Tectonophysics, Elsevier
173 (1990) 247-256
Science Publishers
247
B.V.. Amsterdam
- Printed
in The Netherlands
Deep seismic profiling in central Australia C. WRIGHT
‘, B.R. GOLEBY
*, C.D.N.
COLLINS
S.A. GREENHALGH ’ Bureau of Mineral Resources,
‘, R.J. KORSCH
2 and S. SUGIHARTO
*, T. BARTON
‘,
3
C.P.O. Box 378, Canberra, A.C. T. 2601 (Australia)
2 School of Earth Sciences, Flinders University of South Australia, ’ Sceptre Resources Pty. Ltd., Jakarta (Received
October
5, 1988; accepted
C.D.N.,
Korsch,
R.J., Barton,
Bedford Park, S.A. 5042 (Australia) (Indonesia)
April 13,1989)
Abstract Wright,
C., Goleby,
B.R.. Collins,
seismic profiling (Editors),
in central
Seismic Probing
Deep seismic profiling
Australia.
of Continents
undertaken
refraction
work and a small-scale
reflection
profiling.
dipping mapping.
events that are interpreted The Redbank
defines
a marked
absent;
sub-horizontal
Seismic
refraction
Southern
the resolution
basement
Zone,
refraction
Australia
a major
velocity
of anisotropy
feature, below
long,-range
spread
incidence
Block in central
reflection
Australia
has been imaged Zone,
the Southern
show abundant
to depths
Arunta
reflections
are
Basin.
between
the
reflection
spreads
and
of special geological
interest,
and
rocks of the northern Arunta
northerly geological
and Amadeus
the boundary
Basin. Expanding
to the results in regions of the Central
dipping
Province both
in surface
of at least 30 km, and
steep, northerly
50 km thick below
in the sedimentary
in the granulites
Kennett
profiling,
part of the Amadeus
fine details
S., 1990. Deep
and B.L.N.
173: 247-256.
faults, many of which are evident
is more than
variations
J.C. Dooley
as well as the more usual near-vertical
South of the Redbank
and the northern
survey have added
of complicated
from dipping
are prevalent
that the crust
Provinces
the Anmta
thrust
expanding
survey,
S.A. and Sugiharto,
C. Wright,
Tectonophysics,
comprised
refraction
within
character.
reflections
indicate
Arunta
Basin and the measurement
sections
in reflection
profiles
and Central
a tree-dimensional include
in central
as reflections
Deformed
change
and their Margins.
three-dimensional
Seismic reflection
T., Greenhalgh,
In: J.H. Leven, D.M. Finlayson,
Province
part of the Amadeus
adjacent
to the Redbank
Zone.
In 1985, the Australian
Bureau
of Mineral
Re-
deep-reflection and long-range refraction profiling. Finally, some key results from expanding spread reflection and three-dimensional refraction
sources undertook a program of seismic reflection and refraction profiling across the Arunta Block
profiling are discussed. The implications tectonic evolution of the central Australian
and the Ngalia and Amadeus Basins in central Australia (Fig. 1). The purpose of the seismic work was to constrain the structure of the deep
are discussed et al. (1990).
crust and to test models of the geological evolution of the central Australian region. A summary of the seismic recording parameters is given by
The geology and evolution of the central Australian region
Goleby et al. (1988). In this paper we review briefly the tectonic problems that have been identified by earlier geological and geophysical studies, and present the most significant results of the
The Arunta Block (Fig. 1) has been interpreted as a Proterozoic mobile belt underlain by continental crust. It consists of three tectonic provinces, each with separate histories of deformation
in the companion
paper
for the region
by Goleby
AMADEUS
@----
ov
BASiN
Refraction
survey
f 1985/
Refraction
survey
(19881
Reflection
profile
(1985)
El, E2. E3 @-
Expanding
RDZ-
Redbank
GF - Gardmer
Road
M P - Missmnar
Fig. 1. Map of central reflection
spreads
Australian
and transmission
survey
area showing
tomography
location
experiment.
central
of seismic
The Arunta
and southern
and metamorphism (Shaw et al., 1984). The Redbank Deformed Zone (RDZ) that forms much of the northern boundary of the Southern Arunta Province is an easterly-trending zone of anastomosing mylonites, 7-10 km wide, dipping northwards at about 45”. In the region covered by the seismic profiling, granulite facies rocks of the Central Arunta Province have been thrust southwards over amphibolite-facies migmatitic gneisses of the Southern Province (G&son, 1987; Shaw, 1987). The Ngalia Basin covers much of the southern part of the Northern Province of the Arunta Block and contains Late Proteruzoic and Palaeozoic
spread
Three -’dfmensmnal
reflection
deformed
survey
zone
Fault y Plain
lines, seismic
Block is divided
(abbreviated
locations
refraction
refraction
into three tectonic
profiles, provinces:
expanding northern,
to STH).
sedimentary rocks of 6 km maximum thickness (to the west of the seismic profile of Fig. 1) that can be correlated with sedimentary rocks of the Amadeus Basin (Wells and Moss, 1983). The Amadeus Basin is an east-west trending intracratonic depression of about 800 km length, bounded on the north and south by the Arunta and Musgrave Blocks, respectively. It also contains Late Proterozoic and Palaeozoic sediments that reach a maximum thickness in the northern part of the basin of 14 km; south of the Gardiner Fault (Fig. l), the sedimentary cover in the southem platform region of the basin is much thinner (Wells et al., 1970; Lindsay and Korsch, 1989).
DEEP
SEISMIC
PROFILING
IN CENTRAL
Some of the largest any where
continent
gravity
present
the total variation
Generally, occur
are
the most
near
anomalies
in central is about
negative
the basin
249
AUSTRALIA
margins
seen on Australia,
1400 pm s-‘.
Bouguer while
anomalies the positive
solely stretching the basins northern
and southwestern
Australian
of the gravity
The
field in central
and
Wellman
Australia
and Shaw (1973)
(1978).
Basins have a complex
were de-
tive model
profiles
and
Ngalia
eation
over a
the deep crust, the mapping
evolutionary
history
basin
margins
of changes
of major
help
in crustal
The are also
Models in the
for the central
by Teyssier
(1985)
(1987)
may
locations
period of crustal compression, during which time the crust buckled to form the depocentres and significant developed
seismic
Shaw
(1976)
long period of time (c. 600 Ma). A mechanical model by Lambeck (1983) invokes a protracted
basement
and
because
equilibrium.
region were devised
(thin-skinned)
Mathur
The Amadeus
mechanisms,
in isostatic
characterised by thrust structures. style of crustal deformation
anomalies correspond to the Arunta and Musgrave Blocks. Models of the crust to explain the features vised by Anfiloff
or thermal
are not
(thick-skinned). to constrain
thickness,
faults or detachment
the
the delin-
surfaces
of sedimentary
into thick-
nesses throughout the basins, and the overall geometry of the basins. These features will assist in discriminating between evolutionary models of the central
Australian
region.
highs. A revised model that still invokes periods of compressional tectonics was by Lambeck et al. (1988). An alternaby Lindsay
and
Korsch
(1989)
pro-
poses a complex history involving both extensional and compressional mechanisms. The evolution of the region cannot be satisfactorily explained by models of basin formation involving
Results from near-vertical incidence profiling Northern
and Central Arunta
Provinces
The main features inferred from the stacked seismic sections are shown with the gravity profile in Fig. 2. Figure 3 is a migrated version of Fig. 2,
s
N
AMADEUS
BASIN
I
ARUNTA BLOCK
1j)Okm
Fig. 2. Line diagram of main north-south
reflection line Ll (Fig. 1) with the observed gravity profile. Regions of prominent
reflections have been marked by thicker lines, and shading denotes zones of strong reflected energy. Vertical exaggeration is 2 an average velocity of 6.0 km s-‘.
MN, GH and EF show locations of seismic sections of Figs. 4 and 5.
: 1 for
250 AMADEUS Southern
S
SI
G
Reg,on
N
N
M
Missionary
BASIN
Plattorm
ARUNTA Redbsnk
Plain “1
BLOCK Ngalla Basin
n
E
N
40km
Fig. 3. Line diagram of Fig. 2 migrated with a constant velocity of 6.0 km s-‘. Vertical exaggeration is 2 : 1. MN, GH and El” show locations of seismic sections of Figs. 4 and 5.
assuming a constant seismic velocity of 6.0 km s-‘. The band of northerly dippixtg reflections at tW between 2 and 10 s beneath the Northern Ar~ta _Province is ~~~1~~~ strik&g (Figs. 2 and 3). -These reflections dip 20-W W probably coqnd to a series of fax& surfaces. This interpretation is consistent with the pattern of dipping faults within the Arunta Block inferred from the surfp geology. Further south, the strength of the r&Iections diminishes soznewhat in the granulites of the Central Arunta Province, though the ap-
parent northerly dip of the reflections contiitues. The most significant boundary of the entire profile is the RDZ which is &x&y i asaplausar feature to depths of at least 30 km, ihe m&ted dip is about 35-40”. Southern Arunta Province and Northern Awwdms Basin To the south of the RDZ, the feflectioa character is quite different. The persistent, steep,
DEEP SEISMIC
PROFILING
IN CENTRAL
AUSTRALIA
COP
Fig. 4. Seismic sections Southern
recorded
Arunta
in the northern
Province
part of the Amadeus
(B) corresponding
northerly apparent dip of the observed absent, and the section contains strong
signals is sub-hori-
zontal bands of reflected energy at times greater than 6 s. Figure 4B shows prominent deep reflections within 21-30
the Southern
Arunta
km) that are also observed
Basin (A) corresponding
to EF of Figs. 2 and 3. The gap between
Province at earlier
(depths times
on the parallel profile (L2 of Fig. 1) to the east, so that there is a small westerly component of dip as well as the northerly component evident in Fig. 4B. Figure 4A shows the seismic section at the northern edge of the Amadeus Basin, where the sedimentary section is more than 10 km thick. The lowermost part of the Proterozoic sequence gives rise to the discontinuous reflection segments at times greater than 3.2 s, and the uppermost basement boundary is not clearly defined. The reflections die out at the northern end of Fig. 4A, close to where surface geological observations show that the sedimentary rocks have been folded upwards. The deep section of Fig. 4B has a layered character similar to sections observed in some other Proterozoic areas, such as the Siljan impact structure in Sweden (Dahl-Jensen et al., 1987); drilling in the Siljan area has shown the reflectors to be mafic sills (Juhlin, 1990). Sills of mafic rocks or alternating layers of mafic and felsic rocks provide an acceptable explanation of the deep reflections observed below the Southern Arunta Province. The youngest intrusions observed in the surface geology of the Southern Arunta Province
to GH in Figs. 2 and 3, and in the the sections
is about
20 km.
are the Stuart Dyke Swarms (south and east of L2 of Fig. I), of doleritic composition, and dated at about 900 Ma (Black et al., 1980). They pre-date the youngest sedimentary rocks of the Amadeus Basin. However, rocks of sedimentary origin could also explain the large reflection coefficients. Is it possible that the deep reflections of Pig. 4B are from
rocks
that
were
originally
part
of
the
Amadeus Basin, in which case they would delineate a major overthrust? Or could the reflectors represent deep crustai shear zones? The latter explanation appears unlikely because of the relatively high reflection amplitudes and the thickness (about 10 km) of the reflecting region, but cannot be dismissed entirely (see Warner, ‘1990). Reprocessing of the data at the northern margin of the Amadeus Basin may provide clues by enabling clearer imaging of some faults. Southern platform
Strong
region of the Amadeu.v Basin
reflections
are observed
throughout
the
sedimentary rocks of the northern part of the Amadeus Basin (Figs. 2 and 3). A vertical uplift of the southern block of about 5 km is inferred along the Gardiner Fault from the seismic sections. Reflections from the sedimentary section together with some multiples remain clear for a distance of 40 km south of the Gardiner Fault. However, further south within the southern platform region,
and the bands of deep basement reflectrons are almost a mirror image of the northerly dipping bands of deep reflections observed below the Southern Arunta Province (Fig. 4) and the fainter reflections
associated
with the Ormiston
Nappe
and Thrust Zone (Goleby et al., 1990). The similarity of the style of basement the southern Amadeus
reflectivity
below
Basin to that below the
Southern Arunta Province suggests that the basement from south of the RDZ margin
of the Amadeus
Basin
to the southern forms
a single
tectonic province. The base of the crust, usually defined as the transition to a lower non-reflective region, is not clearly discernible along the profile, though a crustal thickness of 35-40 km appears reasonable below the Northern Arunta Province (Goleby et al., 1990). Fig. 5. Seismic section Basin, 5.5-6.2
showing
strong
s (MN southerly
from the southern bands
of Figs. dipping
part of the Amadeus
of reflected
2 and
energy
3). Note
thrust marked
also
starting
at
the possihle
by arrows.
shallow reflections become diffuse, and there are few clear reflections from the deep crust. The absence of strong shallow reflections continues to the southern end of the profile; the sedimentary cover is often less than 2.5 km thick throughout the southernmost
150 km. Variable
thicknesses contribute
Other seismic profiling
weathering
to the poor record quality,
but reprocessing with improved statics corrections has resulted in better resolution of some reflections.
Seismic refraction profiies The refraction survey recorded to offsets of 350 km in 1985 and extended to 500 km in 1988 (Fig. 1) showed no Pn arrivals (Wright et al., 1987; Goleby et al., 1988). Several branches of later arrivals (Fig. 6) can be interpreted as possible wide-angle reflections from the crust-mantle boundary (PmP), suggesting an average crustal thickness of at least 50 km for the region of the Southern
Arunta
Province
that has been thrust
below the Central Arunta Province (Fig. 2). Seismic refraction data recorded across the north-
Strong reflections similar in appearance to those observed beneath the Southern Arunta Province occur at times between 5 and 10 s below the southern part of the southern platform region (MN of Figs. 2 and 3; Fig. 5). There is an apparent dip to the south, and the onset of these bands of reflections is sharp over a distance of more than 40 km. Figure 5 also shows a planar, southerly dipping feature with an apparent dip of about 20” that is interpreted as a thrust fault; at
Expanding reflection spreads and three-dimensional refraction profiling
times greater than 2 s, the observed energy is reflected from within basement. South of the present seismic profile, in the Musgrave Block, the existence of southerly dipping thrusts is well established from geological evidence (Collerson et al., 1972). The southerly dip of the inferred thrust
Expanding reflection spreads were recorded in the Arunta Block and northern part of the Amadeus Basin (Fig. 1; Wright et al., 1990). The Amadeus Basin expanding spread yields a detailed average velocity model for the basin sedimentary
ern part of the Amadeus Basin (Fig. 1) also indicate a crustal thickness in excess of 50 km. An intra-crustal increase in seismic velocities from 6.2 to about 7.0 km s- * occurs at 40 km depth below the Amadeus Basin, in contrast to 30 km within the Southern Arunta Province.
DFFP
SFISMIC
PROFTI.ING
IN CENTRAL
253
AUSTRALIA
ARUNTA
BLOCK REFRACTION
TRAVERSE
w
AMADEUS
BASIN
Oastance
Fig. 6. Seismic refraction
sections,
Arunta
Block and Amadeus travel-time
REFRACTION
(km)
Basin. Numbers branches
rocks that shows two pronounced low-velocity layers (Fig. 7); its main function is to assist studies of basin evolution by providing reliable seismic velocity estimates at depths below 3 km, where velocity resolution from both industry and BMR seismic reflection profiling is poor (Wright et al.,
TRAVERSE
in km s
on sections
represent
apparent
velocities
of identified
‘.
et al., 1988; Greenhalgh et al., 1990b). The refracted arrivals recorded by the remote instruments, after reduction by a tomographic inversion technique, show significant lateral heterogeneity in the crystalline rocks of the Central Arunta Pro-
1990). A geological interpretation of Fig. 7 is given by Wright et al. (1989). While the two expanding spreads were being recorded in the Arunta Block, remote seismic recorders were deployed on the line orthogonal to
vince (Greenhalgh et al., 1990b). Superimposed on this lateral heterogeneity is about 7% anisotropy (Fig. 8) attributed mainly to propagation through strongly foliated granulites formed at depths below 25 km and thrust up to the earth’s surface; the direction of maximum velocity (east-west) coin-
the one with the shots and reflection spread to give three-dimensional refraction coverage (Goleby
cides with the dominant direction of foliation inferred from geological studies in nearby outcrop
254
4.5
R.m.5.
Velouty (km;s) 5.0
5.5
(Glikson, 1987; Greenhalgh et al., 1990a). The expanding spreads recorded within the Arunta Block also indicate a region of increased reflectivity between depths of about 27 and 35 km with seismic velocities in excess of 7 km s-’ (Wright et al., 1990); this is in good agreement with the refraction results of Fig. 6.
6.0
veicciti
Condusious
Fig. 7. Root mean square (r.m.s.) velocity measurements (dots) with standard errors for sedimentary rocks of the Amadeus Basin. IntervaI vehxities have been computed from the smooth curve (cubic spbne) fitted through the r.m.s. velocity terms. A, B, C and D refer to prominent reflections on the seismic section that were used to define dip and moveout corrections for r.m.s. velocity measurements (Wright et al., 1989). Numbers on the right are approximate depths of reflrztions.
Persistent northerly dipping events within the Northern and Central Arunta Provinces are best explained as reflections from faults. Strong reflections within the Southern Arunta Province and the southern part of the Amadeus Basin are produced at depths between 18 and 30 km and have a layered character. The RDZ forms the most fundamental boundary of the survey region and is interpreted as a planar feature extending to depths of at least 30 km. Crustal thickness exceeds 50 km beneath the northern part of the Amadeus Basin and the Southern Arunta Province. It appears to decrease to 35-40 km below the Central Arunta Province. The reflection profiles support a thickskinned model of the tectonic evolution of the central Australian region (Shaw, 1987; Goleby et al., 1990), and suggest a present crust-mantle configuration that agrees best with that proposed by Lambeck et al. (1988). Experimental profiling
5 0
90
270
180 Azimuth
360
(deg)
Fig. 8. Seismic velocity versus azimuth for gram&e facies rocks of the Neutral Arunta Province, showing about 7%anisotropy.
DEEP
SEISMIC
yields
PROFILING
detailed
IN CENTRAL
information
the granulites
at shallow
of the Central
Arunta
on the three-dimensional
structure
An expanding
spread
northern thick
reflection
part of the Amadeus
constrained stratigraphic
on and
of the RDZ. recorded
throughout
sequence,
studies
depths
Province
in the
Basin provides
seismic vefocities
sedimentary
255
AUSTRALIA
that
of basin
well
the 9 km
are
useful
in
Arunta
Block,
evolution.
Greenhalgh,
S.A., Sugiharto,
1990b. Tomographic ity variations J.H.
B.L.N. and
Kennett
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We thank B. Drummond and D. Finlayson for critically reading the manuscript. This paper is published with the permission of the Director, Bureau of Mineral Resources.
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(Editors),
Margins.
C. Wright, Seismic
Tectonophysics,
J.C
Probing 173:
Dooley
dnd
of (I ontinents 73--X2
(this