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Rock Physics
In the Rock Physics Laboratory,
our aim is to investigate the mechanical, physical and transport
properties of crustal rocks. We perform deformation experiments
on rocks under conditions that simulate the pressure, temperature,
deviatoric stress, and pore pressure environment of the upper
(seismogenic) crust. Importantly, we also measure changes
in a range of key properties (porosity, permeability, wave
velocities, microseismic emissions and electrical conductivity
and potential) simultaneously with deformation.
These are the properties that are routinely
measured on the reservoir or crustal scale. Thus, we are able
directly to link the changes in physical and transport properties
to the state of stress and deformation in the rock under carefully
controlled conditions. This cannot be done at the reservoir
or crustal scale. Thus, we are able to provide insights into
improved interpretation of reservoir and crustal scale geophysical
data.
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| Some Current Research Projects: |
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CREEP:
Long-term time-dependent rock deformation in the laboratory
and in a deep-sea observatory
Water-saturated rocks are ubiquitous in Earth’s
upper crust and the chemistry of water-rock interactions leads
to time-dependent deformation through the mechanism of stress
corrosion that allows rocks to fail over extended periods
of time at stresses far below their short-term strength. Recent
theoretical models, based on mean-field damage mechanics,
suggest that the growth and interaction of cracks leads to
acceleration to failure once some critical damage threshold
has been reached. Recent experimental observations in the
Rock Physics laboratory at UCL (Baud & Meredith, 1997).support
this approach.
We are therefore investigating this process
by conducting constant stress, brittle creep experiments in
our triaxial deformation apparatus. Because the process is
highly non-linear, it is necessary to run experiments lasting
from a few tens on minutes to a few tens of days in the laboratory.
In order to extend the range of observation
even further, we would need to conduct experiments with durations
of months or even years. Clearly, such experiments are not
practicable in a normal laboratory. We have therefore constructed
an apparatus to allow us to conduct ultra-long-term experiments
at 2km depth in a deep-sea observatory in the Ionian Sea off
Sicily. The main reason for considering the deep-sea environment
is its stability; constant pressure and temperature throughout
the year. The constant pressure at depth provides both the
confining pressure and the constant creep stress (via a pressure
intensifier).
To date, we have run experiments up to 6
months duration and achieved strain rates in the range 10-11
s-1; some two orders of magnitude lower than our slowest laboratory
experiments. Importantly, these rates encompass the time-scales
typical of the periods of precursory activity that precede
major crustal failure events, and they bridge the gap between
laboratory strain rates and those typical of the crust.
CREEP Data |
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| Influence of pore space anisotropy on
the development of compaction bands Compaction
bands are newly recognized but ubiquitous feature of the deformation
of high porosity sedimentary rocks. They are generally manifested
as densely packed, poorly sorted, low porosity bands in otherwise
well sorted, high porosity rocks. They are important because
they occur as low permeability bands in generally high permeability
rocks, and thus act to compartmentalize reservoirs and aquifers.
Anisotropy of pore space is also a ubiquitous
feature of sedimentary rocks, which leads to an anisotropy
of the physical, transport and mechanical properties. We are
therefore studying compaction band development in Diemelstadt
sandstone; a bedded, anisotropic sandstone with an initial
porosity of abut 23% and a mean grain size of about 0.3 mm
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We have quantified the pore-space anisotropy
of Diemelstadt sandstone by measuring radial elastic S and
P wave velocities as a function of azimuth around cores samples
taken in three orthogonal directions. Fluid permeability has
also been measured along these three principal directions
and the technique of pAMS (Benson et al., 2003) has been used
to quantify the anisotropic pore space geometry. We find a
velocity anisotropy of around 10% for P-waves and 5% for S-waves,
lower permeability normal to bedding, and a mean pore space
geometry approximating to an oblate spheroid.
With the pore-space anisotropy established,
we characterised its influence on mode of failure by performing
triaxial deformation experiments on samples cored normal and
parallel to bedding. Both orientations demonstrated a transition
from brittle faulting at low effective pressure to the growth
of discrete compaction bands at higher effective pressure.
We found that the compactive yield envelope for the bedding-normal
samples expanded more towards higher stress values than the
envelope for bedding-parallel samples.
We find that compaction bands formed both
normal and parallel to bedding act as barriers to flow and
reduce bulk permeability, consistent with previous work (Vajdova
et al., 2004). Microstructural comparisons of the discrete
compaction bands formed parallel vs normal to bedding show
that those formed normal are more tortuous and less extensive
than those formed parallel.
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| Modelling the permeability evolution of
micro-cracked rocks from elastic wave velocity inversion at
elevated isostatic pressure. A
key consequence of the presence of microcracks within rock
is their significant influence upon elastic anisotropy and
transport properties. In this study, two microcracked rock
types (a basalt and a granite) with known but contrasting
microstructures have been investigated using an advanced experimental
setup to measure sample porosity, P-wave velocity, S-wave
velocity and permeability contemporaneously for effective
pressures up to 100 MPa (Rock
Fluids Laboratory).
Using the Kachanov (1994) non-interactive
effective medium theory, the laboratory measured elastic wave
velocities are inverted using a least square fit, allowing
us to evaluate the evolution of crack density and crack aspect
ratio with increasing isostatic pressure. Overall, the agreement
between measured and predicted velocities is good, with average
error less than 0.05 km/s. At larger scales above the percolation
threshold, macroscopic fluid flow also depends on the crack
density and aspect ratio. Using the permeability model of
Guéguen & Dienes (1989) and the crack density and
aspect ratio recovered from the elastic wave velocity inversion,
we successfully predict the evolution of permeability with
pressure for direct comparison to the laboratory permeability
results. In addition, we calculate the influence of the crack
porosity element, also based upon crack density and evolution,
for direct comparison to the experimentally measured porosity
change with isostatic pressure. These combined modelling/experimental
results illustrate the importance of understanding the details
of how the rock microstructure can change in response to an
external stimulus in order to predict the common evolutions
of rock physical properties.
Click Here For Experimental Data
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Designed & Maintained by
N. Hughes
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