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My research interest has focused on understanding the role of hydrous and
magmatic fluids in orogenic systems; an explanation to their possible origin(s)
in the crust and upper mantle and their implications to partial melting and
rheology changes, their role in fault systems, and the relation between fluid
flow and lithospheric deformation.
I specialized
in the Magnetotelluric (MT) and Geomagnetic Deep Sounding (GDS) methods, which
measure the natural time variations of the electric & magnetic fields at the
earth's surface originating from ionospheric & magnetospheric currents, inducing
telluric currents under the surface. The aim of MT and GDS measurements is to
obtain the electrical conductivity values of the underground as a function of
depth at each station, and build two-dimensional or three-dimensional
conductivity models of the earth by calculation of the Maxwell field equations
through numerical forward algorithms (e.g., finite element or finite
difference), and through model inversion. I have built 2-D and 3-D electrical
conductivity models of the earth's crust and mantle in active continental
margins (Andean subduction zone) and in a craton (the Slave, NW Canada;
Jones et al., 2003),
giving a geo-tectonic interpretation in the
context of other geological & geophysical observations such as seismic
reflection and attenuation, gravimetry, heat flow measurements and geochemistry.
Hydrous fluids play a key role in the temperature dependent metamorphic
reactions of rocks producing state and compositional changes, affecting the bulk
electrical conductivity of the material. Salinary fluids flowing in a permeable porous
material will enhance ionic conductivity, increasing the total conductivity value with
increasing porous interconnection.
My PhD thesis research involved the analysis and 3-D modeling
of magnetotelluric data collected in the Southern Central Andean subduction
zone. The conductivity structures of the model integrated with geothermal
gradients and seismic reflectors bring insights into the properties of
lithospheric deformation for the fore- and magmatic-arc region of the subduction
zone (Fig.1).
Fluids flowing in partially molten rocks matrix (of enhanced bulk conductivity)
and beyond cause a reduction of the melting point temperature that can lead to
an expansion of the melting process beyond the existing boundaries. The brittle-
ductile transition zone may be affected when molten rocks are displaced into
deeper zones of higher temperatures.
A good example of an anomalous ductile rheology of the lithosphere in an active orogenic system
is found from geophysical observations in the
back-arc of the Andean subduction zone at latitude 24 S, underneath the Puna
plateau.
An upward
lithospheric displacement of the brittle-ductile transition zone beneath the
Puna occur, with a ductile -partially melted- lower crust associated to active
magmatism and tectonic deformation. The asthenospheric upwelling is supported by
both high seismic attenuation values and the temperature dependent electrical
conductivity values obtained from magnetotelluric modelling (
Lezaeta et al., 2001).
Conductvity model of the Andean subduction zone at latitude 20-21.5 S
The
model on the right
shows a W-E cross section at latitude 20.5 S of a
3-D electrical resistivity (the inverse of conductivity) model obtained from magnetotelluric
surveys carried along the Southern Central Andes subduction system. Explanations
of the main features presented in the model are shown in the
figure caption
(taken from: PhD Thesis, pp
159-167).
Interpetation of the conductivity model is
explained below for each along strike geological region forming the fore- and magmatic-arc
of the Andean subduction system at latitute 20- 21.5 S:
Coastal Cordillera mountain range (forearc):
The resolution in depth of an upper crustal high conductivity zone (<10 km depth)
along the Atacama mega strike-slip fault (AF) of the Coastal Cordillera cannot
be resolved from on-shore measurements due to the screen effect of the
conductive ocean. Ocean bottom surveying would allow discriminating the presence
of a conductive zone in the (coupling) seismogenic zone near the mantle wedge
associated to an
hydrated oceanic slab (high Vp/Vs ratio and low attenuations), in which case
fluids could be released from dehydration and find their pathway upward through
the fractured brittle crust. This hypothesis would be proofed by finding high
conductivity values along vertical pathways associated to the Atacama
fault system reaching down to moho depths (40-50 km). In the current model
obtained from land measurements, the Atacama fault system at latitudes between
20 S and 21.5 S appears to be highly conductive in a vertical dike-like fashion
at least down to depths of 10 km. These structures are vertical pathways for
salinary fluids that may have origined from meteoric (surficial) waters at least
for the upper crustal levels. Besides the meteoric water, that is rainwater and
fluvial sources, surficial fluids may also have come originally from thermal
convections developed at mid-crustal level excited by intrusions.
Porous rocks can also have retained
water from dehydration of past methamorphic reactions occured within the mid-
crust. The Coastal Cordillera was subject to postgradational metamorphism during
the Jura (210-120 Ma), and may have continued with retrograde metamorphism
during the emplacement of the volcanic arc to the east. Metamorphic fluid fluxes
and crustal porosities could have well be maintained long after the end of
dehydration metamorphism (>100 Ma), with fluid production ending after about 70
Ma (e.g., Thompson & Connolly, 1990). Thus, water may have been trapped in the
fractured rocks until presently, especially if the vertical pathways extend
beyond 10 km depth downto mid-crustal levels.
Mineralizations in the active shear zone
or ore fluids can also enhance conductivity. Ore minerals have
higher densities than the average crust, leading to enhance the
P-wave velocities and resulting in positive isostatic residual
field, in accordance with geophysical observations in the Coastal
Cordillera. On the other hand, highly
conductive minerals such as illmenite, magnetite and pyrhotine can
develop aligned in shear zones. The widespread
nitrate deposits east of the Atacama fault
are probably related to metallogenetic events, where ore fluids
may have been channeled in the Atacama fault system, such as that
from epithermal gold-silver.
The origin of the fluids in the Atacama fault can be a combination
of the mechanisms explained above. However, the hypothesis
regarding the upward migration of water into the crustal
fractures released from the seismogenic zone, can not be
supported by the MT observations on land. The levels of the slab are
beyond the penetration depths of the MT data since measurements
carried out off-shore are required to resolve this zone as outlined above.
Precordillera Fault system (forearc):
The High Conductivity Zone (HCZ) in the Precordillera (PC) can be separated
into two blocks. A shallow structure (<5 Ohm.m) between 2
and 10 km deep in the form of approximately N-S elongated
conductors along the Precodillera fault system (PCFS); a deeper
block below 10 km depth with lateral N-S gradient of conductivity
decreasing from north to south. Its central part (at 20.5°S)
extends to the west in the Longitudinal Valley. See
overview of the 3-D model at different depths to identify the structure
of the Precordillera HCZ.
The upper crustal dike-type conductors can be
related to the Precordillera fault system, and hence explain the
conductivity enhancement as being due to salinary fluids
circulating in the fractures of the brittle upper crust
(temperatures <200°C;
fig.1).
In the
western PC as well as part of the Longitudinal Valley, a N-S
thrust-fold system has been inferred from an isostatic model
(fig.1;
west of 69°W), and is interpreted as
the west-flank of the Miocene-Holocene tectonic Altiplano uplift
which developed in connection with ignimbrite-magmatism
(Victor et al., 2000). The thrust-fold in the western PC as well as
the West Fissure (WF) shear zone are geological structures
recognizable in the field. The
upper crustal dikes at latitude 20.5°S correlate well with the PC
thrust-fold system and the WF
(fig.1).
The depth of the WF ($\sim$25 km) is presumed by accounting for the
isostatic model of the thrust-fold system by Victor et al. (2000),
the geothermal gradient and the low seismic velocity zone at a
30-40 km depth modeled by Yuan (2000) from P-S converted
seismic phases. Thus, the crust in the Precordillera can be
considered to have a brittle regime at depths above 30 km, whereas
at depths below about 30 to 40 km it undergoes a brittle-ductile
transition (with temperatures between 300°C and 500°C;
Fig.1).
The temperatures in the lower crust
and upper mantle do not exceed 650°C, indicating that partial
melt is not possible here, supported also by the lack of high
seismic attenuation registered in this zone (e.g.,
Haberland, 1999).
A larger high conductivity zone (HCZ) extends below the conductive
dikes at depths between 10 and 35 km, with a N-S gradient of
conductivity decreasing from north (<5 Ohm m) to south
(>10 Ohm m; PC in
"presentation of the 3-D model at different depths"). Although the
lower boundary is not well constrained, it could be constrained by
inserting another HCZ at the levels of the oceanic crust (70-90 km
depth at 69°W; Fig.1; right), which is seen to give
an equivalent response under 2-D modelling.
The origin of the fluids in the fractures can be argued in a
similar manner for the PC-fault system as was explained for the Atacama
fault system. The conductive dikes of the upper crust may be fed
by meteoric water trapping from the surface and/or by ore fluids (inferred from
the huge porphyry copper in Chuquicamata at latitude 22°S,
associated with the West Fissure zone; Reutter, 1995). Water
released from fractured hydrated porous rock, remaining from older
metamorphic reactions, can also be a possibility for the brittle
crust.
In the Precordillera however, the rheology and the tectonic
history differ from the crust of the near coast. The last
important compressional deformation in the Precordillera occurred
about 35 Ma ago (Reutter et al., 1995}), when the crust was
thickened subsequently subject to a retrograde metamorphism
(Reutter, pers. comm.). Thermotectonic modeling has shown that a
lithosphere subject to a strong and sudden thickening by
overthrusting will need a long period of time (>100 Ma) to
recover its original thermal state (Thompson, 1981). Within a
period of about 70 Ma the crust can still undergo metamorphic
reactions, adjusting fluid productions Thompson (1990). This
model can be suitable for the Precordillera if we relate the
pressure-temperature diagrams of metamorphic hydrous rocks which
characterize a subduction zone (Peacock et al., 1996) with the
geotherms estimated by Springer (1998) for the Precordillera
(Fig.1). The mid-crust undergoes intermediate
metamorphic reactions (temperatures from 300°C to 550°C) where
greenschists transform to epidote amphibolite
(
fig.1; EA on left diagram) indicating the first appearance of
water, and liberating fluids break down in the absence of partial
melting (Wannamaker, 1986). At greater depths (30-45 km) the crust contains
wet rocks with epidote blueschist or epidotite amphibolite. At the lowest crustal
depths, the P-T diagram indicates a composition of eclogite (dry
rock) for the ductile lower crust of the Precordillera
(Fig.1; left; 45-60 km depth and T=500-600°C), which
does not indicate conductivity enhancement since eclogite can not
retain water.
Along strike variations of volcanic activity:
It is proposed that continuing metamorphic reactions in the mid-crust, which liberate fluids
from cracks and ascend into the fractures of the Precordillera fault system, are the cause of
the conductivity enhancement at mid-crustal levels (10-30 km). In the north the conductivity
is clearly higher than to the south, which may be related to the different volcanic history
known at these latitudes. North of 21.S magmatism ceased about 25 Ma, whereas to the
south volcanism is younger (<10 Ma; de Silva [1989]). If magmatism and tectonic compression
would occurred simultaneously (Victor [2000]), then tectonic overthrusting would have started
at about 10 Ma in the south whereas to the north it would have began ~30 Ma ago (Victor
[2000], pers. comm.). In this manner, according to a thermotectonic model of a thickened
crust by overthrusting that induces a thermal perturbation over time (Thompson [1981]),
metamorphic reactions may evolve under different P-T conditions from north to south in the
Precordillera. This suggests that a distinct production of fluids in the crust might develop
north and south of 21.S. A ~30 Ma thickened crust can lead to a higher production of fluids
(and hence higher electrical conductivity values in the north) than a recently deformed crust
subject to younger metamorphism.
An additional explanation is that in the north, where
magmatism is older (>25 Ma) than in the south (<10 Ma), the crust might be more fractured
due to a cooler and more brittle regime than in the south, allowing the fluids to be better
interconnected and hence the electrical conductivity to be enhanced.
2-D Modelling of the Back-Arc of the Andean Subduction Zone at Latitude 24 S
Figure 2
Fluids flowing in partially molten rocks matrix (of enhanced bulk conductivity)
and beyond cause a reduction of the melting point temperature that can lead to
an expansion of the melting process beyond the existing boundaries. The brittle-
ductile transition zone may be affected when molten rocks are displaced into
deeper zones of higher temperatures.
Fig. 2 shows an
example of seismic attenuation and MT surveys performed in the Central Andes
zone at latitude 24 S. The 2-D resistivity model supports one of the two seismic
attenuation models proposed by Whitman et al. (1992) in the back-arc zone, the former showing a
western upwelling of the electrical asthenosphere in direction to the Puna
volcanism. More recent seismic measurements show the Puna plateau with a zone of
low P velocities and high seismic attenuations (not shown here) at lower crustal
levels. Partial melts and/or magma at crust /upper mantle levels below the Puna
zone is a good candidate to explain the seismic anomalies, confirmed also by
high conductivity values in the mid-low crust modelled from magnetotelluric
sites located west of the MT profile shown here (Lezaeta & Brasse, 2002). Some authors (as Kay & Kay, 1993) support
the well-known hypothesis of upper mantle delamination due to a thickening of
crust of the Puna plateau, causing crustal uplift, asthenospheric upwelling, and
pressure-release melting. Both MT and seismic models support a thinning of the
rheologic lithosphere beneath the Puna, interpreted as an asthenospheric
upwelling due to an increase of mantle temperature according to heat flow
measurements in the area. An upward lithospheric displacement of the brittle-
ductile transition zone beneath the Puna occur, with a ductile -partially
melted- lower crust associated to active magmatism and tectonic deformation. The
asthenospheric upwelling is supported by both high seismic attenuation values
and the temperature dependent electrical conductivity values obtained from
magnetotelluric modelling ( Lezaeta et al., 2001).
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