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Three-dimensional numerical simulations of crustal deformation and subcontinental mantle convection

dc.contributor.authorMoresi, LNen
dc.contributor.authorLenardic, Aen
dc.date.accessioned2026-01-01T10:42:22Z
dc.date.available2026-01-01T10:42:22Z
dc.date.issued1997en
dc.description.abstract3-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.statusPeer-revieweden
dc.format.extent11en
dc.identifier.issn0012-821Xen
dc.identifier.otherWOS:A1997XZ77900005en
dc.identifier.otherORCID:/0000-0003-3685-174X/work/162950309en
dc.identifier.scopus0031428003en
dc.identifier.urihttps://hdl.handle.net/1885/733799881
dc.language.isoenen
dc.sourceEarth and Planetary Science Lettersen
dc.subjectMohorovicic discontinuityen
dc.subjectContinentsen
dc.subjectGravity anomaliesen
dc.subjectIsostasyen
dc.subjectMantleen
dc.subjectOrogenyen
dc.subjectTectonicsen
dc.titleThree-dimensional numerical simulations of crustal deformation and subcontinental mantle convectionen
dc.typeJournal articleen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage243en
local.bibliographicCitation.startpage233en
local.contributor.affiliationMoresi, LN; Climate and Ocean Geoscience, Research School of Earth Sciences, ANU College of Science and Medicine, The Australian National Universityen
local.identifier.citationvolume150en
local.identifier.doi10.1016/S0012-821X(97)00093-9en
local.identifier.pure00adbded-a8ff-4573-8e9b-d4d5c2840676en
local.identifier.urlhttps://www.webofscience.com/api/gateway?GWVersion=2&SrcApp=anu_research_portal_plus2&SrcAuth=WosAPI&KeyUT=WOS:A1997XZ77900005&DestLinkType=FullRecord&DestApp=WOS_CPLen
local.type.statusPublisheden

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