EBOOK-LUSI
Lupi 2014a
Lusi mud eruption triggered by
geometric focusing of seismic waves
M.
Lupi, E. H. Saenger, F. Fuchs and S. A. Miller
Nature
Geoscience 6, 642–646 (2013); published online 21 July 2013; corrected after
print 28 August 2014.
In
our 2013 article1 numerical
simulations. We were subsequently alerted to artefacts in that velocity
profile, so below we present revised simulation results, based on additional
data.
The
seismic P-wave (Vp) and S-wave (Vs) velocity profiles measured in the BJP1
borehole (Supplementary Fig. 1) show that the Vp profile extends from a depth
of about 300 m to the bottom of the section.
The
S-wave and density profiles, however, were only determined from the depth of the casing (approximately
1,100 m) to the bottom of the section.
As
we mentioned previously1 more vigorously to S-wave energy, but the critical
information about the S-wave mechanical impedance (Vs multiplied by density, ρ)
does not exist for the first 1,100 m of this section.
Instead,
we estimate an S-impedance profile above the mud layer by using the observed Vp
profile and the observation that Vs in the mud layer is as low as 380 m s–1 at
1,100 m depth.
This
extremely low value reinforces what has
been pointed out elsewhere2,3, that the mud layer is a low-velocity zone
representative of an over-pressured and under-consolidated sedimentary horizon.
Such
horizons are common throughout sedimentary basins in Southeast Asia.
We
estimate Vs above the mud layer using experimental data (Supplementary Fig. 2)
showing the relationship between Vs and Vp.
Although
the Vp profile above the mud layer seems not to vary significantly
(Supplementary Fig. 1a), a closer inspection (Supplementary Fig. 1b) shows that
the Vp steadily increases just above the mud layer from about 1,500 m s–1 to
about 2,000 m s–1, low effective stress4 between
about 700 and 875 m depth.
The
steady increase in Vp with depth, typical of a normal compacting horizon,
indicates lower fluid pressures relative
to the fluid pressure in the underlying mud layer.
We
assume that the top of the mud layer corresponds to the observed drop in Vp at around 900 m depth,
which is consistent with the well log data (Supplementary Fig. 3).
Using
the recorded Vp constraint of 2,000 m s–1 with a Vp/Vs ratio of about 2.7
(Supplementary Fig. 2), we estimate Vs at the top boundary of the mud layer
to be about 750 m s–1 .
We
assume that the 380 m s–1 Vs recorded at 1,100 m depth extends to the top of
the mud layer because of the relatively constant and reduced Vp below the
compacting layer (Supplementary Fig. 1b).
It
should be emphasized that there is considerable
uncertainty in Vs above the mud layer, but the observed reduction in Vp
with depth (after a systematic increase of velocity with depth in the layer above) corresponds to a far greater
reduction in Vs within the mud layer.
Therefore,
the interface between the mud layer and the compacting layer corresponds to an
impedance contrast.
This
is evident in the elevated Vp/Vs ratios of about 4.5 within the mud layer
(Supplementary Fig. 4), which again indicate low effective normal stress
(Supplementary Fig. 2).
At
low effective stress, Vp and Vs are only weakly coupled whereby Vp remains
relatively constant while Vs varies depending on the pore pressure.
The
effective stress depend-ence on Vp/Vs ratios occurs because Vs is solely
dependent on the shear modulus while Vp is dominated by the bulk modulus.
Since
shear modulus varies strongly as a function of pore pressure, small changes in
pore pressure at low effective stress generate large changes in Vs, with little
influence on Vp.
From
the available experimental data (Supplementary Fig. 2), we can expect about a
factor of two difference in Vp/Vs.
We
multiply our estimated Vs profile (Fig. 1a) with the measured density profile
(see Supplementary Fig. 3), using 1,800 kg m–3 where there is no data, to
generate a new impedance profile (Fig. 1b).
We
used this impedance profile as input for our numerical simulation, using the
same input and boundary conditions as described previously1have been removed.
The
results from our revised simulations (Fig. 1c) show that our estimated
impedance-contrast between the low-velocity mud layer and the compacting sediments above produces a
comparable focusing effect and maximum shear strain, as we reported previously1
Notably,
our two-dimensional simulations underestimate by a factor of five the
additional amplification when the third dimension of this parabolic structure is considered Our
conclusions1
References
1. Lupi,
M., Saenger, E. H., Fuchs, F. & Miller, S. A. Lusi mud eruption triggered
by geometric focusing of seismic waves. Nature Geosci. 6, 642–646 (2013).
2. Istadi,
B. P., Pramono, G. H., Sumintadireja, P. & Alam, S. Modeling study of
growth and potential geohazard for LUSI mud volcano: East Java, Indonesia. Mar. Petrol. Geol. 26, 1724–1739 (2009).
3. Tanikawa,
W., Sakaguchi, M., Wibowo, H. T., Shimamoto, T. & Tadai, O. Fluid transport
properties and estimation of overpressure at the LUSI mud volcano, East Java
Basin. Engin. Geol. 116, 73–85 (2010).
4. Lee,
M. W. Predicting S-Wave Velocities for Unconsolidated Sediments at Low
Effective Pressure (USGS Scientific Investigations report 2010–5138, 2010).
5. Davis,
P. Triggered mud eruption? Nature Geosci. 6, 592–593 (2013).
Acknowledgements
We
thank Maxwell Rudolph at Portland State University, USA, Mark Tingay at the
University of Adelaide, Australia, Michael Manga and Chi-Yuen Wang at the
University of California, Berkeley, USA, and Richard Davies at Durham
University, UK, for alerting us to the errors in the original seismic velocity
profile and for providing us with the additional data from the BJP1 borehole.
Figure
1 | Revised numerical simulations.
a,
We estimate a Vs (red line) profile based on the measured Vp (green line) and
Vs (blue line) profiles.
The
model domain was discretized into 21 layers (with higher resolution for the
first 2,000 m) approximated from the measured and estimated profiles (Supplementary Figs 1 and 2).
Experimental
data4 suggest that Vs varies indirectly with Vp. That is, Vp ∝
AVs, where A is a coefficient that varies depending on the shear modulus, pore pressure
and effective pressure (Supplementary Fig. 2).
Hence
Vs does not always correlate positively with Vp. The observation of Vp = 2,000 m s–1 directly
above the mud layer (Supplementary Fig. 1b) implies from Supplementary Fig. 2
that Vs = 750 m s–1, while further
observations of Vp = 1,600–1,750 m s–1 in the mud layer are also consistent
with the observation of Vs = 380 m s–1 and Vp /Vs = 4.5 in the mud layer (Supplementary Fig. 4).
Therefore,
we suggest there is little uncertainty in the magnitude of the impedance contrast,
and small changes in these values will
not significantly affect our results because they scale with impedance
contrast.
b,
We use the S-wave estimates (a) to construct an S-wave impedance profile (with
units kg m–2 s–1).
c,
We use the S-wave impedance profile (b) in our numerical simulation, using the
same input and boundary conditions as our original model simulation1 impedance
contrast at Lusi is sufficient to focus seismic energy into the mud layer.
The
dashed line marks the top of the mud layer. The results from this simulation
show that the inferred Additional
information.
Supplementary
information is available in the online version of the paper., we adopted a
published velocity profile2 described as check-shot data, which we used as an
input constraint for our in
Supplementary Fig. 2 are from a different lithology than that at Lusi, the
physics is lithology-independent,
therefore remain
unchanged. We appreciate this opportunity to correct the record.
Nature
Geosciences
SUPPLEMENTARY
INFORMATION
DOI:
10.1038/NGEO2239
Lusi mud eruption triggered by
geometric focusing of seismic waves
M. Lupi, E. H. Saenger, F.
Fuchs and S. A. Miller
Supplementary
Figure 1. Measured Vp and Vs profiles (a) from the BJP-1 borehole.
The
Vp record extends to about 300 m depth, while the Vs record does not begin
until the casing shoe at about 1100 m depth. Notice that Vs is about 380 m/s in
the mud layer.
A
zoom-in of a portion of the record (b) shows increasing Vp with depth above the
mud layer, between about 700 m and 875 m depth (blue line), indicative of a
normally compacting horizon.
A reduction in Vp at depths
from 875 m to 1150 m indicates
significantly reduced effective stress from the over-pressured and
under-consolidated mud layer.
Supplementary
Figure 2. Experimental data showing large reductions in Vp/Vs ratios with
increasing effective stress.
We
used the measured Vp of 2000 m/s at the top of the mud layer to estimate a Vs
of about 750 m/s at this boundary.
The
recorded S-wave velocity of 380 m/s in the mud layer (Vp/Vs=4.5, supplementary
fig 4) indicates low effective stress representative of an under-consolidated
and over-pressured horizon, typically referred to as low-velocity zones.
Modified from [Lee, 2010].
Supplementary
Figure 3. The complete montage of the well log recorded for the BJP1 borehole.
In
our original study, we interpreted the top of the mud layer to exist at about
1,100 m depth based on a published velocity profile.
However, well log data recorded at borehole BJP1 show
that the mud layer begins at ~900 m and we have adjusted our analyses and
interpretations accordingly.
Supplementary
Figure 4. Measured Vp/Vs ratios showing persistently elevated ratios of about 4.5 within the mud layer indicative of
a low effective stress (high pore pressure) environment.
References:
Lee,
M.W., (2006c), A simple method of predicting S-wave velocity: Geophysics, v.
71, p. F161–F164.
Lee , M. W. (2010), Predicting S-Wave
Velocities for Unconsolidated Sediments at Low Effective Pressure, USGS
Scientific Investigations report 2010-5138.
Walton, K., (1987), The effective elastic
moduli of a random packing of spheres: Journal of the Mechanics and Physics of
Solids, v. 35, p. 213–226.
Zimmer, M.A., (2003), Seismic velocities in unconsolidated sands―Measurements of
pressure, sorting, and compaction effects: Palo Alto, Calif., Stanford, Ph. D
thesis 204 p.
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