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GEOMAGNETISM
F.E.M. (Ted) Lilley
Research during 2003 has focussed on marine science, both in
analysing data from previous experiments, in computations using
global web-based data, and in participation in a research voyage on
the Australian Research Vessel "Southern Surveyor". This voyage also
provided the opportunity of sea-going experience for two RSES
students, Claire Menesguen and Tjipto Prastowo. During the year
progress has also been made in developing methods for the analysis of
magnetotelluric data.
Participation in the Australian Society of Exploration Geophysicists
Convention in Adelaide in February provided an opportunity to present
recent RSES results in geomagnetism to the Australian community, and
to make contact with collaborators in Adelaide. The ASEG meeting in
Adelaide was immediately followed there by an international workshop,
the third on 3D Electromagnetic Induction, which provided further
opportunities for discussion both nationally and internationally.
Collaboration also continued with colleagues in Canada, and Professor
J.T. Weaver visited RSES for some ten days following his
participation in the Adelaide meetings.
Canadian student Ms Karen Weitemeyer worked as a summer research
scholar on various projects at RSES from January to April. She
attended the ASEG meeting in Adelaide, and made major contributions
to a paper presented there.
Dr C.E. Barton, formerly of Geoscience Australia, was welcomed as a
Visiting Fellow in October. Recently elected to a four-year term as
president of the International Association of Geomagnetism and
Aeronomy, he returned to RSES where he was a research student some
quarter of a century earlier.
Research Results
BASIN TECTONICS AND SALT STRUCTURE DELINEATION IN THE
BROWSE-BONAPARTE COMPARTMENTS, TIMOR SEA.
A. White (Flinders University), G. Heinson (University of Adelaide),
S. Donnelley (University of Adelaide), T. Prastowo, C. Menesguen,
F.E.M. Lilley
The sedimentary basins beneath the Timor Sea have very high
hydrocarbon potential and have already become major exploration
areas. Basic structural information on sedimentary basins and salt
structures that are potential hydrocarbon traps has been obtained by
conventional seismic methods. These methods are good at locating the
top of salt structures but have poor sensitivity to lower salt
structures due to reverberation and losses of acoustic energy.
Magnetotelluric (MT) methods, in which natural electromagnetic
variations signals are measured at the seabed, have recently been
found to be highly successful in similar marginal seas at locating
not only the top but also the bottom of the salt diapirs and the
depth to basement, imaging them in terms of electrical conductivity.
This experiment represents a pilot study and some twenty separate MT
deployments were made, the majority for just several days. The MT
instruments were deployed in transects, with spacing of 2-3 km, along
a previous seismic line near the Tern Well in Bonaparte Gulf where
there are salt diapiric structures. The purpose is to develop an
electrical conductivity model for the area which complements and
enhances geological understanding of the salt structures.
The magnetotelluric (MT) instruments free-fall to the sea floor and
record magnetic and electric field fluctuations until they are
accoustically commanded to re-surface. The instruments weigh
approximately 250 kg, and deployment and recovery is by light crane
over the side of the vessel.
Four long-period instruments were deployed at the start of the
cruise, and recovered at the end. For the short-period instruments,
17 deployments were made, and 16 successful recoveries (there was one
loss, thought to be due to interference by a fishing vessel).
In addition to the electromagnetic signals originating external to
Earth and causing electromagnetic induction in the crustal rocks,
oceanographic signals are also present in the observed data, caused
by tidal motion and ocean wave signals.
SEA-SURFACE OBSERVATIONS OF THE MAGNETIC SIGNALS OF OCEAN SWELLS
F. E. M. Lilley, Adrian P. Hitchman, Peter R. Milligan (Geoscience
Australia) and Tina Pedersen
Ocean swells have a magnetic signal, caused by the motional induction
of sea water moving in the steady main magnetic field of Earth. To
check the character of such signals at the sea surface, several years
ago a magnetometer was set free from a ship to float unrestricted on
the surface of the ocean for periods of several days. The path of
the floating magnetometer was tracked by satellite; this procedure
enabled also the eventual recovery of the magnetometer by the ship.
Superimposed upon a background of slow change of magnetic field, as
the magnetometer drifted across different patterns of crustal
magnetisation, are high-frequency signals generated by the strong
ocean swell present at the time. These wave-generated signals are
typically up to 5 nT trough-to-peak, consistent with theory for
their generation by ocean swells several metres trough-to-peak in
height.
The power spectra of the magnetic signals show a consistent peak at
period 13 s, appropriate for the known characteristics of ocean swell
in the area. The power spectra then exhibit a strong (-7 power)
fall-off as period decreases below 13 s. This strong fall-off is
consistent with oceanographic observations of the spectra of surface
swell, combined with motional induction theory.
APPARENT AEROMAGNETIC WAVELENGTHS OF THE MAGNETIC SIGNALS OF OCEAN SWELL
F.E.M. Lilley and Karen A. Weitemeyer
The magnetic signals of ocean swells, caused by the motional
induction of sea water moving in the steady main magnetic field of
Earth, may be sensed by a low-flying aircraft, carrying out
aeromagnetic measurements over the ocean. The apparent spatial
wavelength which such signals will have, when observed data are
plotted out for geological purposes, can vary greatly. It will
depend particularly on the relative speeds and directions of travel
of the observing aircraft and the ocean swells. The apparent
wavelength of the ocean-swell magnetic signal cannot be less than the
actual ocean-swell wavelength. Generally it is greater, and it can
range up to infinity in value. For observations over continental
shelves the situation is complicated by the dependence of the swell
phase-velocity on water depth, so that the swell speed generally
slows as land is approached.
MAGNETOTELLURIC THEORY: THE RELATIONSHIP BETWEEN THE MAGNETOTELLURIC
TENSOR INVARIANTS AND THE PHASE TENSOR OF CALDWELL, BIBBY AND BROWN
J.T. Weaver (University of Victoria, Canada), A.K. Agarwal
(University of Victoria, Canada), F.E.M. Lilley
We examine the relationship between the seven invariants of the
complex MT tensor, which we previously proposed as a vehicle for
testing the dimensionality of the regional conductivity structure
prior to an analysis of MT data, and the three invariants of the real
'phase tensor', recently introduced as an innovative aid in the
treatment of MT data. It is found that the relevant invariants, and
the necessary conditions on them for galvanically distorted data to
be consistent with 1D, 2D or 3D structures, agree in almost every
detail for the two approaches. The new method does lead, however, to
an improved normalisation of the eighth (dependent) invariant
previously introduced. It is shown that the phase tensor can be
expressed as a sum of three simple matrices, clearly associated with
1D, 2D and 3D conductivity structures respectively. It is further
shown that it can be depicted graphically as a single Mohr circle
that retains the principal properties of the separate real and
imaginary Mohr circles associated with the MT tensor. The simplicity
and elegance of the phase tensor method is achieved by dispensing
with the capability of distinguishing between galvanically distorted
and undistorted data in 1D and 2D regions, a distinction that is
ultimately unimportant and unnecessary with real data. The paper
concludes with a simple illustrative example of the theory applied to
a real MT dataset from NE Australia. A shallow 1D regional
conductivity structure associated with a sedimentary basin is
revealed, and a 2D anomaly with a calculated strike angle is also
identified.
TWO-DIMENSIONAL MAGNETOTELLURIC RESPONSES OF THREE-DIMENSIONAL BODIES
K. Broxholme (University of Adelaide), G. Heinson (University of
Adelaide), S. Busuttil (University of Adelaide), F.E.M. Lilley
Magnetotelluric (MT) tensors have significantly different forms
depending on whether the subsurface is one-dimensional (1D),
two-dimensional (2D) or three-dimensional (3D). In subsurface
geological structures that are not 1D, two-dimensionality is often
assumed, as inversion routines for 2D earth models are
computationally more tractable than those for full 3D media. In 2D,
the MT tensor decouples into two independent modes, the transverse
electric (TE) mode and the transverse magnetic (TM) mode. Often only
one of these modes is acquired during commercial operations.
Field data were collected with the Mt Isa Mines Distributed
Acquisition System (MIMDAS) in the Deep Well prospect of the
Curnamona Province in South Australia. The target for the survey was
an elongate magnetic anomaly of a type that would normally be
approximated as 2D but which has a finite strike length and is
therefore a 3D body. With this in mind, the applicability of
interpreting data defined as TE and TM were assessed using (a) Mohr
circles galvanic distortion analyses, (b) determination of strike of
local and regional geology, and (c) comparison of 2D inversion
techniques. We show that the TM mode accurately delineates
boundaries and that since boundary-charges are included in the
inversion formulation, it also provides accurate values of apparent
resistivity. The TE mode provides poor boundary delineation and
underestimates the resistivity of the 3D body. Joint inversions
provide only a small improvement upon TM-only inversions, but
determination of dimensionality, strike and detection of galvanic
distortion mean that collection of both data modes is still
preferable.
Back to the beginning
Questions about this topic to Ted Lilley: Ted.Lilley@anu.edu.au
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