the mantle induce horizontal and vertical motion of the Earth’s lithosphere which leave an imprint on the geological record. Positive surface deflections induced by mantle convection create erosional/non-depositional environments which lead to gaps (hiatuses) in the stratigraphic record, while negative deflections provide accommodation space for sedimentation to occur. Thus, by mapping hiatus and no-hiatus signals on inter-continental scales at timescales of geological series (ten to tens of millions of years), one gains a proxy for the long-wavelength uplift and subsidence associated with dynamic topography. Here, we present the global continental hiatus surfaces since the Upper Jurassic and their links to known mantle dynamic events. For example, we tend to observe the appearance of a hiatus surface, indicating an uplift of the lithosphere, before the arrival of a mantle plume. In Europe, we mapped a large-scale sedimentary hiatus during the Paleocene (~66- 56 Million years ago), prior to the arrival of the Iceland plume. We then use these maps as a constrain on mantle circulation models (MCMs), which make predictions of the history of dynamic topography. To make such comparison, we filter the modelled dynamic topography through the geological lenses and obtain the synthetic hiatus maps which are directly comparable to the true maps. By generating synthetic hiatus maps for a variety of high-resolution TERRA MCMs, we show that such maps alow for falsification or verifications of MCMs based on their prediction of dynamic uplift/subsidence events. Our results imply that a key property of time-dependent geodynamic Earth models must be a difference in timescale between mantle convection itself and resulting dynamic topography. Moreover, they highlight the importance of continental-scale compilations of geological data to map the temporal evolution of mantle flow beneath the lithosphere.
dc.format
2 p.
dc.format
application/pdf
dc.language
eng
dc.publisher
Barcelona Supercomputing Center
dc.rights
http://creativecommons.org/licenses/by-nc-nd/4.0/
dc.rights
Open Access
dc.subject
Àrees temàtiques de la UPC::Informàtica::Arquitectura de computadors
dc.subject
High performance computing
dc.subject
Càlcul intensiu (Informàtica)
dc.title
Dynamic topography inferred from global continental hiatus surfaces as a tool for constraining global mantle circulation models
dc.type
Conference report


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