finite-elementmodellingofcontemporaryandpalaeo- · computers&geosciences31(2005)297–307...
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ARTICLE IN PRESS
0098-3004/$ - se
doi:10.1016/j.ca
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Computers & Geosciences 31 (2005) 297–307
www.elsevier.com/locate/cageo
Finite-element modelling of contemporary and palaeo-intraplate stress using ABAQUSTM$
S. Dyksterhuis�, R.A. Albert1, R.D. Muller
School of Geosciences and University of Sydney Institute of Marine Science, Edgeworth David Building (F05),
University of Sydney, NSW 2006 Australia
Received 27 August 2003; received in revised form 24 September 2004; accepted 6 October 2004
Abstract
Knowledge of the contemporaneous and palaeo-orientation of maximum horizontal compressive stress (SHmax) in the
Earth’s crust is important for the exploration and recovery of hydrocarbons and also provides insights into the
mechanisms driving plate motion and intra-plate seismicity. To date, most approaches for modelling intraplate stress
orientations have been based on applying forces to homogeneous elastic plates. However, real tectonic plates consist of
oceanic and continental lithosphere, including sedimentary basins, fold belts and cratons with large differences in elastic
properties. We have used the finite-element method as implemented in the software package ABAQUSTM along with
the optimisation software Nimrod/O to model the orientations and magnitudes of SHmax over the Indo-Australian plate
for the present and the Miocene. An elastic 2D plane stress model incorporating realistic mechanical properties for the
Australian continent was used consisting of 24,400 elements, providing a resolution of 0.21 in both latitude and
longitude. In general, modelled SHmax directions correlate well with observed contemporary stress indicator data and
reactivation histories over the NW Shelf and Bass Strait regions of the Australian continent, where Tertiary tectonic
reactivation through time is best documented. Large perturbations in SHmax orientation over the Australian continent
are shown to occur in and around regions of heterogeneous material properties.
r 2004 Elsevier Ltd. All rights reserved.
Keywords: Australia; Stress; Palaeo-stress; Modelling; Plate dynamics
1. Introduction
An understanding of the orientation of contempora-
neous maximum horizontal compressive stress (SHmax) is
e front matter r 2004 Elsevier Ltd. All rights reserve
geo.2004.10.011
server at http://www.iamg.org/CGEditor/
ing author.
esses: [email protected]
[email protected] (R.D. Muller).
ess: ExxonMobil Upstream Research Co., P.O.
ston, TX 77252-2189, USA.
relevant to many areas of earth science, providing
fundamental insights into the mechanisms driving plate
motion. Knowledge of contemporaneous and palaeo
SHmax orientations and magnitudes is also useful for
improved exploration and recovery of hydrocarbons,
allowing for the creation of a predictive framework for
fault reactivation and the planning of deviated drilling.
Since SHmax data can be sparse over large areas of
continents and over geologic time, geophysical model-
ling of SHmax regimes is necessary to provide a
satisfactory understanding of the regional stress field.
Data compiled as part of the World Stress Map project
(Zoback, 1992) provide important constraints on
d.
ARTICLE IN PRESSS. Dyksterhuis et al. / Computers & Geosciences 31 (2005) 297–307298
present orientation and magnitude of SHmax regimes of
continents, and in particular data contained in the
Australian Stress Map project (Hillis and Reynolds,
2000) are used here as constraint on modelled con-
temporary SHmax orientations for the Indo-Australian
plate.
Up to now most approaches for modelling Indo-
Australian intraplate stress orientations have been based
on applying forces to homogeneous elastic plates
(Coblentz et al., 1995, 1998; Hillis et al., 1999; Reynolds
et al., 2002). While these studies model the first-order
pattern of stress over the Australian continent well,
more recently Zhao and Muller (2003) studied the
second-order effects of homogeneous material proper-
ties on the stress field of Eastern Australia, determining
through inverse analysis that inclusion of realistic
material properties improves the regional fit between
modelled and measured SHmax orientations.
Modelling of the stress regime of the Indo-Australian
plate was carried out here using ABAQUSTM, an
engineering industry standard finite-element modelling
software package, in conjunction with the distributed
optimisation software Nimrod/O. A 2D plane-stress
elastic finite-element model was created consisting of
24,400 elements allowing for a spatial resolution of 0.21
of both latitude and longitude (Fig. 1). While the
assumption of elastic rheology, which precludes any true
time dependence, is an oversimplification it is justifiable
Fig. 1. Mesh of ABAQUSTM contemporary Indo-Australian plate mo
giving a resolution of roughly 0.21 in both latitude and longitude.
for the modelling of such large scale, low order tectonic
stresses. Forces applied to the models are averaged over
a lithosphere of 100 km thickness.
2. Modelling method
Finite-element modelling of the Indo-Australian and
Australian plate for the present and geologic past was
carried out utilising the software packages ABAQUSTM
and Nimrod/O. ABAQUSTM is a robust, industry
accepted finite-element modelling program and allowed
for simple creation and alteration of model geometries
and parameters using the program ABAQUSTM
CAETM (Complete ABAQUSTM Environment). Imple-
menting ABAQUSTM in conjunction with Nimrod/O
allowed for extensive exploration of parameter space
through automated execution of thousands of models
using intelligent optimisation techniques (Abramson et
al., 2000; Lewis et al., 2003).
In order to compare modelled results a residual misfit
value was calculated between modelled stress orienta-
tions and measured stress orientations contained in the
Australian Stress Map database (Hillis and Reynolds,
2000). In order to calculate the residual misfit, modelled
SHmax orientations were averaged over a small window
whose centre corresponded to the location of an average
SHmax orientation as determined by Reynolds et al.
del used in analysis. Model contains 24,400 plane stress elements
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Fig. 2. Mechanical provinces implemented in models. YL ¼
Yilgarn Craton; PB ¼ Pilbara Craton; AR ¼ Arunta Block;
MUS ¼ Musgrave Block; NC ¼ Northern Cratons; MI ¼ Mt:Isa Block; GA ¼ Gawler Block; NEB ¼ North East Block;
CB ¼ Central Block; MD ¼ Murray–Darling Basin; OT ¼
Otway Basin; LN ¼ Northern Lachlan Fold Belt; SN ¼
Southern Lachlan Fold Belt; NE ¼ New England Fold Belt;
CS�NW ¼ North�West Continental Shelf; CS� E ¼
Eastern Continental Shelf; CS� S ¼ Southern Continental
Shelf; White areas represent Basin. Values for mechanical
properties are listed in Table 1.
S. Dyksterhuis et al. / Computers & Geosciences 31 (2005) 297–307 299
(2002) for various regions over the Australian continent
and continental shelf. The difference between azimuths
of the average modelled and average measured SHmax
orientations then determined the residual misfit.
Modelling using the ABAQUSTM program is divided
into modules, the framework of which will be used to
discuss model construction. The ABAQUSTM Part,
Assembly, Step, Interaction, Property, Load and Job
modules are relevant to model construction while the
ABAQUSTM Visualisation module is used for graphical
analysis of model output data.
2.1. Parts and partitions
Geometrical models of the plates in the study were
constructed as sketches within the ABAQUSTM Part
module by projecting the latitudes and longitudes along
the model boundaries into Cartesian coordinates using
the Generic Mapping Tools (GMT) software (Wessel
and Smith, 1991). The projected latitude/longitude data
were interpolated along the plate boundary to obtain an
even sampling distribution. The data were then filtered
to remove high frequencies. ABAQUSTM python sketch
files were then created using the projected, smoothed
Cartesian coordinate data. The python sketch files can
then be easily imported into the ABAQUSTM environ-
ment using the ABAQUSTM CAETM Sketch module.
Regions representing areas within the model with
differing rheological properties were also created within
the ABAQUSTM model using the process outlined
above. These regions, however, were created as so-called
‘partitions’ within the model. Interaction between
ABAQUSTM model parts was set to a tie constraint
where a ‘master’ and ‘slave’ surface is defined with all
degrees of freedom for the nodes on the ‘slave’ surface
being eliminated, allowing for the joining of all parts in
the model to form one tectonic plate.
The Australian continent was subdivided into four
categories (cratons, fold belts, basins and continental
shelf) in the modelling process based on the differing
rheologies and strength of the continent as determined
by Zuber et al. (1989) and Simons et al. (2000).
Regarding terminology, note that use of the words
‘‘strength’’, ‘‘strong’’, or ‘‘weak’’, etc. within this paper
refer to relative stiffness or deformability within the
elastic regime (as governed by Young’s modulus and
Poisson’s ratio), as opposed to some measure of the
stresses or stress differences that result in an onset of
inelasticity. As we are constrained to (linearly) elastic
behaviour, we have no consideration for any departure
from that rheology. Fig. 2 shows the Australian
continent illustrating these areas. Results from seismic
tomography of the Australian continent (Kennett, 1997;
Simons et al., 1999) support the findings of Zuber et al.
(1989) and further indicate the existence of a seismically
slow, probably relatively weak zone located in central
eastern Australia (labeled CB in Fig. 2). The existence
of a weak zone in this area is also supported by high heat
flow data (McLaren et al., 2003). Simons and van
der Hilst (2002) pointed out that mechanical strength
and seismic thickness of the Australian continent do not
always match. Therefore, we only modified our
model for mechanical strength in one area in central
eastern Australia (CB in Fig. 2) where seismic tomo-
graphy and heat flow data provide strong evidence for
relatively hot and presumably weak lithosphere. The
relative strengths of the individual provinces were
implemented by altering the Young’s moduli of the
materials. Zuber et al. (1989) estimated the northern
Australian cratons to have the highest rigidity, with a
value of 2.1� 1025N/m2. Areas with this rigidity were
assigned an effective Young’s modulus of 6� 1010N/m2.
All other areas were assigned an effective Young’s
modulus scaled according to the ratio between their
rigidity and that of the highest rigidity as estimated by
Zuber et al. (1989). Table 1 lists the values of rigidity
determined by Zuber et al. (1989) and the scaled
effective Young’s moduli assigned to each of the
provinces implemented in the models.
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Table 1
Values defined for material properties used in model
Province Effective elastic
plate thickness
(km)a
Flexural rigidity
(� 1025Nm2)aScaling factor Scaled Young’s
modulus
(� 1010Nm2)
Refined Young’s
modulus
(� 1010Nm2)b
Refined rigidity
(� 1025Nm2)
Basins 64 0.25 0.12 1 1 —
Yilgarn Block 132 2 0.95 5.7 5.7 —
Pilbara Block 132 2 0.95 5.7 5.7 —
Northern Cratons 134 2.1 1.00 6 6 —
Arunta Block 88 0.61 0.29 1.74 1.74 —
Musgrave Block 88 0.61 0.29 1.74 1.74 —
Gawler Block 92 0.69 0.33 1.98 1.98 —
Mt. Isa Block 134 2.1 1.00 6 6 —
North Lachlan Fold
Belt
26 0.016 0.0076 0.046 0.06 —
South Lachlan Fold Belt 20 0.0077 0.0037 0.022 0.03 0.0105
North East Block — 2 0.9524 5.7 5.7 —
Murray–Darling Basin 29 0.022 0.0105 0.063 0.063 —
New Eng. F. B. 16 0.0036 0.0017 0.01 0.01 —
Otway Basin — — — — 0.063 0.02205
Oceanic crust — — — — 7 2.45
NW continental shelf — — — — 0.31 0.1085
Southern continental
shelf
— — — — 0.11 0.0385
Eastern continental shelf — — — — 0.031 0.01085
Central Block — — — — 0.02 0.007
aValues for effective elastic plate thickness and flexural rigidity from Zuber et al. (1989).bRefined values from stress modelling. Scaling factor determined by the ratio of the provinces value of flexural rigidity with the
highest value for flexural rigidity determined by Zuber et al. (1989).
S. Dyksterhuis et al. / Computers & Geosciences 31 (2005) 297–307300
The mechanical strength of the Australian continental
margin remains relatively poorly constrained. However,
it cannot exceed that of the continental lithosphere since
the continental margins are extended and thinned
continental lithosphere, and it cannot exceed that of
the adjacent, cool and relatively strong oceanic litho-
sphere. Modelled SHmax directions on the continental
shelf and within the continental interior are dependant
on the strength of the continental shelf. In order to
determine the strength of the continental shelf we have
compared two approaches. The first approach was to
assume that stretched continental crust thermally
reheated in the Late Mesozoic/Cenozoic has remained
mechanically weak (effective Young’s Modulus of
1� 108N/m2) since breakup, following the suggestion
by Fowler and McKenzie (1989) that thinned continen-
tal crust does not regain its elastic strength similar to
ageing oceanic lithosphere. This produced a model with
large residual misfit and poor correlation with observed
stress data (Table 2). The second approach was to
assume that the elastic strength of the continental shelf
has grown equivalent to ageing oceanic lithosphere
(Karner et al., 1983) and the continental shelf was
divided into three regions corresponding roughly to the
last age of thermal reactivation (Fig. 2). Values for the
strength of the individual regions were prescribed an
effective Young’s modulus range of 1� 108–1� 1010N/
m2. Final material property values in the model were
determined by minimising the residual misfit with
measured stress orientations through extensive explora-
tion of parameter space using Nimrod/O. The results
(Table 2) indicate that a continental shelf with varying
material properties best represents the strength of the
Australian continental shelf. This novel approach
demonstrates that stress orientation data can be used
for constraining the relative strength of continental
shelf, therefore helping to resolve the long-standing
controversy whether or not stretched continental litho-
sphere regains its strength like oceanic lithosphere in
principle.
2.2. Load definition and boundary conditions
Primary forces applied to models in this study
(Table 3) were the topographic forces of ridge push
and slab pull and the forces created at collisional
boundaries. A basal traction force was not implemented
due to the poor understanding and relatively uncon-
strained nature of this force. In the case of the
contemporaneous Indo-Australian Plate the dominant
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Table 3
Forces applied to contemporary and Miocene models
Location Contemporary Miocene
Mid-Ocean ridge 1.90 1.10
Australia–Antarctic Discordance 2.1 (3.1)a 1.7 (2.5)a
Papua New Guinea 3.80 —
Banda Arc �0.50 —
Java �0.30 �0.30
New Hebrides 1.00 —
Solomon 1.20 —
Sumatra 2.00 2.00
New Zealand 2.40 2.40
Southern New Zealand Alps 2.80 2.80
Tasman Sea 1.25 1.20
Carol — �0.60
Ontong Plateau — 2.50
Positive forces are directed towards the interior of the plate.
Note: Force magnitudes are 1� 1012N/m which is equivalent to
a stress of 10MPa across a plate of thickness 100 km.aForce applied where the effects from the Australia–Antarc-
tic Discordance were not included.
Table 2
Residual misfit between average predicted and average measured stress orientations
Provincea Homogeneousb Best Fitc No Australia
Antarctic
Discordanced
Uniform Continental
Margine
Amadeus 68.1 12.5 106.2 53
North Bonaparte 14 4.8 24 92.2
South Bonaparte 0.6 1.1 11 68.9
Bowen 143.1 92.3 95.4 74.15
Canning 21.7 11.5 33.8 44.7
Canarvon 1.8 7.9 16.8 5
Cooper 46.1 6.7 65.2 3
Gippsland 6.5 1.0 4.5 1.1
Otway 3.5 6.5 6.4 102.4
Perth 37 2.9 28 24.6
Total Residual Misfit 342.4 147.2 391.3 469.05
aAs defined by Coblentz et al. (1998) and Reynolds et al. (2002). The Models have the following differences:bhomogeneous material properties (Fig. 5);cmodel producing best fit with observed stress data (Fig. 6);dresidual misfit of model where effects of the Australia–Antarctic Discordance were not implemented;eresidual misfit of model with a uniform continental margin with an effective Young’s Modulus of 1� 10�8N/m.
S. Dyksterhuis et al. / Computers & Geosciences 31 (2005) 297–307 301
plate driving forces are the ridge push, slab pull and
collisional forces originating at collision zones north of
the Indo-Australian plate. The ridge push force (FRP)
arises due to elevated topography at mid-ocean ridges
(MOR), and is a distributed pressure gradient that acts
normal to the strike of the mid-ocean ridge (Wilson,
1993). The force contribution from the subsiding
oceanic lithosphere created at the MOR is given by the
relationship (Turcotte and Schubert, 2002 ):
FRP ¼ grmavðTm � T0Þ 1þ2
prmavðTm � T0Þ
ðrm � r0Þ
� �kt; (1)
where gravity (g) is 10m/s2, the densities of the mantle
ðrmÞ and water ðrwÞ are 3300 and 1000 kg/m3, respec-
tively, thermal diffusivity (k) is 1mm2/s, the temperature
difference between the mantle and the surface (Tm and
T0, respectively) is 1200K, the thermal expansion
coefficient (av) is 3� 10�5/K and t is the age of the
lithosphere in seconds.
The ridge push force was implemented in the
modelling process as a pressure applied along a
boundary representing the location where ridge push
force would be maximum, for example, if the ridge push
force was calculated for a mid-ocean ridge with a
spreading age of 45Ma, the pressure would be applied to
the 45Ma isochron boundary in the model. Figs. 3 and 4
illustrate the locations where forces were applied to the
contemporaneous and Miocene models, respectively.
The Australia–Antarctic Discordance is an area south of
the Great Australian Bight that is characterised by
bathymetry 800m deeper than the surrounding spread-
ing ridge (Gurnis et al., 1998), resulting in a relatively
diminished ridge push force. The exact difference in the
ridge push force arising from the Australia–Antarctic
Discordance is not well constrained, since factors
effecting the potential ridge push force from the
Australia–Antarctic Discordance do not merely rely on
the elevation of the ridge, but also the chemistry of the
underlying mantle (Gurnis et al., 1998), but has been
modelled here as a force 23that of the calculated RPF.
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Fig. 3. Forces applied to contemporary model are also illustrated; HYM ¼ Himalayas (fixed boundary); SUM ¼ Sumatra Trench;
JAVA ¼ Java Trench; BA ¼ Banda Arc; PNG ¼ Papua New Guinea; SOL ¼ Solomon Trench; NH ¼ New Hebrides; CT ¼
Continental Topographic Force; TS ¼ Tasman Sea; NZ ¼ New Zealand; SNZ ¼ Southern New Zealand Alps;
AAD ¼ Australia–Antarctic Discordance; MOR ¼ Mid-Ocean Ridge. Boundary between light grey area along which MOR and
AAD force arrows are located is region along which ridge push force was applied for contemporary model. Note that force arrows are
not drawn to scale.
S. Dyksterhuis et al. / Computers & Geosciences 31 (2005) 297–307302
The slab pull force (FSP) originates from the negative
buoyancy of the down-going dense oceanic lithosphere
at subduction zones and is proportional to the excess
mass of the cold slab in relation to the mass of the
warmer displaced mantle (Spence, 1987). The force
contribution can be given by the relationship (Turcotte
and Schubert, 2002):
FSP ¼ 2rmgavbðTc � T0Þkl2pu0
� �12
0@
1A
þ2ðTc � T0Þg Dros
rm
kl2pu0
� �12
0@
1A; ð2Þ
where b is the slab length, l is 4000 km, u0 is 50mm/yr, gis 4MPa/K, DrOS is 270 kg/m3, other parameters are
described in Eq. (1).
For fast moving plates (5–10 cm/yr) the subducting
slab attains a ‘terminal velocity’ where forces related to
the negative buoyancy of the slab are balanced by
viscous drag forces acting on the slab as it enters the
mantle and the net force experienced by the horizontal
plate is quite small (Forsyth and Uyeda, 1975). The
amount of net force actually transferred to the
horizontal plate, however, is still quite controversial.
Schellart (2004) suggests as little as 8–12% of slab pull
force is transferred to the horizontal plate while Conrad
and Lithgow-Bertelloni (2002) suggest as much as
70–100% may be transmitted. Magnitudes of slab pull
forces were varied over a range of 1� 107 to
�1� 10�7N/m with final force magnitudes constrained
by the resulting fit with the measured stress directions
contained in the Australian Stress Map database (Hillis
and Reynolds, 2000), as were the forces at collisional
boundaries. The collisional boundary between the IAP
ARTICLE IN PRESS
Fig. 4. Miocene model setup illustrating forces applied. CA ¼ Carol Trench; refer to Fig. 3 for more details on other plate boundary
names.
S. Dyksterhuis et al. / Computers & Geosciences 31 (2005) 297–307 303
and Eurasian plate at the Himalayas was modelled as a
fixed boundary in the modelling process in order to
maintain mechanical equilibrium.
2.3. Visualisation
The ABAQUSTM CAETM Visualisation module is
used to view the model results, however, it was found to
be limited in its capabilities of data representation. In
order to have more control over the data visualisation
the *El Print and *El File options in the analysis input
file were used to output variable data from the analyses
into the analysis data and results files. The ABAQUSTM
fprin subroutine was then used to calculate the elemental
stress values and also the direction of the stress vectors.
These data were then plotted using the GMT software,
allowing for more flexibility in data visualisation.
2.4. Palaeo-modelling method
A palaeo-stress model (Fig. 4) for the Miocene
(20Ma) was created using reconstructed plate boundary
configurations (Heine et al., 2004; Hall, 2002) and the
age–area distribution of ocean crust around Australia
(Muller et al., 2000) to obtain estimates of spatial
distribution and magnitude of ridge push and slab pull
forces, while estimates of forces acting at other
boundaries were extrapolated using results of contem-
porary stress modelling. Values for material properties
were held constant with the values used in and obtained
from the contemporary stress analysis.
3. Results
3.1. Contemporary
Our results show that spatially significant rotations of
the SHmax direction can be modelled as a consequence of
perturbations of SHmax in areas of juxtaposed strong and
weak rheologies. The materials with higher values of
rigidity deform only slightly under a given loading, and
so place relatively small displacements on the bound-
aries of adjacent, weaker materials. This results in
ARTICLE IN PRESSS. Dyksterhuis et al. / Computers & Geosciences 31 (2005) 297–307304
deviation of stress trajectory directions within higher
rigidity materials around weaker materials. Large
differences in both magnitude and direction of SHmax
can be seen around areas in the Australian continental
lithosphere where there are juxtaposed strong and weak
rheologies. Fig. 5 shows the predicted SHmax regime for
a model with homogeneous material properties while
Fig. 6 shows the ‘‘best fit’’ model obtained out of many
thousands of model runs using heterogeneous material
properties. It is clear that the stress pattern predicted by
a model with heterogeneous material properties shows
more variance in SHmax direction and magnitude than
that of a model with homogeneous material properties.
This is best illustrated over the western margin of the
Yilgarn Craton (marked YL in Fig. 2) where there is up
to roughly a 901 rotation of the stress direction over an
area roughly 200 km in diameter. The model also
emulates the observed 891 rotation in SHmax orientation
between the Amadeus and Cooper basin stress provinces
defined by Reynolds et al. (2002) well with reasonably
low residual misfits in the Amadeus and Cooper basins
of 12.5 and 6.7, respectively. Such spatially rapid
Fig. 5. Modelled contemporary maximum horizontal compressive str
properties. Filled grey lines indicate compressional stress while filled bl
a circle show measured stress orientations of A–C quality taken from
variation in SHmax directions is not present in the
homogeneous model. While the value of residual misfit
for the heterogeneous model in the Bowen Basin is quite
high (Table 2), modelled SHmax magnitudes are lowest in
this region indicating that local sources of stress may
play a dominant role in controlling the orientation of
SHmax (Zoback, 1992).
3.2. Miocene
Forces applied to the boundaries of the Miocene
(20Ma) model are illustrated in Fig. 4 and listed in
Table 3. Docking of the Australian plate with the
Ontong–Java plateau had begun in the early Miocene
(Hall, 2002), however, collision with Papua New Guinea
had not yet been initiated; instead the Australian plate
was subducting beneath the Caroline plate (Hall, 2002).
Forces along the plate boundary at New Zealand were
similar to those at present with the inception of the
Alpine Fault occurring at 23Ma (Kamp, 1986).
The absence of the collisional Papua New Guinean
boundary to the north of the Australian continent in the
ess (SHmax) orientations for a plate with homogeneous material
ack lines indicate tensional stress. Filled black lines marked with
Australian Stress Map database.
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Fig. 6. ‘Best Fit’ modelled SHmax orientations with realistic material properties for the Australian continent and continental shelf (see
Fig. 2 for further explanation of provinces). Filled grey lines indicate compressional stress while filled black lines indicate tensional
stress. Filled black lines marked with a circle show measured stress orientations of A–C quality taken from the Australian Stress Map
database.
S. Dyksterhuis et al. / Computers & Geosciences 31 (2005) 297–307 305
Miocene produces a dramatically different stress regime
(Fig. 7) to that of the present. The stress distribution is
more uniform with less spatially rapid variation. A
general NW–SE SHmax orientation is evident over the
Australian continent during the Miocene, whereas at
present there exists a general NE–SW trend over
Northern Australia with SHmax orientations over the
southern continent displaying more variation. Orienta-
tions of SHmax directions over the NW shelf and Bass
Straight region in particular show large differences
during the Miocene compared to present, with modelled
SHmax orientations agreeing well with fault reactivation
histories of these areas.
SHmax directions over the NW shelf have changed
from a NW–SE orientation in the early Miocene to a
general NE–SW at present. Reactivation histories of
coast-paralleling extensional basin forming faults on the
Canarvon Terrace on the NW shelf occurred during the
Miocene (Baillie and Jacobson, 1995; Muller et al., 2002)
with migration of hydrocarbons also taking place at this
time (Crostella and Boreham, 2000). This is consistent
with the results of this study which show rotation of
SHmax directions over the Canarvon Terrace from
orientations oblique to the coastline during the early
Miocene to orientations normal to the coastline at
present.
Inversion in the Torquay Embayment and Otway
Ranges of the Bass Strait region occurred in the
Miocene due to compressional reactivation of numerous
NE striking extensional faults (Hill et al., 1995).
Modelled SHmax results in this region of the Bass Strait
show a rotation from roughly EW in the early Miocene
to NNW–SSE at present, indicating a SHmax regime
conducive to compressional inversion in the Torquay
Embayment and Otway Ranges existed between the
early Miocene and present.
4. Summary
Modelling the intraplate stress regime of tectonic
plates represents a novel use for the engineering software
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Fig. 7. Modelled Miocene SHmax orientations. Filled grey lines indicate compressional stress while filled black lines indicate tensional
stress.
S. Dyksterhuis et al. / Computers & Geosciences 31 (2005) 297–307306
package ABAQUSTM that has not previously been
explored. We have developed a methodology implemen-
ted as programs and shell scripts which allows for
straightforward creation of geophysical models within
ABAQUSTM CAETM. All programs and scripts used to
create models in ABAQUSTM as part of this work can
be accessed at www.geoframework.org and are freely
available for use and alteration under the GNU license
agreement.
We have modelled the maximum horizontal compres-
sive stress regime for the Indo-Australian plate for the
present and Miocene. Methods developed allow for easy
creation of models with different geometries. The
Generic Mapping Tools software (Wessel and Smith,
1991) has been used to plot the modelled and measured
data. Modelling results show significant perturbations of
SHmax directions and magnitudes in areas of juxtaposed
weak and strong materials in the heterogenous model.
The results demonstrate that models with heterogeneous
material properties fit observed stress directions con-
tained in the Australian Stress Map database better than
models with homogeneous material properties. Rapid
spatial rotations of SHmax directions, as seen in the
observed stress data, cannot be reproduced in homo-
geneous models, only in models with heterogeneous
material properties. Modelled Palaeo-SHmax orientations
also demonstrate the dramatic changes in SHmax regime
that occurred over the Indo-Australian plate between
the Miocene and present day, with modelled SHmax
regimes agreeing well with fault reactivation histories
over the NW Australian Shelf and in the Bass Strait
region.
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