News Facilities People Research Education GeoHome Rice home page Image Map - If you are viewing with images off, check the bottom of the page for links.  Otherwise, click the location that you would like to go to

RESEARCH PAGES: Short Red Bar

Research by topic

Faculty research pages

World tour (large images)

Research sites within the department

Studying Submarine Accretionary Prisms in a "Numerical Sandbox"

Investigator : Julia K. Morgan

Funding Source: NSF Grant OCE96-18198


Snapshot of the final state of a compressional "experiment" in a numerical sandbox. Assemblage has deformed by displacement of left-hand wall to the right, compressing the system and causing slip along the basal decollement surface. Particle configurations show cumulative displacements of particles resulting final wedge geometry. Displacement vectors indicate portions of the system which displaced within the last increment of strain. Displacement gradients denote discontinuities, i.e., instantaneous fault surfaces; fore thrusts and back thrusts can be observed, as well as the advancing deformation front and protothrust zone. Average particle differential stresses (darker colors) increase as the wedge grows, and principal stress orientations (vectors) rotate to become subhorizontal once the deformation front progresses past them.


Abstract

Submarine accretionary prisms are composed largely of poorly consolidated sediments, particularly near the toe. Field and laboratory observations have shown that these sediments can display both brittle and ductile behavior, depending on local stress conditions, stress history, and physical properties of the sediment. This complexity in deformation behavior of accreted sediments has stymied many attempts to develop numerical models for the study of accretionary processes; continuum models may capture the overall geometry of the prism, but cannot reproduce the complex structure and evolution of natural prisms.

A numerical technique known as the distinct element method (DEM) provides a way to simulate accretionary prisms as discontinuous systems, e.g., assemblages of particles that interact individually with eachother to generate the behavior of the whole. Because particles obey simple physical laws of interaction, the technique defines rather than relies on the constitutive behavior of the assemblage. In this "numerical sandbox", it becomes possible to explore relationships among sediment properties, local stress conditions, deformation mode, and prism structure. As a test of the feasibility of this technique, a series of DEM simulations were conducted using several thousand particles within compressional boundaries. These simulations qualitatively reproduce the behavior and geometries of natural prisms. Depending on material strength, the prism grows by smooth advance of the deformation front (ductile deformation) or by formation and propagation of discrete frontal thrust faults (brittle deformation); broad folds form above thrust faults; out-of-sequence thrusts displace faults and strata within the prism. Estimates of prism taper show variations with internal and basal friction in approximate agreement with critical Coulomb wedge theory.



RiceInfo GeoHome Education Research People Facilities News

Rice University
Department of Geology and Geophysics, MS-126
6100 Main St
Houston, TX 77005-1892
geol@rice.edu
Tel. (713) 348-4880, Fax (713) 348-5214.

Comments? E-mail the
webmaster
Last updated 1 November, 2000 by dale@rice.edu