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

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Presentation on theme: "Subduction Dynamics: From Initiation to Maturity Mike Gurnis Caltech Mantle Convection Workshop, June, 2005."— Presentation transcript:

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

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

6 Stern & Bloomer, 1992

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8 Billen & Gurnis, 2005

9 Plate has nearly lost all strength in the trench

10 Gurnis et al. 2004

11 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

12 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)

13 viscous resistance, F v fault friction, F f buoyancy, F b tectonic force, F t subduction occurs if F b + F t > F el + F f + F v (modified from McKenzie, 1977) Subduction Dynamics: Driving & Resisting Forces F el

14 Toth & Gurnis, 1998

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

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

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

18 Homogeneous 30 Myr Plate

19 Underthrusting Overriding Homogeneous, 30 Myr Plate

20 Stern & Bloomer, 1992

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22 10 Ma – 40 Ma Fracture Zone

23 Hall et al., 2003

24 Evolution of topography for 10 Ma – 40 Ma Fracture Zone Model

25 Evolution of Forces 40 Ma Plate 10 Ma Plate

26 Plastic Yielding Envelopes  y = C +  n  y yield strength C cohesion  coeff. of friction Normal ‘unfaulted’ lithosphere Fault zone

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

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

29 0 Ma40 Ma Map View Side View

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

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

33 Estimate Resistance at ~55 Ma Total resistance over 2500 km of plate boundary is 2x10 19 N (Hall et al., 2003). Small compared to current driving forces (2x10 21 N globally, value from Conrad & Lithgow-Bertelloni, 2002)

34 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

35 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

36 Coupling With Pyre

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

38 Regional CitcomS coupled to full CitcomS

39 Examples of coupling codes with Pyre (“superstructure” framework): GeoFramework Pyre CitcomSSNACpHMelts a geophysics solver Exchanger

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

41 Billen et al. 2003

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

43 (Asimow et al., 2004; Ghiorso et al., 2002) 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

44 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

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

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

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