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Boundary Layers in the Mantle; a Tomographer’s View Adam M. Dziewoński VLAB Workshop, August 10, 2007 In cooperation with: Gőran Ekstrőm Yu Jeffrey Gu Bogdan Kustowski
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Boundary Layers in the Mantle; a Tomographer’s View

Jan 11, 2016

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Boundary Layers in the Mantle; a Tomographer’s View. Adam M. Dziewo ń ski. In cooperation with: G ő ran Ekstr ő m Yu Jeffrey Gu Bogdan Kustowski. VLAB Workshop, August 10, 2007. ScS – S elephant; the need for global 3-D thinking. Power spectra of three recent models. - PowerPoint PPT Presentation
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Page 1: Boundary Layers in the Mantle; a Tomographer’s View

Boundary Layers in the Mantle;

a Tomographer’s View

Adam M. Dziewoński

VLAB Workshop, August 10, 2007

In cooperation with:Gőran EkstrőmYu Jeffrey GuBogdan Kustowski

Page 2: Boundary Layers in the Mantle; a Tomographer’s View

ScS – S elephant;the need for global 3-D

thinking

Page 3: Boundary Layers in the Mantle; a Tomographer’s View

Power spectra of three recent models

Harvard Caltech Berkeley

Surface

T.Z.

C.M.B

Page 4: Boundary Layers in the Mantle; a Tomographer’s View

Power spectra of the three models;

a closer look Harvard Caltech Berkeley

Page 5: Boundary Layers in the Mantle; a Tomographer’s View

It cannot be that simple

Grand et al., 1997

Page 6: Boundary Layers in the Mantle; a Tomographer’s View

Diverse data sets is what

made the progress possible

Page 7: Boundary Layers in the Mantle; a Tomographer’s View

Data – the critical element

Three types of data are needed: 1. Fundamental mode surface waves to resolve the near surface structure;

2. Overtone data to resolve structure in the transition zone and

3. Travel time data to resolve the lower mantle structure.

Only three research groups (Berkeley, Caltech/Oxford and Harvard) use this, or equivalent, combination of data

Page 8: Boundary Layers in the Mantle; a Tomographer’s View

Fundamental mode surface waves

Rayleigh 75 seconds

Love35 seconds

Page 9: Boundary Layers in the Mantle; a Tomographer’s View

Sensitivity kernels

from Nettles (2005)

Page 10: Boundary Layers in the Mantle; a Tomographer’s View

Long-period body wave waveforms

from Gu et al. (2001)

Page 11: Boundary Layers in the Mantle; a Tomographer’s View

Mantle wave waveforms

from Gu et al. (2001)

Page 12: Boundary Layers in the Mantle; a Tomographer’s View

Rayleigh waves 1-D sensitivity kernels

from Ritsema et al., 2004

Page 13: Boundary Layers in the Mantle; a Tomographer’s View

Body wave travel times

Page 14: Boundary Layers in the Mantle; a Tomographer’s View

CMB 650 km Moho

Depth resolution of different data subsets

Page 15: Boundary Layers in the Mantle; a Tomographer’s View

Models from different data subsets

120 km

600 km

1600 km

2800 km

After Ritsema et al., 2004

Page 16: Boundary Layers in the Mantle; a Tomographer’s View

Surface Boundary Layer

Page 17: Boundary Layers in the Mantle; a Tomographer’s View

Velocity

lowattenuation

highattenuation

Attenuation

Recent velocity modelsare very well correlatedin the top 200 km, or so, of the mantle

Page 18: Boundary Layers in the Mantle; a Tomographer’s View

Radial anisotropyS-velocity at 150 km

Azimuthal anisotropy75 sec Rayleigh waves

Page 19: Boundary Layers in the Mantle; a Tomographer’s View

From Peru Trench to Japan Trench

from Nettles, 2005

Page 20: Boundary Layers in the Mantle; a Tomographer’s View

Thickness of the continental lithosphere/tectosphere

Page 21: Boundary Layers in the Mantle; a Tomographer’s View

Shapiro & Ritzwoller (2002)

Very sharp bottom of the cratonic lithosphere

From Kustowski et al. (2006)

Page 22: Boundary Layers in the Mantle; a Tomographer’s View

Questions:• What processes cause radial anisotropy in a 100 Ma old oceanic lithosphere at a depth of 150 km?

• Why are the isotropic velocity anomalies correlated with the age of the oceanic plate down to a depth of 200 km, even though plate cooling models prefer 100 km thickness?

• What is the thickness of the continental lithosphere

Page 23: Boundary Layers in the Mantle; a Tomographer’s View

Transition Zone

Page 24: Boundary Layers in the Mantle; a Tomographer’s View

Degree-2 Upper Mantle SignalShifts of the Spectral Peaks Plotted at the Pole Positions

Masters et al., 1982

Page 25: Boundary Layers in the Mantle; a Tomographer’s View

Stagnant slabs are common

from Fukao et al. (2001)

Page 26: Boundary Layers in the Mantle; a Tomographer’s View

Patterns of velocity anomalies above and below the 670 km discontinuity are not similar

From Gu et al. (2001)

Page 27: Boundary Layers in the Mantle; a Tomographer’s View

Power spectra of three modelswith good depth resolution

Harvard Caltech Berkeley

Page 28: Boundary Layers in the Mantle; a Tomographer’s View

600 km depth

800 km depth

Harvard Caltech Berkeley

Page 29: Boundary Layers in the Mantle; a Tomographer’s View

Additionalevidence

Change in the stress pattern near the 650 km discontinuity

Page 30: Boundary Layers in the Mantle; a Tomographer’s View

Model S362ANIDepth 750 km

Strong, but spatially limited fast anomalies in the lower mantle may represent regions of limited penetration of subducted material accumulated in the transition zones

l

Page 31: Boundary Layers in the Mantle; a Tomographer’s View

Pacific “superplume”

Romanowicz and Gung, 2002

QRLf12

(Q-1)

SAW24B16

(Vs)

The slow velocities in a superplume andhigh attenuation in the transition zonecould be explained if transition zone isalso a thermal boundary layer.

EPR

Page 32: Boundary Layers in the Mantle; a Tomographer’s View

Two stage plume generation

Courtillot et al. (2003)

Page 33: Boundary Layers in the Mantle; a Tomographer’s View

Conclusions• Overtone/waveform data are critical for resolution of the transition zone structure.

• The change in the spectrum across the discontinuity is as sharp as can be resolved at the present time.

• We conclude that the transition zone is a boundary layer that could be penetrated by episodic events, but does not permit steady state circulation across the 650 km discontinuity.

Page 34: Boundary Layers in the Mantle; a Tomographer’s View

Lowermost Mantle

Page 35: Boundary Layers in the Mantle; a Tomographer’s View

Dziewonski, 1984

Page 36: Boundary Layers in the Mantle; a Tomographer’s View

Equatorial Cross-section

Dziewonski (1984) and Woodhouse and Dziewonski (1984)

Page 37: Boundary Layers in the Mantle; a Tomographer’s View

Megaplumes span whole lower

mantle

3-D view of +0.5% and -0.5% isosurfaceof S-velocity modelof Masters et al. (2000). The uppersurface is truncated at 800 km depthand lower – at CMB

Page 38: Boundary Layers in the Mantle; a Tomographer’s View

Usually, models of the shear and compressional velocity are obtained independently. However, P-velocity depends both on shear modulus and bulk modulus. To isolate this interdependence, Su and Dziewonski (1997) formulated the inverse problem for a joint data set and derived 3-D perturbations of bulk sound velocity and shear velocity

Model of shear and bulk sound velocities

Page 39: Boundary Layers in the Mantle; a Tomographer’s View

K-μ Inversion550 km Depth

At this depth, the shear and bulk sound velocities show high correlation; both show fast values in the Western Pacific and South America, likely associated with the ponding of subducted slabs.

Page 40: Boundary Layers in the Mantle; a Tomographer’s View

K-μ Inversion2800 km Depth

Near the CMB, there is a distinct negative correlation between K/ρ and μ/ρ under the Pacific and African Superplumes.

Page 41: Boundary Layers in the Mantle; a Tomographer’s View

Bulk Sound and Shear Velocity Anomalies

Correlation between the bulk sound and shear velocity anomalies changes from +0.7 in the transition zone to –0.8 in the lowermost mantle. From Su and Dziewonski, 1997.

Page 42: Boundary Layers in the Mantle; a Tomographer’s View

K-μ Inversion2800 km Depth

In the vicinity of the “China High”, the correlation remains positive. This is likely an expression of compositional heterogeneity, perhaps, combined with a thermal one.

Page 43: Boundary Layers in the Mantle; a Tomographer’s View

Questions:

• How have the super-plumes formed?• What part of the anomalies is caused by compositional rather than thermal variations?

• Why do the super-plumes continue across the D” without an apparent change in the amplitude of the anomaly?