Here I analyze one of the two amplitude effects observed in the data:
increasing amplitudes with increasing offset. Figure
shows
a reflectivity gather and the corresponding BSR AVO
trend picked along the BSR reflection. The reflectivity
gather displays a fairly well-resolved BSR wavelet.
The AVO trend
shows clearly the increasingly negative amplitudes with increasing angle.
The offsets were converted into angles by using the reflection angles at the
BSR, which were computed by the prestack migration (see Chapter 2).
For incidence angles between
and
,
the amplitudes are anomalously
low as a result of uncorrected amplitude effects as described
in Chapter2, section 2.4.3 (i.e. hydrophone array attenuation at central
offsets). Therefore, these two points are given small weights in the
following AVO modeling procedure.
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The initial P- and S-wave velocity used in the modeling are shown in Figure
. The P-wave velocity above and below the BSR is calculated
directly by averaging the interval velocity obtained from velocity analysis.
The S-wave velocity is determined by assuming a Poisson's ratio of 0.45,
which is consistent with the brine-saturated, highly unconsolidated
sediments typical of this region.
In the first attempt to model the observed AVO amplitudes, these initial
velocities are used as input velocities. The resulting AVO curve is
obtained using the Zoeppritz equations and is compared with the one observed
in the data (Figure
). The comparison of both curves shows that
with nearly constant amplitudes with increasing angles,
the initial velocity model fails not only to reproduce the
zero-offset reflection coefficient, but also to
reproduce the general AVO trend. Assuming negligibly
small density contributions, the near-offset amplitudes are mainly dependent
on the P-wave velocity contrast at the reflector, while the AVO trend is
characterized primarily by the S-wave velocity contrast. Thus, the AVO
response resulting from the initial velocity model implies the use of both
incorrect P- and S-wave velocities at the BSR.
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Based on this result, the subsequent modeling attempts to increase the
P-wave velocity contrast across the BSR in order to recreate the observed
zero-offset reflection amplitudes. The required increase is obtained
by increasing the velocity in the hydrate layer and simultaneously decreasing
the velocity in the layer underneath (Figure
.
This yields a thinner hydrate layer
over brine sediment. The S-wave velocity is again determined using a
Poisson's ratio of 0.45.
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The resulting AVO trend is shown in Figure
.
The comparison of the modeled AVO response with the observed response
indicates that
this model can successfully reproduce the zero-offset data. This suggests
a P-wave velocity of 2.05 km/s in the hydrate and 1.58 km/s in the underlying
sediments might resemble the actual conditions at the BSR. However, the
calculated AVO trend is still contrary to the observed one, displaying
nearly constant amplitudes with increasing angles. Hence, a change in Poisson's
ratio seems to be required at the transition from hydrate-bearing sediments
to the sediments underneath.
The observed AVO trend of the data suggests that the hydrate-bearing sediment
has a higher Poisson's ratio than the sediment underneath (see Figure
). Since it does not make sense physically to increase
the hydrate Poisson's ratio above 0.45 (fluids have Poisson's ratios of
about 0.5), I decrease the Poisson's ratio in the layer underneath to
simulate the drop in Poisson's ratio. This yields the same P-wave velocities
as described before, but an increase in S-wave velocity of about 0.25 km/s
across the BSR (Figure
).
The resulting velocities represent a Poisson's ratio of 0.45 in the hydrate
and approximately 0.28 in the sediments underneath. Instead of keeping
the hydrate Poisson's ratio constant, I could have increased the S-wave
velocity there as well. This would have yielded a lower Poisson's ratio
in the hydrate and would have required an even lower Poisson's ratio than 0.28
in the sediments underneath. Nonetheless, both cases would require
a strong increase in S-wave velocity across the BSR.
Since the drilling at the Blake Outer Ridge Matsumoto et al. (1996) has
shown that the overall shear structure in the sediments is very weak,
increasing the model S-wave velocities too much would generate
conditions that do not resemble in-situ conditions.
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The significant drop in P-wave velocity at the BSR as well as the decrease of Poisson's ratio suggests the presence of free gas underneath the hydrate layer. Domenico showed that the presence of gas can cause a decrease in Poisson's ratio down to 0.1 Domenico (1976). However, because the sediments at the Blake Outer Ridge are highly unconsolidated and have shale contents of more than 50% Matsumoto et al. (1996), I would not expect the Poisson's ratio to drop as low as 0.1 in the presence of free gas.
A comparison of the synthetic AVO curve obtained from the model in Figure
with the AVO trend observed in the data is shown in
Figure
. The synthetic curve agrees well with the real data
for both near and far offsets. Thus, a strong increase in S-wave
velocity and a simultaneous decrease in P-wave velocity at the transition from
hydrate-bearing sediments to sediments containing free gas is required to
explain the seismic data. The inferred velocity contrasts are, furthermore,
in good agreement with the prediction based on the negative P-impedance
contrast and positive S-impedance contrast obtained from the impedance
inversion.