Here I analyze the second amplitude effect observed along the BSR: nearly
constant amplitudes with increasing angle. A representative reflectivity
gather and the picked BSR amplitude trend are shown in Figure
. Since some residual amplitudes are left at the
central offsets between
and
(Chapter 2, section 2.4.3),
those amplitudes are edited manually to be
in better agreement with the general amplitude trend.
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As described before, I determine the initial velocity models by averaging
the interval velocity determined in Chapter 2 and assuming a Poisson's
ratio of 0.45, representative of brine-saturated sediments. This initial
velocity model is shown in Figure
.
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The synthetic AVO curve corresponding to this velocity model is again
calculated using the Zoeppritz equations. It is compared with the AVO trend
observed in the data in Figure
. The comparison shows that
this first velocity model fails to reproduce the zero-offset reflection
coefficient, while the general AVO trend appears to be in fairly good
agreement. This already suggests that this AVO trend might not represent
a hydrate-over-gas model.
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In order to fit the data, the P-wave velocity across the BSR must be
increased and the S-wave velocity contrast slightly decreased
(Figure
). The result is similar
to the P-wave velocity contrast described in the previous
section: the hydrate velocity increases to approximately 2.07 km/s while the
velocity in the underlying sediment decreases to about 1.55 km/s.
The slight decrease in S-wave velocity contrast results in a slightly smaller
Poisson's ratio of about 0.43 in the sediments below the hydrate, compared
to a value of 0.45 in the hydrated sediment itself.
This small decrease in Poisson's ratio is consistent with
a hydrate-over-brine model, and may be explained by the heterogeneity of the
sediments, which can cause not only variations in P-wave velocity but also
in Poisson's ratio.
The resulting AVO curve is shown in Figure
. The comparison
of the modeled AVO curve with the one observed indicates that this model
successfully reproduces the zero-offset reflection coefficient and the
AVO trend. This good agreement suggests that there exists
a small decrease in S-wave velocity across the BSR.
This indicates that the
model of hydrate over brine-saturated sediment would be required to
reproduce the nearly constant amplitudes with increasing offset.
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The analysis of the nearly constant amplitude trend with increasing angle indicates that the BSR amplitudes require a significant negative P-wave velocity contrast and a small negative S-wave velocity contrast. Based on the fairly unchanged Poisson's ratio at the transition, this would suggest a hydrate-over-brine sediment model for these amplitude variations. However, the significant decrease in the velocities underneath the hydrate, consistent with drilling results and similar seismic analyzes in the region, strongly suggests the presence of free gas Holbrook et al. (1996); Katzman et al. (1994); Lee et al. (1994); Matsumoto et al. (1996); Wood et al. (1994). Consequently, two interpretations are possible:
A heterogeneous distribution of gas and brine saturation is physically plausible in marine sediment. The gas can be trapped in thin layers that serve as permeability barriers, yielding a patchy gas distribution Dillon et al. (1993). However, the resolution of localized patches of brine and gas saturation from surface seismic is highly questionable. Therefore, it is more reasonable to assume that the constant amplitudes result from thin layer tuning effects, rather than patchy brine saturation beneath the BSR.