Three-dimensional numerical simulations of crustal deformation and subcontinental mantle convection
| dc.contributor.author | Moresi, LN | en |
| dc.contributor.author | Lenardic, A | en |
| dc.date.accessioned | 2026-01-01T10:42:22Z | |
| dc.date.available | 2026-01-01T10:42:22Z | |
| dc.date.issued | 1997 | en |
| dc.description.abstract | 3-D simulations of mantle convection allowing for continental crust are explored to study the effects of crustal thickening on lithosphere stability and of continents on large-scale mantle flow. Simulations begin with a crustal layer within the upper thermal boundary layer of a mantle convection roll in a 1 x 1 x 1 Cartesian domain. Convective stresses cause crust to thicken above a sheet-like mantle downwelling. For mild convective Vigor an initial crustal thickness Variation is required to induce 3-D lithospheric instability below the zone of crustal convergence. The amplitude of the required Variation decreases with increasing convective vigor. Morphologically, instability is manifest in the formation of drip-like thermals that exist within the large-scale roll associated with initial crustal thickening. A strong surface signature of the drips is their ability to cause deviations from local Airy compensation of topography. After the initial thickening phase, the crustal accumulation that forms serves as a model analog to a continent. Its presence leads to mantle flow patterns distinctly different from the steady-state roll that results in its absence. Large lateral thermal gradients are generated at its edge allowing this region to be the initiation site for continued small-scare thermal instabilities. Eventually these instabilities induce a restructuring of large-scale mantle flow, with the roll pattern being replaced by a square cell. Although preliminary and idealized, the simulations do show the fluid dynamical plausibility behind the idea that significant mantle variations can be generated along the strike of a largely 2-D mountain chain by the formation of the chain itself. The ability of a model continent to cause a change in fundamental convective planform also suggests that the effects of continental crust on mantle convection may be low-order despite the seemingly trivial volume of crust relative to mantle. (C) 1997 Elsevier Science B.V. | en |
| dc.description.status | Peer-reviewed | en |
| dc.format.extent | 11 | en |
| dc.identifier.issn | 0012-821X | en |
| dc.identifier.other | WOS:A1997XZ77900005 | en |
| dc.identifier.other | ORCID:/0000-0003-3685-174X/work/162950309 | en |
| dc.identifier.scopus | 0031428003 | en |
| dc.identifier.uri | https://hdl.handle.net/1885/733799881 | |
| dc.language.iso | en | en |
| dc.source | Earth and Planetary Science Letters | en |
| dc.subject | Mohorovicic discontinuity | en |
| dc.subject | Continents | en |
| dc.subject | Gravity anomalies | en |
| dc.subject | Isostasy | en |
| dc.subject | Mantle | en |
| dc.subject | Orogeny | en |
| dc.subject | Tectonics | en |
| dc.title | Three-dimensional numerical simulations of crustal deformation and subcontinental mantle convection | en |
| dc.type | Journal article | en |
| dspace.entity.type | Publication | en |
| local.bibliographicCitation.lastpage | 243 | en |
| local.bibliographicCitation.startpage | 233 | en |
| local.contributor.affiliation | Moresi, LN; Climate and Ocean Geoscience, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National University | en |
| local.identifier.citationvolume | 150 | en |
| local.identifier.doi | 10.1016/S0012-821X(97)00093-9 | en |
| local.identifier.pure | 00adbded-a8ff-4573-8e9b-d4d5c2840676 | en |
| local.identifier.url | https://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=anu_research_portal_plus2&SrcAuth=WosAPI&KeyUT=WOS:A1997XZ77900005&DestLinkType=FullRecord&DestApp=WOS_CPL | en |
| local.identifier.url | https://www.scopus.com/pages/publications/0031428003 | en |
| local.type.status | Published | en |