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Seismic velocity gradients across the transition zone

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Presentation on theme: "Seismic velocity gradients across the transition zone"— Presentation transcript:

1 Seismic velocity gradients across the transition zone
CIDER-06 Group B Seismic velocity gradients across the transition zone

2 Participants Fabio Cammarano (UCB) Colleen Dalton (Harvard)
Nico DeKoker (Michigan) Federica Marone (UCB) Antonio Piazzoni (Munich) Barbara Romanowicz (UCB) Yi Wang (SUNY)

3 What have we tried to do? Compute elastic velocity profiles (Vp and Vs) in the upper mantle based on 3 different mineral physics based methods Compare two different compositional models: pyrolite and piclogite Compare fits to seismic data (travel times and modes) Understand where differences are coming from and assess how fits to seismic data can be improved

4 Compositional models (Ita and Stixrude 1992)
Pyrolite (%) MgO SiO FeO Al2O CaO 3.3 Piclogite (%) MgO SiO FeO Al2O CaO Duffy and Anderson, 1989 Anderson and Bass, 1984 Ringwood, 1979

5 Phase diagrams

6 Computation of elastic properties from mineral physics
1) Stixrude and Lithgow-Bertelloni (2005) Gibbs Free Energy Minimization (a) 2) Piazzoni et al. (2006 – submitted to G-cubed) Gibbs Free Energy Minimization (b) 3) Weidner and Wang (1998, 2000) Use directly data from experiments – All use the same temperature profile (1600K potential temperature)

7 Seismic velocity profiles (Vs)
Piro Piclo PREM S&LB Weidner Piazzoni

8 Fit to global dataset of seismic P wave travel times (EHB catalog)

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11 Fit to normal mode data: spheroidal modes

12 Fit to normal mode data: toroidal modes

13 Conclusions: Velocities obtained are too slow
Colder temperature? Velocity gradient in the transition zone is better for piclogite than for pyrolite: Effect of Ca content? Possible effect of water: test using a homologous temperature model

14 Fit to global dataset of seismic P wave travel times (EHB catalog)

15 Test with 150K colder potential temperature
Pyro Piclo PREM S&L 1600K S&L -150K S&L -150K

16 Conclusions (2) What helps – a combination of:
Colder temperatures Effect of convection on adiabats Stagnant slabs? Increase in Ca content (oceanic crust?) What can be improved (future): Elastic properties at high T,P need to be better known Understand better differences between thermodynamic models Effect of water through and on Q Need to include high resolution seismic constraints on velocity jumps at 400 and 660 km.

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18 Attenuation profiles


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