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Subduction Dynamics: From Initiation to Maturity

This workshop explores the empirical and numerical modeling of subduction dynamics, including topics such as subduction initiation, visco-elastoplastic models of transform faults and subduction, and software needs for future research.

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Subduction Dynamics: From Initiation to Maturity

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  1. Subduction Dynamics: From Initiation to Maturity Mike Gurnis Caltech Mantle Convection Workshop, June, 2005

  2. Outline • Empirically: What’s important for this problem • Visco-elastoplastic models of transform faults & subduction initiation • Chad Hall, Luc Lavier • Some thoughts on software needed for the future • Frameworks: Eh Tan • Coupling scales: Eun-seo Choi • Micro physics coupling to large-scale: Laura Baker, Paula Smith, Chad Hall, Paul Asimow

  3. Evolutionary Model for the formation of the IBM Originally from Hilde et al. [1977] as modified by Stern & Bloomer [ 1992].

  4. Stern & Bloomer, 1992

  5. Billen & Gurnis, 2005

  6. Plate has nearly lost all strength in the trench Billen & Gurnis, 2005

  7. Gurnis et al. 2004

  8. Time-scale of subduction initiation • ~50% of known subduction zones initiated since early Cenozoic • Time-scale for creating new subduction zones 10-100 Myr (SI) • Age of oldest sea floor in Atlantic ~ 180Ma (atl) • Time-scale for continental rearrangements 250-500 Myr (mc) • SI<atl ; SI<<mc

  9. Take home messages for subduction initiation • 50% of SZ initiatiated since early Cenozoic • Elasticity is important during SI, but may not be so after transition to self-sustaining state • Some subduction zones initiate at fracture zones and near old spreading centers • Rapid extension could be important during self-nucleation (Stern model)

  10. Subduction Dynamics:Driving & Resisting Forces fault friction, Ff tectonic force, Ft elastic resistance Fel viscous resistance, Fv buoyancy, Fb subduction occurs if Fb + Ft > Fel + Ff + Fv (modified from McKenzie, 1977)

  11. Toth & Gurnis, 1998

  12. Visco-elastoplastic models of transform faults & subduction initiation With Chad Hall & Luc Lavier

  13. Use an explicit finite difference method to solve the force balance equation Brittle crust (Mohr-Coulomb) Non-linear, temperature dependent viscosity in crust, lithosphere and mantle f C, Plastic strain Method akin to Fast Lagrangian Analysis of Continua (FLAC) [Poliakov and Buck, 1998; Lavier et al., 2000]. A. Poliakov, Y. Podladchikov & Talbot [ 1993] Benchmarked method against Rayleigh-Taylor problem • Explict method • Visco elasto-plastic material • Track plastic strain • Frequent regridding

  14. Conceptual Basis • FLAC (Cundall 1989) • Solve a force balance equation for each node • Explicit finite difference formulation in time

  15. Homogeneous 30 Myr Plate

  16. Homogeneous, 30 Myr Plate Underthrusting Overriding

  17. Stern & Bloomer, 1992

  18. 10 Ma – 40 Ma Fracture Zone

  19. Hall et al., 2003

  20. Evolution of topography for 10 Ma – 40 Ma Fracture Zone Model

  21. Evolution of Forces 40 Ma Plate 10 Ma Plate

  22. Plastic Yielding Envelopes sy = C + msn sy yield strength C cohesion m coeff. of friction Normal ‘unfaulted’ lithosphere Fault zone

  23. Fault Strength and Evolution of Convergence Zones Hall, Gurnis & Lavier < 25 MPa: Localized (Arc in Extensional) > 25 MPa: Localized (Arc in Compression) 60 – 180 MPa: Transition to distributed deformation (buckling)

  24. Fault Strength and Evolution of Convergence Zones Lower Friction (63 MPa) Higher Friction (180 MPa) Hall, Gurnis & Lavier

  25. 0 Ma 40 Ma Map View Side View

  26. Murray Fracture Zone Forward Gravity Models South  North 10 MPa models typically too strong Hall & Gurnis, 2005

  27. Paleo age grids from Mueller and Sdrolias in Hall et al. [2003]

  28. Estimate Resistance at ~55 Ma • Total resistance over 2500 km of plate boundary is 2x1019 N (Hall et al., 2003). • Small compared to current driving forces (2x1021 N globally, value from Conrad & Lithgow-Bertelloni, 2002)

  29. Outcomes of computational models • Reinterpreted Eocene history of IBM. Earlier compressive stage preceded rapid extension • Most intense periods of back-arc extension all followed subduction initiation • Developing explicit test (through IODP) for initiation of Tonga-Kermadec SI

  30. Some thoughts on software needed for the future • Frameworks: Eh Tan • Coupling scales: Eun-seo Choi • Micro physics coupling to large-scale: Laura Baker, Paula Smith, Chad Hall, Paul Asimow

  31. Coupling With Pyre

  32. Regional and Global Mantle Flow Coupled with Pyre CitcomS.py, Eh Tan

  33. Regional CitcomS coupled to full CitcomS CitcomS.py, Eh Tan

  34. Examples of coupling codes with Pyre (“superstructure” framework): GeoFramework Pyre a geophysics solver CitcomS Exchanger SNAC pHMelts

  35. SNAC CitcomS coupling (Crust-Mantle Interaction) Eun-seo Choi et al.

  36. Billen et al. 2003

  37. Cartoon Models of Wedge Melting Formation of water-saturated zone Diapirism of hydrated mantle Baker, Smith, Hall, Gurnis, & Asimow

  38. pHMelts Petrological Model Given composition and state variables, pHMelts will return the assemblage that minimizes free energy Gives partitioning of water to nominally anhydrous minerals (Asimow et al., 2004; Ghiorso et al., 2002)

  39. 17,000 particles Thermodynamic data from pHMelts passed back to solid flow solver: Water content, melt fraction, buoyancy, latent heat - Particles advected by solid flow solver - (P, T, X) are passed to pHMelts

  40. Free water (black contours) passes through saturated zone to generate partial melt (white contours)

  41. Thinning of mechanical boundary layer as water lowers viscosity Initial (temperature-dependent) viscosity structure Feedback between Thermodynamics & Mechanics

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