Numerical models of the evolution of accretionary wedges and fold-and-thrust belts using the distinct-element method

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dc.contributor.authorBurbidge, D.
dc.contributor.authorBraun, Jean
dc.date.accessioned2015-12-13T23:24:30Z
dc.date.issued2002
dc.date.updated2015-12-12T09:20:44Z
dc.description.abstractA 2-D numerical model is used to investigate the evolution of accretionary wedges and fold-and-thrust belts. The numerical method is based on the distinct-element method (DEM). Unlike many continuum numerical models, DEM allows localization to occur even
dc.identifier.issn0956-540X
dc.identifier.urihttp://hdl.handle.net/1885/92249
dc.publisherBlackwell Publishing Ltd
dc.sourceGeophysical Journal International
dc.subjectKeywords: accretionary prism; collision zone; crustal deformation; distinct element method; fold and thrust belt; normal fault; numerical model Collision belts; Crustal deformation; Faulting; Lateral heterogeneity; Normal faulting; Numerical techniques
dc.titleNumerical models of the evolution of accretionary wedges and fold-and-thrust belts using the distinct-element method
dc.typeJournal article
local.bibliographicCitation.lastpage561
local.bibliographicCitation.startpage542
local.contributor.affiliationBurbidge, D., College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationBraun, Jean, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidBurbidge, D., u4014522
local.contributor.authoruidBraun, Jean, u8901439
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor040313 - Tectonics
local.identifier.ariespublicationMigratedxPub23276
local.identifier.citationvolume148
local.identifier.doi10.1046/j.1365-246x.2002.01579.x
local.identifier.scopusID2-s2.0-0036127319
local.type.statusPublished Version

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