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Velocity model building with long-offset and full-azimuth data: a case history for full-
waveform inversion Wei Huang*, Hongda Ma, Denes Vigh, Jerry Kapoor, Kun Jiao, Xin Cheng, Dong Sun, WesternGeco
Summary
In the last few years, there has been an increased focus on
designing advanced acquisition methods for better subsalt
imaging. These acquisition methods usually offer large-
offset, full-azimuth datasets with higher signal-to-noise
ratio and rich content of low frequency data. To fully
exploit the capability of these large-offset data sets, full-
waveform inversion is often adopted as the tool to build a
high-fidelity, high-resolution velocity model. In this paper,
we describe our general steps and QC measurements in
full-waveform inversion model building for a field data set.
Comparison of reverse time migration (RTM) images
between the initial tomography velocity and full-waveform
inversion velocity validate the uplift provided by full-
waveform inversion.
Introduction
Wide-azimuth (WAZ) towed-streamer acquisition has
proven to be a successful technique for subsalt imaging in
the Gulf of Mexico. Numerous survey and imaging projects
have been undertaken to achieve quality subsalt images.
However, the rapid development in imaging and modeling
algorithms demand a more advanced acquisition technique
that offers even better signal-to-noise ratio, illumination,
and azimuth information. One of the viable approaches that
offers an even distribution of azimuth information is the
circular shooting geometry. The concept of circular
geometry for towed-streamer marine acquisition was
introduced in the early 1980s by French (1984), where the
full-azimuth data set can be acquired by a single vessel
sailing along overlapped circles. Successive efforts and
developments in acquisition design further this idea by
implementing multi vessel long-offset circular shooting
geometry (Moldoveanu and Kapoor, 2009). Multi-vessel
long-offset circular shooting involves two recording vessels,
each with their own sources, and two additional source
vessels, all sailing in large (12- to 15-km diameter)
interlinked circles, which is schematically shown in figure
1. The trace density of this type of survey is greater than
that of typical WAZ designs, resulting in a higher fold and
improved signal-to-noise ratio for subsalt imaging (Huang
et al., 2013).
However, big-volume, large-offset and full- azimuth data
sets bring new challenges for velocity model building and
imaging. The first challenge comes from how we can fully
exploit the extra information from the far-offset data; the
second challenge stems from the substantial computational
cost demanded by the large-volume datasets. Reflection
tomography is a global optimization method that minimizes
the residual depths from common-imaged-gathers (CIG);
however, in the Gulf of Mexico (GoM) geological setting,
reflection tomography has its limitations when there exists
large velocity contrast, e.g., the presence of a salt body.
Tomography using diving waves can be an alternative for
velocity model building with long-offset data.
One of the other advanced techniques that can offer the
ability to resolve the velocity field and fully exploit the rich
information offered by far-offset data is full-waveform
inversion (FWI). Although first introduced in the 1980s
(Tarantola, 1984), only recently has FWI been successfully
applied to WAZ data sets (Vigh et al., 2009). It is
recognized that, to lessen the sensitivity of the initial
velocity, FWI must start with low frequencies and long
offsets. (Bunks et al., 1995; Pratt and Shipp, 1999).
One of the other reasons preventing the application of FWI
to large-volume data sets is the high computational cost
associated with FWI. FWI is a data-fitting technique based
on finite–difference forward modeling, which requires a
Figure 1: Schematic plot of lay out of multi-vessel long-offset
circular shooting acquisition Figure 2: Survey location in GOM and total about 400000 of
shots were recorded in this area
© 2013 SEGSEG Houston 2013 Annual Meeting Page 4750
Model building with long-offset and full-azimuth data
number of iterations to obtain an optimal velocity field.
Recent synthetic studies suggest using statistical sampling
to achieve a solution with less cost (van Leeuwen and
Hermann, 2012). Application of this statistical sampling is
of great interest for 3D very large data sets.
Application of FWI to real-world data sets is quite different
from synthetic tests, where a ground-truth velocity model is
readily given. There are many challenges for velocity
model building with FWI, e.g., higher noise level,
uncertainness of the initial model, and others. The model
building process is far from being as standardized as that of
current layer-stripped ray-based tomography updates. In
this study, we first give a general description of the field
data set used for this study. We then outline our general
velocity model building steps for FWI and discuss the
benefit we can get from FWI model building.
Field Data Description
The multi vessel long-offset circular shooting data set used
in this study is located primarily in the Keathley Canyon
area of the GoM, and part of the survey area lies in the
Sigsbee Escarpment. The geology is characterized by
extensive salt sheets with intervening deep-water sediment-
filled mini-basins. The salt canopy is characterized by
simple-to-complex salt features, some of which have a
thickness of up to 30,000 ft and some are extremely
shallow, i.e., just under the water bottom. There are several
major discoveries in this area, including the Lucius,
Moccasin, and Hadrian prospects. The overall goal of this
study is to employ FWI and the large-offset data to enhance
the subsalt image.
The fully imaged area shown in figure 2 is approximately
2901 km2 (124 OCS blocks). The record length for each
shot is 16.8 s and the maximum offset was around 15,000
m. A total of more than 400,000 shot gathers were recorded,
which were further super-grouped into around 100,000
shots for computational efficiency. Standard pre-migration
processing was performed before the FWI, e.g., de-noise
and de-multiple.
.
Full waveform inversion flow and results
The full waveform inversion used for this study is
implemented in time domain using acoustic wave equation.
A conjugate gradient method was adopted for updating the
velocity field by iteratively reducing the global misfit:
2
mod2
1∑∑ −=
S R
obs ddE (1)
where E is the global misfit, obsd and modd are the
observed and modeled shots respectively.
The inversion utilized anisotropic propagators using tilted
transverse isotropy, and the inversion updates only velocity.
ε and δ are derived from well information and
extrapolated to the target area. θ and φ are derived from a
vintage vertical transverse isotropic RTM image. The
starting velocity was a less-detailed ray-based tomography
velocity. The subsalt velocity was built by superposing a
regional velocity gradient below the salt.
Equipped with the initial velocity model and preprocessed
datasets, the first step for field data FWI model building is
wavelet estimation. Wavelet estimation is the key step to
achieve a successful FWI update, especially for field data.
Correct setting of the acquisition parameters is also critical
to the success of a FWI velocity update, e.g., source-
detector depth, dead trace information, and others. Unlike
the synthetic case where the source wavelet is always
readily given, the source wavelet for field data is generally
contaminated by factors such as noise, ghost, and
Figure 3: Wavelet estimation for target frequency (2.5Hz) : A)
Inverted wavelet . B) Overlay of modeled and observed shots
Figure 4: Global misfit reduction over FWI iterations
© 2013 SEGSEG Houston 2013 Annual Meeting Page 4751
Model building with long-offset and full-azimuth data
uncertainties in the velocity model. To incorporate these
effects, we adopt an approach based on the variable
projection method to estimate the source wavelet during
inversion. Validation of the source wavelet is done by
comparing the modeled and real data water bottom and
direct arrival in time and phase. Figure 3 gives the inverted
source wavelet and sample shots from modeling and
observed, where phase information of the water bottom and
direct arrival is correctly modeled.
After achieving a valid starting source wavelet, together
with the initial velocity, FWI at 2.5 Hz were performed for
this pilot study. To lessen the contamination from the
residual multiples, we limited the data used for the FWI
update to be above the first multiple. To make the inversion
more efficient, statistical sampling was adopted for this
FWI implementation, whereas different subsets of the shots
were used for consecutive FWI update.
In the absence of well control, we do not have an
independent direct measurement of the FWI update. Global
misfit drop is a natural measurement of a FWI update
because the kinematics of FWI are to reducing the global
misfit. The global misfit drop is demonstrated in figure 4.
After FWI update , around 20% of the global misfit drop
was observed for this study. However, the global misfit
drop may not be sufficient to validate the updated velocity
by FWI. QC measurements were performed to validate our
FWI update. The similarity between the forward-modeled
shots and the observed shots was first investigated.
The forward-modeled shot gather using the FWI-updated
velocity model and the initial modeled shot gather at 2.5 Hz
are shown in figure 5. The top row of figure 5 presents the
modeling comparison from the near cable and the bottom
row shows the far cable. The near cable contains data
information from about 200 m to 8 km, while the far cable
shots contain up to 15 km. Both the near-cable and far-
cable shot gathers from the FWI model show a higher
resemblance in phase and time to the observed shots than to
that of the initial model. To quantify the resemblance
between the observed data and modeled data, we apply
zero-lag cross correlation between the modeled and
observed shots. The correlation between observed and
modeled was done in five different time windows for these
gathers. Figures 6(A) and 6(B) show an example of the
correlations for the initial model and the FWI-updated
models, respectively. A histogram of the correlations over
shot-gather domain is also presented in figure 6(C). It is
observed that the peak of the correlation move from 0.45 to
around 0.62 after FWI update, suggesting a higher
resemblance globally.
Ray-based CIG are another important QC measurement of
the quality of the updated velocity model. The Kirchoff
gathers were observed to be flat over the whole area. An
example of the gather change around the Hadrian area after
the FWI update is given in figure 7 (A) and 7(B),
After these QC measurements, a reverse time migration at
18 Hz was run to see the impact of the velocity change by
the FWI update. Figure 7 presents the velocity and
corresponding RTM image for the target line around the
Hadrian prospect. The updated velocity field shows more
details, especially in the shallow part. The updated velocity
Figure 6: Coreelaions at (2.5Hz) : A) correlation for initial modeling B) correlation for FWI modeling C) global correlation histogram
Figure 5: Shot gathers filtered at 2.5 Hz (A) recorded near cable (B)
initial modeling of near cable (C) FWI modeling of near cable (D)
recorded far cable (E) initial modeling of far cable (F) FWI
modeling of far cable
© 2013 SEGSEG Houston 2013 Annual Meeting Page 4752
Model building with long-offset and full-azimuth data
follows the general trend of the geology. A narrow low-
velocity zone was observed in the depth of 10000, which
could potentially be beneficial for high resolution pore-
pressure prediction. In the RTM image comparison, we
observe a significant improvement in the continuity and
focusing of the subsalt structure, thereby justifying the FWI
result.
Conclusions
In this paper, we outlined the general step and QC
measurements for a pilot project using a far-offset and full-
azimuth dataset. Starting with reflection tomography
velocity and wavelet matching, we run iterations of FWI
update. In order to reduce the humongous computational
cost required by the large volume 3-D dataset, a statistical
sampling scheme was used in this study. Various QC
measurements were performed to qualify our velocity
update using FWI. Reverse time migration was performed
and it was concluded that even though the velocity updates
are limited to shallow area, the subsalt events can become
more coherent.
Figure 7: Comparison between initial and FWI updated: A) gather from initial model; B) gather from FWI updated model; C) velocity
from initial model; D) velocity from FWI updated model; E) RTM image from initial model; F) RTM image from FWI updated model.
© 2013 SEGSEG Houston 2013 Annual Meeting Page 4753
EDITED REFERENCES Note: This reference list is a copy-edited version of the reference list submitted by the author. Reference lists for the 2013 SEG Technical Program Expanded Abstracts have been copy edited so that references provided with the online metadata for each paper will achieve a high degree of linking to cited sources that appear on the Web.
REFERENCES
Bunks, C., F. M. Saleck, S. Zaleski, and G. Chavent, 1995, Multicscale seismic waveform inversion: Geophysics, 60, no. 5, 1457–1473, http://dx.doi.org/10.1190/1.1443880.
French, W. S., 1984, Circular seismic acquisition system: United States Patent 4,486,863.
Huang, W., K. Jiao, D. Vigh, J. Kapoor, H. Ma, and K. D. Dingwall, 2013, Salt exit velocity retrieval using full-waveform inversion: 75th Conference and Exhibition, EAGE, Extended Abstracts.
Moldoveanu, N., and J. D. Kapoor, 2009, What is the next step after WAZ for exploration in the Gulf of Mexico: 79th Annual International Meeting, SEG, Expanded Abstracts, 41-45.
Pratt, R. G., and R. M. Shipp, 1999, Seismic waveform inversion in the frequency domain, Part2: Fault delineation in sediments using crosshole data: Geophysics, 64, no. 3, 902–914, http://dx.doi.org/10.1190/1.1444598.
Tarantola , A., 1984, Inversion of seismic reflection data in the acoustic approximation: Geophysics, 49, no. 8, 1259–1266, http://dx.doi.org/10.1190/1.1441754.
van Leeuwen, T. and F. J. Hermann, 2012, Fast waveform inversion without source encoding: Geophysical Prospecting, 61, no. s1, 10–19, http://dx.doi.org/ 10.1111/j.1365-2478.2012.01096.x.
Vigh, D., W. E. S. Starr, and K. D. Dingwall, 2009, 3D prestack time domain full waveform inversion: 71st Conference and Exhibition, EAGE, Extended Abstracts.
© 2013 SEGSEG Houston 2013 Annual Meeting Page 4754