Download presentation
1
Migrating elastic data
Aaron Stanton
2
Outline The seismic imaging problem Why not direct inversion?
Migrating scalar wavefields Downward continuation Imaging condition Migrating vector wavefields Wavefield decomposition Wavefield recomposition
3
The forward problem
4
The forward problem
5
The forward problem
6
The forward problem
7
The forward problem
8
The forward problem model data
9
model data ? The inverse problem
Non-linear, underdetermined (grid sizes are very tiny), and data sets are massive (tera bytes and even peta-bytes).
10
Linearize!
11
Model
12
Model perturbation
13
Born Scattering
14
Born Scattering
15
Born Scattering
16
Migration
17
Migration image = up/down
18
Downward continuation
19
Now for vector wavefields!
20
Vector data
21
Vector data
22
Vector data If we assume isotropy we can use Helmholtz decomposition
23
Helmholtz decomposition
24
Helmholtz decomposition
Etgen, 1988
25
Helmholtz recomposition
Etgen, 1988
26
Synthetic data example
Marmousi 2
27
vp
28
vs
29
Shot gathers
30
LS Migration: mpp 25˚ incidence angle
31
Migration: mps 25˚ incidence angle
32
Synthetic data example
Anticline model
33
Simulated OBC Acquisition
★ osx = 100m ; dsx = 100m ; nsx = 69 ; sz = 10m ; dgx = 8m ; gz = 550m ; recording aperture = 6608m
34
X-Component
35
Z-Component
36
Mpp Constant Incidence angle of 10˚
37
Mpp x = 1600m
38
Mps Constant Incidence angle of 10˚
39
Mps x = 1600m
40
Conclusions Migration of scalar wavefields consists of
downward continuation imaging condition Migration of vector wavefields consists of wavefield separation wavefield recombination
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.