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Constraints on the model
We ran a variety of models to test the limits that can be placed on the
axial resistivity structure. Of particular interest are the constraints
which can be placed on the mid-crustal low resistivity anomaly. The lowest
reasonable resistivity for the anomalous body is 0.2
, corresponding
to pure basaltic melt at approximately 1300 ° C
(Waff & Weill, 1975). A melt lens of only 100 m thickness and a
width of 4 km, consistent with the lens of very low velocity material
detected seismically (Navin etal , this issue), cannot alone explain the
data. Although there is a radial/azimuthal split for the data from Noddy,
it is not as large as that observed in the data. The magnitude of the radial
field enhancement caused by a low resistivity body increases quickly as
the thickness of the body increases, levelling off for thicknesses greater
than a skin depth (400 m in this case). Increasing the width of the
melt lens up to 9 km improves the fit to the radial fields, but increasing
the width past this results in a degradation of the fit to the azimuthal
fields.
Although the data can be fit using a 400 m thick body of pure melt,
such a large body of melt is incompatible with the seismic data, which suggest
the presence of a much smaller melt lens, surrounded by a wider low velocity
zone (Navin etal, this issue). Since there is a trade off between the size
of the low resistivity zone and the resistivity within it, a body with a
higher resistivity distributed over a wider region is also possible, and
more likely given the seismic constraints. Instead of a thin body of very
low resistivity, a thicker region with a higher resistivity can be used
to explain the data so long as it is at least a skin depth thick. However,
resistivities of 2.5
or lower are required to reproduce the degree
of splitting between the radial and azimuthal fields which is observed,
requiring a thickness of at least 1300 m. The maximum thickness of
the low resistivity anomaly cannot be constrained with the CSEM data, although
the MT results (Heinson etal, this issue) are best fit when the low axial
conductance is confined to the upper 3 km of the crust.
The fit of the response is not adversely affected by varying the depth to
the top of the low resistivity anomaly between 1.8 km and 2.5 km
below the seafloor. Increasing the depth past 2.5 km results in a significant
decrease in the 0.75 Hz response between 5 km and 9 km source
receiver range. When the top of the anomaly is shallower than 1.8 km,
the low resistivity zone severely attenuates fields diffusing through the
axis. In this case the response in the range 9-15 km, corresponding
to the data recorded by Noddy, severely underestimates the observed amplitudes.
The best results are obtained when the width of the 2.5
region is in the
range 7-9 km. If the region is too narrow there is insufficient enhancement
to explain the magnitude of the predominantly radial Quail tow 2 and Noddy
tow 1 data. Increasing the width of the 2.5
region too far results
in response amplitudes which overestimate the magnitude of the Noddy data
from the second source tow.
The minimum width of the structure above the low resistivity anomaly is
constrained by the short range data from Quail. The 11 Hz data in particular
can be adequately fit with a 1-dimensional resistivity structure, implying
that they are not affected by lateral changes in resistivity. In order for
the 11 Hz data to be unaffected by the increase in resistivity with
distance from the axis, the width of the axial region above the mid-crustal
anomaly must be greater than 2 km. Constraint on the maximum width
of the structure above the anomaly comes from examining the off axis ELF
data. Increasing the width of the shallow axial structure results in an
increase in attenuation of fields diffusing through the axis. Since the
fields detected by the ELF instruments have all diffused through the axial
zone, this results in a decrease in all amplitudes. Similarly decreasing
the width results in an increase in the amplitudes. However, a decrease
in attenuation will increase the azimuthal fields more than the radial fields,
reducing the split between the two components. A balance must therefore
be found between the width of the shallow axial structure, which controls
the overall level of the response, and the magnitude of the sub-axial anomaly,
which controls the splitting between the radial and azimuthal components.
The resistivity of the mid-crustal anomalous region in Figure. 7
is chosen to be as as high as possible while still reproducing the features
observed in the data. For this anomaly, the width of the shallow low resistivity
on axis is fairly well constrained at 4-5 km.
Next: Along axis
variability Up: Modelling
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Lucy MacGregor
Fri Aug 15 08:48:04 PDT 1997