/
Geophysical Inverse Problems Geophysical Inverse Problems

Geophysical Inverse Problems - PowerPoint Presentation

piper
piper . @piper
Follow
66 views
Uploaded On 2023-10-26

Geophysical Inverse Problems - PPT Presentation

with a focus on seismic tomography CIDER2012 KITP Santa Barbara Seismic travel time tomography 1 In the background reference model Travel time T along a ray g v 0 s velocity at point s on ID: 1025092

travel model ray time model travel time ray inverse solution minimize theory velocity data problem gtg matrix size blocks

Share:

Link:

Embed:

Download Presentation from below link

Download Presentation The PPT/PDF document "Geophysical Inverse Problems" is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.


Presentation Transcript

1. Geophysical Inverse Problemswith a focus on seismic tomographyCIDER2012- KITP- Santa Barbara

2. Seismic travel time tomography

3. 1) In the background, “reference” model: Travel time T along a ray g:v0(s) velocity at point s onthe rayu= 1/v is the “slowness”Principles of travel time tomographyThe ray path g is determined by the velocity structure using Snell’s law. Ray theory.2) Suppose the slowness u is perturbed by an amount du small enoughthat the ray path g is not changed. The travel time is changed by:

4. lij is the distance travelled by ray i in block jv0j is the reference velocity (“starting model”) in block jSolving the problem: “Given a set of travel time perturbations dTi on an ensemble of rays {i=1…N}, determine the perturbations (dv/v0)j in a 3Dmodel parametrized in blocks (j=1…M}” is solving an inverse problem ofthe form:d= data vector= travel time pertubations dTm= model vector = perturbations in velocity

5. G has dimensions M x NUsually N (number of rays) > M (number of blocks):“over determined system”We write:GTG is a square matrix of dimensions MxMIf it is invertible, we can write the solution as:where (GTG)-1 is the inverse of GTGIn the sense that (GTG)-1(GTG) = I, I= identity matrix “least squares solution” – equivalent to minimizing ||d-Gm||2

6. G contains assumptions/choices:Theory of wave propagation (ray theory)Parametrization (i.e. blocks of some size)In practice, things are more complicated because GTG, in general, is singular:“””least squares solution”Minimizes ||d-Gm||2Some Gij are null ( lij=0)-> infinite elements in the inverse matrix

7. How to choose a solution?Special solution that maximizes or minimizes some desireable property through a normFor example:Model with the smallest size (norm): mTm=||m||2=(m12+m22+m32+…mM2)1/2Closest possible solution to a preconceived model <m>: minimize ||m-<m>||2 regularization

8. Minimize some combination of the misfit and the solution size:Then the solution is the “damped least squares solution”:e=d-GmTikhonov regularization

9. We can choose to minimize the model size, eg ||m||2 =[m]T[m] - “norm damping”Generalize to other norms.Example: minimize roughness, i.e. difference between adjacent model parameters.Consider ||Dm||2 instead of ||m||2 and minimize:More generally, minimize:<m> reference model

10. Weighted damped least squaresMore generally, the solution has the form:For more rigorous and complete treatment (incl. non-linear):See Tarantola (1985) Inverse problem theoryTarantola and Valette (1982)

11. Concept of ‘Generalized Inverse’Generalized inverse (G-g) is the matrix in the linear inverse problem that multiplies the data to provide an estimate of the model parameters;For Least SquaresFor Damped Least SquaresNote : Generally G-g ≠G-1

12. As you increase the damping parameter e, more priority is given to model-norm part of functional.Increases Prediction ErrorDecreases model structure Model will be biased toward smooth solutionHow to choose e so that model is not overly biased?Leads to idea of trade-off analysis.η“L curve”

13. Model Resolution MatrixHow accurately is the value of an inversion parameter recovered?How small of an object can be imaged ?Model resolution matrix R:R can be thought of as a spatial filter that is applied to the true model to produce the estimated values.Often just main diagonal analyzed to determine how spatial resolution changes with position in the image.Off-diagonal elements provide the ‘filter functions’ for every parameter.

14. Masters, CIDER 2010

15. 80%Checkerboard testR contains theoretical assumptionson wave propagation, parametrizationAnd assumes the problem is linearAfter Masters, CIDER 2010

16. Ingredients of an inversionImportance of sampling/coveragemixture of data typesParametrizationPhysical (Vs, Vp, ρ, anisotropy, attenuation)Geometry (local versus global functions, size of blocks)Theory of wave propagation e.g. for travel times: banana-donut kernels/ray theory

17. PSSurface wavesSS50 mnP, PPS, SSArrivals well separated on the seismogram, suitable for traveltime measurementsGenerally:Ray theoryIterative back projection techniques- Parametrization in blocks

18. Van der Hilst et al., 1998Slabs……...and plumesMontelli et al., 2004P velocity tomography

19.

20. Vasco and Johnson,1998P TravelTimeTomography:RayDensitymaps

21. Karason andvan der Hilst,2000Checkerboard tests

22. Honshu410660±1.5 %151305060708091112141513northern Bonin±1.5 %4106601000Fukao andObayashi2011

23. ±1.5%TongaKermadec06070809101112131415±1.5%4106601000Fukao andObayashi2011

24. PRI-S05Montelli et al., 2005EPRSouth Pacific superswellTongaFukao andObayashi,20116601000400S40RTSRitsema et al., 2011

25. Rayleigh waveovertonesBy including overtones, we can see into the transition zone and the top of the lower mantle. after Ritsema et al, 2004

26. Models from different data subsets120 km600 km1600 km2800 kmAfter Ritsema et al., 2004

27. SdiffScS2The travel time dataset in this model includes:Multiple ScS: ScSn

28. Coverage of S and PAfter Masters, CIDER 2010

29. PSSurface wavesSS

30. Full Waveform Tomography Long period (30s-400s) 3- component seismic waveforms Subdivided into wavepackets and compared in time domain to synthetics. u(x,t) = G(m)  du = A dm A= ∂u/∂m contains Fréchet derivatives of GUC B e r k e l e y

31. PAVANACTSSSdiffLi and Romanowicz , 1995

32. PAVANACT

33. 2800 km depthfrom Kustowski, 2006Waveforms only, T>32 s!20,000 wavepacketsNACT

34. To et al, 2005

35. Indian Ocean Paths - SdiffractedCorner frequencies: 2sec, 5sec, 18 secTo et al, 2005

36. To et al., EPSL, 2005

37. Full Waveform Tomography using SEM:UC B e r k e l e y Replace mode synthetics by numerical syntheticscomputed using the Spectral Element Method (SEM)DataSynthetics

38. SEMum (Lekic and Romanowicz, 2011)S20RTS (Ritsema et al. 2004)70 km125 km180 km250 km-12%+8%-7%+9%-6%+8%-5%+5%-7%+6%-6%+8%-4%+6%-3.5%+3%

39. French et al, 2012, in prep.

40.

41. Courtesy of Scott French

42. SEMum2S40RTSRitsema et al., 2011French et al., 2012EPRSouth Pacific superswellTongaSamoaEaster IslandMacdonaldFukao andObayashi, 2011

43. Summary: what’s important in global mantle tomographySampling: improved by inclusion of different types of data: surface waves, overtones, body waves, diffracted waves…Theory: to constrain better amplitudes of lateral variations as well as smaller scale features (especially in low velocity regions) Physical parametrization: effects of anisotropy!!Geographical parametrization: local/global basis functionsError estimation